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Sundial
Sundial
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SSW facing, vertical declining sundial on the Moot Hall in Aldeburgh, Suffolk, England. The gnomon is a rod that is very narrow, so it functions as the style. The Latin motto loosely translates as "I only count the sunny hours."
A horizontal dial commissioned in 1862, the gnomon is the triangular blade. The style is its inclined edge.[1]

A sundial is a horological device that tells the time of day (referred to as civil time in modern usage) when direct sunlight shines by the apparent position of the Sun in the sky. In the narrowest sense of the word, it consists of a flat plate (the dial) and a gnomon, which casts a shadow onto the dial. As the Sun appears to move through the sky, the shadow aligns with different hour-lines, which are marked on the dial to indicate the time of day. The style is the time-telling edge of the gnomon, though a single point or nodus may be used. The gnomon casts a broad shadow; the shadow of the style shows the time. The gnomon may be a rod, wire, or elaborately decorated metal casting. The style must be parallel to the axis of the Earth's rotation for the sundial to be accurate throughout the year. The style's angle from horizontal is equal to the sundial's geographical latitude.

The term sundial can refer to any device that uses the Sun's altitude or azimuth (or both) to show the time. Sundials are valued as decorative objects, metaphors, and objects of intrigue and mathematical study.

The passing of time can be observed by placing a stick in the sand or a nail in a board and placing markers at the edge of a shadow or outlining a shadow at intervals. It is common for inexpensive, mass-produced decorative sundials to have incorrectly aligned gnomons, shadow lengths, and hour-lines, which cannot be adjusted to tell the correct time.[2]

Introduction

[edit]

There are several different types of sundials. Some sundials use a shadow or the edge of a shadow while others use a line or spot of light to indicate the time.

The shadow-casting object, known as a gnomon, may be a long thin rod or other object with a sharp tip or a straight edge. Sundials employ many types of gnomon. The gnomon may be fixed or moved according to the season. It may be oriented vertically, horizontally, aligned with the Earth's axis, or oriented in an altogether different direction determined by mathematics.

Given that sundials use light to indicate time, a line of light may be formed by allowing the Sun's rays through a thin slit or focusing them through a cylindrical lens. A spot of light may be formed by allowing the Sun's rays to pass through a small hole, window, oculus, or by reflecting them from a small circular mirror. A spot of light can be as small as a pinhole in a solargraph or as large as the oculus in the Pantheon.

Sundials may also use many types of surfaces to receive the light or shadow. Planes are the most common surface, but partial spheres, cylinders, cones and other shapes have been used for greater accuracy or beauty.

Sundials differ in their portability and their need for orientation. The installation of many dials requires knowing the local latitude, the precise vertical direction (e.g., by a level or plumb-bob), and the direction to true north. Portable dials are self-aligning: for example, they may have two dials that operate on different principles, such as a horizontal and analemmatic dial, mounted together on one plate. In these designs, their times agree only when the plate is aligned properly. [3]

Sundials may indicate the local solar time only. To obtain the national clock time, three corrections are required:

  1. The orbit of the Earth is not perfectly circular and its rotational axis is not perpendicular to its orbit. The sundial's indicated solar time thus varies from clock time by small amounts that change throughout the year. This correction—which may be as great as 16 minutes, 33 seconds—is described by the equation of time. A sophisticated sundial, with a curved style or hour lines, may incorporate this correction. The more usual simpler sundials sometimes have a small plaque that gives the offsets at various times of the year.
  2. The solar time must be corrected for the longitude of the sundial relative to the longitude of the official time zone. For example, an uncorrected sundial located west of Greenwich, England but within the same time-zone, shows an earlier time than the official time. It may show "11:45" at official noon, and will show "noon" after the official noon. This correction can easily be made by rotating the hour-lines by a constant angle equal to the difference in longitudes, which makes this a commonly possible design option.
  3. To adjust for daylight saving time, if applicable, the solar time must additionally be shifted for the official difference (usually one hour). This is also a correction that can be done on the dial, i.e. by numbering the hour-lines with two sets of numbers, or even by swapping the numbering in some designs. More often this is simply ignored, or mentioned on the plaque with the other corrections, if there is one.

Apparent motion of the Sun

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Top view of an equatorial sundial. The hour lines are spaced equally about the circle, and the shadow of the gnomon (a thin cylindrical rod) moving from 3:00 a.m. to 9:00 p.m. on or around Solstice, when the Sun is at its highest declination.

The principles of sundials are understood most easily from the Sun's apparent motion.[4] The Earth rotates on its axis, and revolves in an elliptical orbit around the Sun. An excellent approximation assumes that the Sun revolves around a stationary Earth on the celestial sphere, which rotates every 24 hours about its celestial axis. The celestial axis is the line connecting the celestial poles. Since the celestial axis is aligned with the axis about which the Earth rotates, the angle of the axis with the local horizontal is the local geographical latitude.

Unlike the fixed stars, the Sun changes its position on the celestial sphere, being (in the Northern Hemisphere) at a positive declination in spring and summer, and at a negative declination in autumn and winter, and having exactly zero declination (i.e., being on the celestial equator) at the equinoxes. The Sun's celestial longitude also varies, changing by one complete revolution per year. The path of the Sun on the celestial sphere is called the ecliptic. The ecliptic passes through the twelve constellations of the zodiac in the course of a year.

Bowstring sundial in Singapore Botanic Gardens. The design shows that Singapore is located almost at the equator.

This model of the Sun's motion helps to understand sundials. If the shadow-casting gnomon is aligned with the celestial poles, its shadow will revolve at a constant rate, and this rotation will not change with the seasons. This is the most common design. In such cases, the same hour lines may be used throughout the year. The hour-lines will be spaced uniformly if the surface receiving the shadow is either perpendicular (as in the equatorial sundial) or circular about the gnomon (as in the armillary sphere).

In other cases, the hour-lines are not spaced evenly, even though the shadow rotates uniformly. If the gnomon is not aligned with the celestial poles, even its shadow will not rotate uniformly, and the hour lines must be corrected accordingly. The rays of light that graze the tip of a gnomon, or which pass through a small hole, or reflect from a small mirror, trace out a cone aligned with the celestial poles. The corresponding light-spot or shadow-tip, if it falls onto a flat surface, will trace out a conic section, such as a hyperbola, ellipse or (at the North or South Poles) a circle.

This conic section is the intersection of the cone of light rays with the flat surface. This cone and its conic section change with the seasons, as the Sun's declination changes; hence, sundials that follow the motion of such light-spots or shadow-tips often have different hour-lines for different times of the year. This is seen in shepherd's dials, sundial rings, and vertical gnomons such as obelisks. Alternatively, sundials may change the angle or position (or both) of the gnomon relative to the hour lines, as in the analemmatic dial or the Lambert dial.

History

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World's oldest sundial, from Egypt's Valley of the Kings (c. 1500 BC)

The earliest sundials known from the archaeological record are shadow clocks (1500 BC or BCE) from ancient Egyptian astronomy and Babylonian astronomy. By 240 BC, Eratosthenes had estimated the circumference of the world using an obelisk and a water well and a few centuries later, Ptolemy had charted the latitude of cities using the angle of the sun. The people of Kush created sun dials through geometry.[5][6] The Roman writer Vitruvius lists dials and shadow clocks known at that time in his De architectura. The Tower of the Winds in Athens included both a sundial and a water clock for telling time. A canonical sundial is one that indicates the canonical hours of liturgical acts, and these were used from the 7th to the 14th centuries by religious orders. The Italian astronomer Giovanni Padovani published a treatise on the sundial in 1570, in which he included instructions for the manufacture and laying out of mural (vertical) and horizontal sundials. Giuseppe Biancani's Constructio instrumenti ad horologia solaria (c. 1620) discusses how to make a perfect sundial. They have been in common use since the 16th century.

A Korean sundial (Angbu-ilgu) first made by Chang Yŏngsil in the Joseon period, displayed in Gyeongbokgung.

Functioning

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A London type horizontal dial. The western edge of the gnomon is used as the style before noon, the eastern edge after that time. The changeover causes a discontinuity, the noon gap, in the time scale.

In general, sundials indicate the time by casting a shadow or throwing light onto a surface known as a dial face or dial plate. Although usually a flat plane, the dial face may also be the inner or outer surface of a sphere, cylinder, cone, helix, and various other shapes.

The time is indicated where a shadow or light falls on the dial face, which is usually inscribed with hour lines. Although usually straight, these hour lines may also be curved, depending on the design of the sundial (see below). In some designs, it is possible to determine the date of the year, or it may be required to know the date to find the correct time. In such cases, there may be multiple sets of hour lines for different months, or there may be mechanisms for setting/calculating the month. In addition to the hour lines, the dial face may offer other data—such as the horizon, the equator and the tropics—which are referred to collectively as the dial furniture.

The entire object that casts a shadow or light onto the dial face is known as the sundial's gnomon.[7] However, it is usually only an edge of the gnomon (or another linear feature) that casts the shadow used to determine the time; this linear feature is known as the sundial's style. The style is usually aligned parallel to the axis of the celestial sphere, and therefore is aligned with the local geographical meridian. In some sundial designs, only a point-like feature, such as the tip of the style, is used to determine the time and date; this point-like feature is known as the sundial's nodus.[7][a] Some sundials use both a style and a nodus to determine the time and date.

The gnomon is usually fixed relative to the dial face, but not always; in some designs such as the analemmatic sundial, the style is moved according to the month. If the style is fixed, the line on the dial plate perpendicularly beneath the style is called the substyle,[7] meaning "below the style". The angle the style makes with the plane of the dial plate is called the substyle height, an unusual use of the word height to mean an angle. On many wall dials, the substyle is not the same as the noon line (see below). The angle on the dial plate between the noon line and the substyle is called the substyle distance, an unusual use of the word distance to mean an angle.

By tradition, many sundials have a motto. The motto is usually in the form of an epigram: sometimes sombre reflections on the passing of time and the brevity of life, but equally often humorous witticisms of the dial maker. One such quip is, I am a sundial, and I make a botch, Of what is done much better by a watch.[8]

A dial is said to be equiangular if its hour-lines are straight and spaced equally. Most equiangular sundials have a fixed gnomon style aligned with the Earth's rotational axis, as well as a shadow-receiving surface that is symmetrical about that axis; examples include the equatorial dial, the equatorial bow, the armillary sphere, the cylindrical dial and the conical dial. However, other designs are equiangular, such as the Lambert dial, a version of the analemmatic sundial with a moveable style.

In the Southern Hemisphere

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Southern Hemisphere sundial in Perth, Australia. Magnify to see that the hour marks run anticlockwise. Note graph above the gnomon of the Equation of Time, needed to correct sundial readings.

A sundial at a particular latitude in one hemisphere must be reversed for use at the opposite latitude in the other hemisphere.[9] A vertical direct south sundial in the Northern Hemisphere becomes a vertical direct north sundial in the Southern Hemisphere. To position a horizontal sundial correctly, one has to find true north or south. The same process can be used to do both.[10] The gnomon, set to the correct latitude, has to point to the true south in the Southern Hemisphere as in the Northern Hemisphere it has to point to the true north.[11] The hour numbers also run in opposite directions, so on a horizontal dial they run anticlockwise (US: counterclockwise) rather than clockwise.[12]

Sundials which are designed to be used with their plates horizontal in one hemisphere can be used with their plates vertical at the complementary latitude in the other hemisphere. For example, the illustrated sundial in Perth, Australia, which is at latitude 32° South, would function properly if it were mounted on a south-facing vertical wall at latitude 58° (i.e. 90° − 32°) North, which is slightly further north than Perth, Scotland. The surface of the wall in Scotland would be parallel with the horizontal ground in Australia (ignoring the difference of longitude), so the sundial would work identically on both surfaces. Correspondingly, the hour marks, which run counterclockwise on a horizontal sundial in the Southern Hemisphere, also do so on a vertical sundial in the Northern Hemisphere. (See the first two illustrations at the top of this article.) On horizontal Northern Hemisphere sundials, and on vertical Southern Hemisphere ones, the hour marks run clockwise.

Adjustments to calculate clock time from a sundial reading

[edit]

The most common reason for a sundial to differ greatly from clock time is that the sundial has not been oriented correctly or its hour lines have not been drawn correctly. For example, most commercial sundials are designed as horizontal sundials as described above. To be accurate, such a sundial must have been designed for the local geographical latitude and its style must be parallel to the Earth's rotational axis; the style must be aligned with true north and its height (its angle with the horizontal) must equal the local latitude. To adjust the style height, the sundial can often be tilted slightly "up" or "down" while maintaining the style's north-south alignment.[13]

Summer (daylight saving) time correction

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Some areas of the world practice daylight saving time, which changes the official time, usually by one hour. This shift must be added to the sundial's time to make it agree with the official time.

Time-zone (longitude) correction

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A standard time zone covers roughly 15° of longitude, so any point within that zone which is not on the reference longitude (generally a multiple of 15°) will experience a difference from standard time that is equal to 4 minutes of time per degree. For illustration, sunsets and sunrises are at a much later "official" time at the western edge of a time-zone, compared to sunrise and sunset times at the eastern edge. If a sundial is located at, say, a longitude 5° west of the reference longitude, then its time will read 20 minutes slow, since the Sun appears to revolve around the Earth at 15° per hour. This is a constant correction throughout the year. For equiangular dials such as equatorial, spherical or Lambert dials, this correction can be made by rotating the dial surface by an angle equaling the difference in longitude, without changing the gnomon position or orientation. However, this method does not work for other dials, such as a horizontal dial; the correction must be applied by the viewer.

However, for political and practical reasons, time-zone boundaries have been skewed. At their most extreme, time zones can cause official noon, including daylight savings, to occur up to three hours early (in which case the Sun is actually on the meridian at official clock time of 3 PM). This occurs in the far west of Alaska, China, and Spain. For more details and examples, see time zones.

Equation of time correction

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The Equation of Time – above the axis the equation of time is positive, and a sundial will appear fast relative to a clock showing local mean time. The opposites are true below the axis.
The Whitehurst & Son sundial made in 1812, with a circular scale showing the equation of time correction. This is now on display in the Derby Museum.

Although the Sun appears to rotate uniformly about the Earth, in reality this motion is not perfectly uniform. This is due to the eccentricity of the Earth's orbit (the fact that the Earth's orbit about the Sun is not perfectly circular, but slightly elliptical) and the tilt (obliquity) of the Earth's rotational axis relative to the plane of its orbit. Therefore, sundial time varies from standard clock time. On four days of the year, the correction is effectively zero. However, on others, it can be as much as a quarter-hour early or late. The amount of correction is described by the equation of time. This correction is equal worldwide: it does not depend on the local latitude or longitude of the observer's position. It does, however, change over long periods of time, (centuries or more,[14]) because of slow variations in the Earth's orbital and rotational motions. Therefore, tables and graphs of the equation of time that were made centuries ago are now significantly incorrect. The reading of an old sundial should be corrected by applying the present-day equation of time, not one from the period when the dial was made.

In some sundials, the equation of time correction is provided as an informational plaque affixed to the sundial, for the observer to calculate. In more sophisticated sundials the equation can be incorporated automatically. For example, some equatorial bow sundials are supplied with a small wheel that sets the time of year; this wheel in turn rotates the equatorial bow, offsetting its time measurement. In other cases, the hour lines may be curved, or the equatorial bow may be shaped like a vase, which exploits the changing altitude of the sun over the year to effect the proper offset in time.[15]

A heliochronometer is a precision sundial first devised in about 1763 by Philipp Hahn and improved by Abbé Guyoux in about 1827.[16] It corrects apparent solar time to mean solar time or another standard time. Heliochronometers usually indicate the minutes to within 1 minute of Universal Time.

Sunquest sundial, designed by Richard L. Schmoyer, at the Mount Cuba Observatory in Greenville, Delaware.

The Sunquest sundial, designed by Richard L. Schmoyer in the 1950s, uses an analemmic-inspired gnomon to cast a shaft of light onto an equatorial time-scale crescent. Sunquest is adjustable for latitude and longitude, automatically correcting for the equation of time, rendering it "as accurate as most pocket watches".[17][18][19][20]

Similarly, in place of the shadow of a gnomon the sundial at Miguel Hernández University uses the solar projection of a graph of the equation of time intersecting a time scale to display clock time directly.

Sundial on the Orihuela Campus of Miguel Hernández University, Spain, which uses a projected graph of the equation of time within the shadow to indicate clock time.

An analemma may be added to many types of sundials to correct apparent solar time to mean solar time or another standard time. These usually have hour lines shaped like "figure eights" (analemmas) according to the equation of time. This compensates for the slight eccentricity in the Earth's orbit and the tilt of the Earth's axis that causes up to a 15 minute variation from mean solar time. This is a type of dial furniture seen on more complicated horizontal and vertical dials.

Prior to the invention of accurate clocks, in the mid 17th century, sundials were the only timepieces in common use, and were considered to tell the "right" time. The equation of time was not used. After the invention of good clocks, sundials were still considered to be correct, and clocks usually incorrect. The equation of time was used in the opposite direction from today, to apply a correction to the time shown by a clock to make it agree with sundial time. Some elaborate "equation clocks", such as one made by Joseph Williamson in 1720, incorporated mechanisms to do this correction automatically. (Williamson's clock may have been the first-ever device to use a differential gear.) Only after about 1800 was uncorrected clock time considered to be "right", and sundial time usually "wrong", so the equation of time became used as it is today.[21]

With fixed axial gnomon

[edit]

The most commonly observed sundials are those in which the shadow-casting style is fixed in position and aligned with the Earth's rotational axis, being oriented with true north and south, and making an angle with the horizontal equal to the geographical latitude. This axis is aligned with the celestial poles, which is closely, but not perfectly, aligned with the pole star Polaris. For illustration, the celestial axis points vertically at the true North Pole, whereas it points horizontally on the equator. The world's largest axial gnomon sundial is the mast of the Sundial Bridge at Turtle Bay in Redding, California . A formerly world's largest gnomon is at Jaipur, raised 26°55′ above horizontal, reflecting the local latitude.[22]

On any given day, the Sun appears to rotate uniformly about this axis, at about 15° per hour, making a full circuit (360°) in 24 hours. A linear gnomon aligned with this axis will cast a sheet of shadow (a half-plane) that, falling opposite to the Sun, likewise rotates about the celestial axis at 15° per hour. The shadow is seen by falling on a receiving surface that is usually flat, but which may be spherical, cylindrical, conical or of other shapes. If the shadow falls on a surface that is symmetrical about the celestial axis (as in an armillary sphere, or an equatorial dial), the surface-shadow likewise moves uniformly; the hour-lines on the sundial are equally spaced. However, if the receiving surface is not symmetrical (as in most horizontal sundials), the surface shadow generally moves non-uniformly and the hour-lines are not equally spaced; one exception is the Lambert dial described below.

Some types of sundials are designed with a fixed gnomon that is not aligned with the celestial poles like a vertical obelisk. Such sundials are covered below under the section, "Nodus-based sundials".

Empirical hour-line marking

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The formulas shown in the paragraphs below allow the positions of the hour-lines to be calculated for various types of sundial. In some cases, the calculations are simple; in others they are extremely complicated. There is an alternative, simple method of finding the positions of the hour-lines which can be used for many types of sundial, and saves a lot of work in cases where the calculations are complex.[23] This is an empirical procedure in which the position of the shadow of the gnomon of a real sundial is marked at hourly intervals. The equation of time must be taken into account to ensure that the positions of the hour-lines are independent of the time of year when they are marked. An easy way to do this is to set a clock or watch so it shows "sundial time"[b] which is standard time,[c] plus the equation of time on the day in question.[d] The hour-lines on the sundial are marked to show the positions of the shadow of the style when this clock shows whole numbers of hours, and are labelled with these numbers of hours. For example, when the clock reads 5:00, the shadow of the style is marked, and labelled "5" (or "V" in Roman numerals). If the hour-lines are not all marked in a single day, the clock must be adjusted every day or two to take account of the variation of the equation of time.

Equatorial sundials

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Timepiece, St Katharine Docks, London (1973) an equinoctial dial by Wendy Taylor[25]
An equatorial sundial in the Forbidden City, Beijing. 39°54′57″N 116°23′25″E / 39.9157°N 116.3904°E / 39.9157; 116.3904 (Forbidden City equatorial sundial) The gnomon points true north and its angle with horizontal equals the local latitude. Closer inspection of the full-size image reveals the "spider-web" of date rings and hour-lines.

The distinguishing characteristic of the equatorial dial (also called the equinoctial dial) is the planar surface that receives the shadow, which is exactly perpendicular to the gnomon's style.[26] This plane is called equatorial, because it is parallel to the equator of the Earth and of the celestial sphere. If the gnomon is fixed and aligned with the Earth's rotational axis, the sun's apparent rotation about the Earth casts a uniformly rotating sheet of shadow from the gnomon; this produces a uniformly rotating line of shadow on the equatorial plane. Since the Earth rotates 360° in 24 hours, the hour-lines on an equatorial dial are all spaced 15° apart (360/24).

The uniformity of their spacing makes this type of sundial easy to construct. If the dial plate material is opaque, both sides of the equatorial dial must be marked, since the shadow will be cast from below in winter and from above in summer. With translucent dial plates (e.g. glass) the hour angles need only be marked on the sun-facing side, although the hour numberings (if used) need be made on both sides of the dial, owing to the differing hour schema on the sun-facing and sun-backing sides.

Another major advantage of this dial is that equation of time (EoT) and daylight saving time (DST) corrections can be made by simply rotating the dial plate by the appropriate angle each day. This is because the hour angles are equally spaced around the dial. For this reason, an equatorial dial is often a useful choice when the dial is for public display and it is desirable to have it show the true local time to reasonable accuracy. The EoT correction is made via the relation

Near the equinoxes in spring and autumn, the sun moves on a circle that is nearly the same as the equatorial plane; hence, no clear shadow is produced on the equatorial dial at those times of year, a drawback of the design.

A nodus is sometimes added to equatorial sundials, which allows the sundial to tell the time of year. On any given day, the shadow of the nodus moves on a circle on the equatorial plane, and the radius of the circle measures the declination of the sun. The ends of the gnomon bar may be used as the nodus, or some feature along its length. An ancient variant of the equatorial sundial has only a nodus (no style) and the concentric circular hour-lines are arranged to resemble a spider-web.[27]

Horizontal sundials

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Horizontal sundial in Minnesota. June 17, 2007 at 12:21. 44°51′39.3″N, 93°36′58.4″W

In the horizontal sundial (also called a garden sundial), the plane that receives the shadow is aligned horizontally, rather than being perpendicular to the style as in the equatorial dial.[28] Hence, the line of shadow does not rotate uniformly on the dial face; rather, the hour lines are spaced according to the rule.[29]

Or in other terms:

where L is the sundial's geographical latitude (and the angle the gnomon makes with the dial plate), is the angle between a given hour-line and the noon hour-line (which always points towards true north) on the plane, and t is the number of hours before or after noon. For example, the angle of the 3 PM hour-line would equal the arctangent of sin L , since tan 45° = 1. When (at the North Pole), the horizontal sundial becomes an equatorial sundial; the style points straight up (vertically), and the horizontal plane is aligned with the equatorial plane; the hour-line formula becomes as for an equatorial dial. A horizontal sundial at the Earth's equator, where would require a (raised) horizontal style and would be an example of a polar sundial (see below).

Detail of horizontal sundial outside Kew Palace in London, United Kingdom

The chief advantages of the horizontal sundial are that it is easy to read, and the sunlight lights the face throughout the year. All the hour-lines intersect at the point where the gnomon's style crosses the horizontal plane. Since the style is aligned with the Earth's rotational axis, the style points true north and its angle with the horizontal equals the sundial's geographical latitude L . A sundial designed for one latitude can be adjusted for use at another latitude by tilting its base upwards or downwards by an angle equal to the difference in latitude. For example, a sundial designed for a latitude of 40° can be used at a latitude of 45°, if the sundial plane is tilted upwards by 5°, thus aligning the style with the Earth's rotational axis. [citation needed]

Many ornamental sundials are designed to be used at 45 degrees north. Some mass-produced garden sundials fail to correctly calculate the hourlines and so can never be corrected. A local standard time zone is nominally 15 degrees wide, but may be modified to follow geographic or political boundaries. A sundial can be rotated around its style (which must remain pointed at the celestial pole) to adjust to the local time zone. In most cases, a rotation in the range of 7.5° east to 23° west suffices. This will introduce error in sundials that do not have equal hour angles. To correct for daylight saving time, a face needs two sets of numerals or a correction table. An informal standard is to have numerals in hot colors for summer, and in cool colors for winter.[citation needed] Since the hour angles are not evenly spaced, the equation of time corrections cannot be made via rotating the dial plate about the gnomon axis. These types of dials usually have an equation of time correction tabulation engraved on their pedestals or close by. Horizontal dials are commonly seen in gardens, churchyards and in public areas.

Vertical sundials

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Two vertical dials at Houghton Hall (Norfolk, UK) 52°49′39″N 0°39′27″E / 52.827469°N 0.657616°E / 52.827469; 0.657616 (Houghton Hall vertical sundials). The left and right dials face south and east, respectively. Both styles are parallel, their angle to the horizontal equaling the latitude. The east-facing dial is a polar dial with parallel hour-lines, the dial-face being parallel to the style.

In the common vertical dial, the shadow-receiving plane is aligned vertically; as usual, the gnomon's style is aligned with the Earth's axis of rotation.[30] As in the horizontal dial, the line of shadow does not move uniformly on the face; the sundial is not equiangular. If the face of the vertical dial points directly south, the angle of the hour-lines is instead described by the formula:[31]

where L is the sundial's geographical latitude, is the angle between a given hour-line and the noon hour-line (which always points due north) on the plane, and t is the number of hours before or after noon. For example, the angle of the 3 P.M. hour-line would equal the arctangent of cos L , since tan 45° = 1 . The shadow moves counter-clockwise on a south-facing vertical dial, whereas it runs clockwise on horizontal and equatorial north-facing dials.

Dials with faces perpendicular to the ground and which face directly south, north, east, or west are called vertical direct dials.[32] It is widely believed, and stated in respectable publications, that a vertical dial cannot receive more than twelve hours of sunlight a day, no matter how many hours of daylight there are.[33] However, there is an exception. Vertical sundials in the tropics which face the nearer pole (e.g. north facing in the zone between the Equator and the Tropic of Cancer) can actually receive sunlight for more than 12 hours from sunrise to sunset for a short period around the time of the summer solstice. For example, at latitude 20° North, on June 21, the sun shines on a north-facing vertical wall for 13 hours, 21 minutes.[34] Vertical sundials which do not face directly south (in the northern hemisphere) may receive significantly less than twelve hours of sunlight per day, depending on the direction they do face, and on the time of year. For example, a vertical dial that faces due East can tell time only in the morning hours; in the afternoon, the sun does not shine on its face. Vertical dials that face due East or West are polar dials, which will be described below. Vertical dials that face north are uncommon, because they tell time only during the spring and summer, and do not show the midday hours except in tropical latitudes (and even there, only around midsummer). For non-direct vertical dials – those that face in non-cardinal directions – the mathematics of arranging the style and the hour-lines becomes more complicated; it may be easier to mark the hour lines by observation, but the placement of the style, at least, must be calculated first; such dials are said to be declining dials.[35]

"Double" sundials in Nové Město nad Metují, Czech Republic; the observer is facing almost due north.

Vertical dials are commonly mounted on the walls of buildings, such as town-halls, cupolas and church-towers, where they are easy to see from far away. In some cases, vertical dials are placed on all four sides of a rectangular tower, providing the time throughout the day. The face may be painted on the wall, or displayed in inlaid stone; the gnomon is often a single metal bar, or a tripod of metal bars for rigidity. If the wall of the building faces toward the south, but does not face due south, the gnomon will not lie along the noon line, and the hour lines must be corrected. Since the gnomon's style must be parallel to the Earth's axis, it always "points" true north and its angle with the horizontal will equal the sundial's geographical latitude; on a direct south dial, its angle with the vertical face of the dial will equal the colatitude, or 90° minus the latitude.[36]

Polar dials

[edit]
Polar sundial at Melbourne Planetarium
Monumental polar sundial in Lalín (Spain)

In polar dials, the shadow-receiving plane is aligned parallel to the gnomon-style.[37] Thus, the shadow slides sideways over the surface, moving perpendicularly to itself as the Sun rotates about the style. As with the gnomon, the hour-lines are all aligned with the Earth's rotational axis. When the Sun's rays are nearly parallel to the plane, the shadow moves very quickly and the hour lines are spaced far apart. The direct East- and West-facing dials are examples of a polar dial. However, the face of a polar dial need not be vertical; it need only be parallel to the gnomon. Thus, a plane inclined at the angle of latitude (relative to horizontal) under the similarly inclined gnomon will be a polar dial. The perpendicular spacing X of the hour-lines in the plane is described by the formula

where H is the height of the style above the plane, and t is the time (in hours) before or after the center-time for the polar dial. The center time is the time when the style's shadow falls directly down on the plane; for an East-facing dial, the center time will be 6 A.M., for a West-facing dial, this will be 6 P.M., and for the inclined dial described above, it will be noon. When t approaches ±6 hours away from the center time, the spacing X diverges to +∞; this occurs when the Sun's rays become parallel to the plane.

Vertical declining dials

[edit]
Effect of declining on a sundial's hour-lines. A vertical dial, at a latitude of 51° N, designed to face due south (far left) shows all the hours from 6 A.M. to 6 P.M., and has converging hour-lines symmetrical about the noon hour-line. By contrast, a West-facing dial (far right) is polar, with parallel hour lines, and shows only hours after noon. At the intermediate orientations of south-southwest, southwest, and west-southwest, the hour lines are asymmetrical about noon, with the morning hour-lines ever more widely spaced.
Two sundials, a large and a small one, at Fatih Mosque, Istanbul, dating back to the late 16th century. It is on the southwest facade with an azimuth angle of 52° N.

A declining dial is any non-horizontal, planar dial that does not face in a cardinal direction, such as (true) north, south, east or west.[38] As usual, the gnomon's style is aligned with the Earth's rotational axis, but the hour-lines are not symmetrical about the noon hour-line. For a vertical dial, the angle between the noon hour-line and another hour-line is given by the formula below. Note that is defined positive in the clockwise sense w.r.t. the upper vertical hour angle; and that its conversion to the equivalent solar hour requires careful consideration of which quadrant of the sundial that it belongs in.[39]

where is the sundial's geographical latitude; t is the time before or after noon; is the angle of declination from true south, defined as positive when east of south; and is a switch integer for the dial orientation. A partly south-facing dial has an value of +1  ; those partly north-facing, a value of −1 . When such a dial faces south (), this formula reduces to the formula given above for vertical south-facing dials, i.e.

When a sundial is not aligned with a cardinal direction, the substyle of its gnomon is not aligned with the noon hour-line. The angle between the substyle and the noon hour-line is given by the formula[39]

If a vertical sundial faces trUe south Or north ( or respectively), the angle and the substyle is aligned with the noon hour-line.

The height of the gnomon, that is the angle the style makes to the plate, is given by :

[40]

Reclining dials

[edit]
Vertical reclining dial in the Southern Hemisphere, facing due north, with hyperbolic declination lines and hour lines. Ordinary vertical sundial at this latitude (between tropics) could not produce a declination line for the summer solstice. This particular sundial is located at the Valongo Observatory of the Federal University of Rio de Janeiro, Brazil.

The sundials described above have gnomons that are aligned with the Earth's rotational axis and cast their shadow onto a plane. If the plane is neither vertical nor horizontal nor equatorial, the sundial is said to be reclining or inclining.[41] Such a sundial might be located on a south-facing roof, for example. The hour-lines for such a sundial can be calculated by slightly correcting the horizontal formula above[42][43]

where is the desired angle of reclining relative to the local vertical, L is the sundial's geographical latitude, is the angle between a given hour-line and the noon hour-line (which always points due north) on the plane, and t is the number of hours before or after noon. For example, the angle of the 3pm hour-line would equal the arctangent of cos( L + R ) , since tan 45° = 1 . When R = 0° (in other words, a south-facing vertical dial), we obtain the vertical dial formula above.

Some authors use a more specific nomenclature to describe the orientation of the shadow-receiving plane. If the plane's face points downwards towards the ground, it is said to be proclining or inclining, whereas a dial is said to be reclining when the dial face is pointing away from the ground. Many authors also often refer to reclined, proclined and inclined sundials in general as inclined sundials. It is also common in the latter case to measure the angle of inclination relative to the horizontal plane on the sun side of the dial. In such texts, since the hour angle formula will often be seen written as :

The angle between the gnomon style and the dial plate, B, in this type of sundial is :

or :

Declining-reclining dials/ Declining-inclining dials

[edit]

Some sundials both decline and recline, in that their shadow-receiving plane is not oriented with a cardinal direction (such as true north or true south) and is neither horizontal nor vertical nor equatorial. For example, such a sundial might be found on a roof that was not oriented in a cardinal direction.

The formulae describing the spacing of the hour-lines on such dials are rather more complicated than those for simpler dials.

There are various solution approaches, including some using the methods of rotation matrices, and some making a 3D model of the reclined-declined plane and its vertical declined counterpart plane, extracting the geometrical relationships between the hour angle components on both these planes and then reducing the trigonometric algebra.[44]

One system of formulas for Reclining-Declining sundials: (as stated by Fennewick)[45]

The angle between the noon hour-line and another hour-line is given by the formula below. Note that advances counterclockwise with respect to the zero hour angle for those dials that are partly south-facing and clockwise for those that are north-facing.

within the parameter ranges : and

Or, if preferring to use inclination angle, rather than the reclination, where  :

within the parameter ranges : and

Here is the sundial's geographical latitude; is the orientation switch integer; t is the time in hours before or after noon; and and are the angles of reclination and declination, respectively. Note that is measured with reference to the vertical. It is positive when the dial leans back towards the horizon behind the dial and negative when the dial leans forward to the horizon on the Sun's side. Declination angle is defined as positive when moving east of true south. Dials facing fully or partly south have while those partly or fully north-facing have an Since the above expression gives the hour angle as an arctangent function, due consideration must be given to which quadrant of the sundial each hour belongs to before assigning the correct hour angle.

Unlike the simpler vertical declining sundial, this type of dial does not always show hour angles on its sunside face for all declinations between east and west. When a Northern Hemisphere partly south-facing dial reclines back (i.e. away from the Sun) from the vertical, the gnomon will become co-planar with the dial plate at declinations less than due east or due west. Likewise for Southern Hemisphere dials that are partly north-facing. Were these dials reclining forward, the range of declination would actually exceed due east and due west. In a similar way, Northern Hemisphere dials that are partly north-facing and Southern Hemisphere dials that are south-facing, and which lean forward toward their upward pointing gnomons, will have a similar restriction on the range of declination that is possible for a given reclination value. The critical declination is a geometrical constraint which depends on the value of both the dial's reclination and its latitude :

As with the vertical declined dial, the gnomon's substyle is not aligned with the noon hour-line. The general formula for the angle between the substyle and the noon-line is given by :

The angle between the style and the plate is given by :

Note that for i.e. when the gnomon is coplanar with the dial plate, we have :

i.e. when the critical declination value.[45]

Empirical method

[edit]

Because of the complexity of the above calculations, using them for the practical purpose of designing a dial of this type is difficult and prone to error. It has been suggested that it is better to locate the hour lines empirically, marking the positions of the shadow of a style on a real sundial at hourly intervals as shown by a clock and adding/deducting that day's equation of time adjustment.[23] See Empirical hour-line marking, above.

Spherical sundials

[edit]
Equatorial bow sundial in Hasselt, Belgium 50°55′47″N 5°20′31″E / 50.92972°N 5.34194°E / 50.92972; 5.34194 (Hasselt equatorial bow sundial). The rays pass through the narrow slot, forming a uniformly rotating sheet of light that falls on the circular bow. The hour-lines are equally spaced; in this image, the local solar time is roughly 15:00 hours ( 3 P.M. ). On September 10, a small ball, welded into the slot casts a shadow on centre of the hour band.

The surface receiving the shadow need not be a plane, but can have any shape, provided that the sundial maker is willing to mark the hour-lines. If the style is aligned with the Earth's rotational axis, a spherical shape is convenient since the hour-lines are equally spaced, as they are on the equatorial dial shown here; the sundial is equiangular. This is the principle behind the armillary sphere and the equatorial bow sundial.[46] However, some equiangular sundials – such as the Lambert dial described below – are based on other principles.

In the equatorial bow sundial, the gnomon is a bar, slot or stretched wire parallel to the celestial axis. The face is a semicircle, corresponding to the equator of the sphere, with markings on the inner surface. This pattern, built a couple of meters wide out of temperature-invariant steel invar, was used to keep the trains running on time in France before World War I.[47]

Among the most precise sundials ever made are two equatorial bows constructed of marble found in Yantra mandir.[48] This collection of sundials and other astronomical instruments was built by Maharaja Jai Singh II at his then-new capital of Jaipur, India between 1727 and 1733. The larger equatorial bow is called the Samrat Yantra (The Supreme Instrument); standing at 27 meters, its shadow moves visibly at 1 mm per second, or roughly a hand's breadth (6 cm) every minute.

Cylindrical, conical, and other non-planar sundials

[edit]
Precision sundial in Bütgenbach, Belgium (Precision = ±30 seconds) 50°25′23″N 6°12′06″E / 50.4231°N 6.2017°E / 50.4231; 6.2017 (Belgium)

Other non-planar surfaces may be used to receive the shadow of the gnomon.

As an elegant alternative, the style (which could be created by a hole or slit in the circumference) may be located on the circumference of a cylinder or sphere, rather than at its central axis of symmetry.

In that case, the hour lines are again spaced equally, but at twice the usual angle, due to the geometrical inscribed angle theorem. This is the basis of some modern sundials, but it was also used in ancient times;[e]

In another variation of the polar-axis-aligned cylindrical, a cylindrical dial could be rendered as a helical ribbon-like surface, with a thin gnomon located either along its center or at its periphery.

Movable-gnomon sundials

[edit]

Sundials can be designed with a gnomon that is placed in a different position each day throughout the year. In other words, the position of the gnomon relative to the centre of the hour lines varies. The gnomon need not be aligned with the celestial poles and may even be perfectly vertical (the analemmatic dial). These dials, when combined with fixed-gnomon sundials, allow the user to determine true north with no other aid; the two sundials are correctly aligned if and only if they both show the same time. [citation needed]

Universal equinoctial ring dial

[edit]
Universal ring dial. The dial is suspended from the cord shown in the upper left; the suspension point on the vertical meridian ring can be changed to match the local latitude. The center bar is twisted until a sunray passes through the small hole and falls on the horizontal equatorial ring. See Commons annotations for labels.

A universal equinoctial ring dial (sometimes called a ring dial for brevity, although the term is ambiguous), is a portable version of an armillary sundial,[50] or was inspired by the mariner's astrolabe.[51] It was likely invented by William Oughtred around 1600 and became common throughout Europe.[52]

In its simplest form, the style is a thin slit that allows the Sun's rays to fall on the hour-lines of an equatorial ring. As usual, the style is aligned with the Earth's axis; to do this, the user may orient the dial towards true north and suspend the ring dial vertically from the appropriate point on the meridian ring. Such dials may be made self-aligning with the addition of a more complicated central bar, instead of a simple slit-style. These bars are sometimes an addition to a set of Gemma's rings. This bar could pivot about its end points and held a perforated slider that was positioned to the month and day according to a scale scribed on the bar. The time was determined by rotating the bar towards the Sun so that the light shining through the hole fell on the equatorial ring. This forced the user to rotate the instrument, which had the effect of aligning the instrument's vertical ring with the meridian.

When not in use, the equatorial and meridian rings can be folded together into a small disk.

In 1610, Edward Wright created the sea ring, which mounted a universal ring dial over a magnetic compass. This permitted mariners to determine the time and magnetic variation in a single step.[53]

Analemmatic sundials

[edit]
Analemmatic sundial on a meridian line in the garden of the abbey of Herkenrode in Hasselt (Flanders in Belgium)

Analemmatic sundials are a type of horizontal sundial that has a vertical gnomon and hour markers positioned in an elliptical pattern. There are no hour lines on the dial and the time of day is read on the ellipse. The gnomon is not fixed and must change position daily to accurately indicate time of day. Analemmatic sundials are sometimes designed with a human as the gnomon. Human gnomon analemmatic sundials are not practical at lower latitudes where a human shadow is quite short during the summer months. A 66 inches (170 cm) tall person casts a 4 inches (10 cm) shadow at 27° latitude on the summer solstice.[54]

Foster-Lambert dials

[edit]

The Foster-Lambert dial is another movable-gnomon sundial.[55] In contrast to the elliptical analemmatic dial, the Lambert dial is circular with evenly spaced hour lines, making it an equiangular sundial, similar to the equatorial, spherical, cylindrical and conical dials described above. The gnomon of a Foster-Lambert dial is neither vertical nor aligned with the Earth's rotational axis; rather, it is tilted northwards by an angle α = 45° - (Φ/2), where Φ is the geographical latitude. Thus, a Foster-Lambert dial located at latitude 40° would have a gnomon tilted away from vertical by 25° in a northerly direction. To read the correct time, the gnomon must also be moved northwards by a distance

where R is the radius of the Foster-Lambert dial and δ again indicates the Sun's declination for that time of year.

Altitude-based sundials

[edit]
Ottoman-style sundial with folded gnomon and a compass. Debbane Palace museum, Lebanon.

Altitude dials measure the height of the Sun in the sky, rather than directly measuring its hour-angle about the Earth's axis. They are not oriented towards true north, but rather towards the Sun and generally held vertically. The Sun's elevation is indicated by the position of a nodus, either the shadow-tip of a gnomon, or a spot of light.

In altitude dials, the time is read from where the nodus falls on a set of hour-curves that vary with the time of year. Many such altitude-dials' construction is calculation-intensive, as also the case with many azimuth dials. But the capuchin dials (described below) are constructed and used graphically.

Altitude dials' disadvantages:

Since the Sun's altitude is the same at times equally spaced about noon (e.g., 9am and 3pm), the user had to know whether it was morning or afternoon. At, say, 3:00 pm, that is not a problem. But when the dial indicates a time 15 minutes from noon, the user likely will not have a way of distinguishing 11:45 from 12:15.

Additionally, altitude dials are less accurate near noon, because the sun's altitude is not changing rapidly then.

Many of these dials are portable and simple to use. As is often the case with other sundials, many altitude dials are designed for only one latitude. But the capuchin dial (described below) has a version that's adjustable for latitude.[56]

Mayall & Mayall (1994), p. 169 describe the Universal Capuchin sundial.

Human shadows

[edit]

The length of a human shadow (or of any vertical object) can be used to measure the sun's elevation and, thence, the time.[57] The Venerable Bede gave a table for estimating the time from the length of one's shadow in feet, on the assumption that a monk's height is six times the length of his foot. Such shadow lengths will vary with the geographical latitude and with the time of year. For example, the shadow length at noon is short in summer months, and long in winter months.

Chaucer evokes this method a few times in his Canterbury Tales, as in his Parson's Tale.[f]

An equivalent type of sundial using a vertical rod of fixed length is known as a backstaff dial.

Shepherd's dial – timesticks

[edit]
19th-century Tibetan shepherd's timestick

A shepherd's dial – also known as a shepherd's column dial,[58][59] pillar dial, cylinder dial or chilindre – is a portable cylindrical sundial with a knife-like gnomon that juts out perpendicularly.[60] It is normally dangled from a rope or string so the cylinder is vertical. The gnomon can be twisted to be above a month or day indication on the face of the cylinder. This corrects the sundial for the equation of time. The entire sundial is then twisted on its string so that the gnomon aims toward the Sun, while the cylinder remains vertical. The tip of the shadow indicates the time on the cylinder. The hour curves inscribed on the cylinder permit one to read the time. Shepherd's dials are sometimes hollow, so that the gnomon can fold within when not in use.

The shepherd's dial is evoked in Henry VI, Part 3,[g] among other works of literature.

The cylindrical shepherd's dial can be unrolled into a flat plate. In one simple version,[62] the front and back of the plate each have three columns, corresponding to pairs of months with roughly the same solar declination (June:July, May:August, April:September, March:October, February:November, and January:December). The top of each column has a hole for inserting the shadow-casting gnomon, a peg. Often only two times are marked on the column below, one for noon and the other for mid-morning / mid-afternoon.

Timesticks, clock spear,[58] or shepherds' time stick,[58] are based on the same principles as dials.[58][59] The time stick is carved with eight vertical time scales for a different period of the year, each bearing a time scale calculated according to the relative amount of daylight during the different months of the year. Any reading depends not only on the time of day but also on the latitude and time of year.[59] A peg gnomon is inserted at the top in the appropriate hole or face for the season of the year, and turned to the Sun so that the shadow falls directly down the scale. Its end displays the time.[58]

Ring dials

[edit]

In a ring dial (also known as an Aquitaine or a perforated ring dial), the ring is hung vertically and oriented sideways towards the sun.[63] A beam of light passes through a small hole in the ring and falls on hour-curves that are inscribed on the inside of the ring. To adjust for the equation of time, the hole is usually on a loose ring within the ring so that the hole can be adjusted to reflect the current month.

Card dials (Capuchin dials)

[edit]

Card dials are another form of altitude dial.[64] A card is aligned edge-on with the sun and tilted so that a ray of light passes through an aperture onto a specified spot, thus determining the sun's altitude. A weighted string hangs vertically downwards from a hole in the card, and carries a bead or knot. The position of the bead on the hour-lines of the card gives the time. In more sophisticated versions such as the Capuchin dial, there is only one set of hour-lines, i.e., the hour lines do not vary with the seasons. Instead, the position of the hole from which the weighted string hangs is varied according to the season.

The Capuchin sundials are constructed and used graphically, as opposed the direct hour-angle measurements of horizontal or equatorial dials; or the calculated hour angle lines of some altitude and azimuth dials.

In addition to the ordinary Capuchin dial, there is a universal Capuchin dial, adjustable for latitude.

[edit]
Navicula de Venetiis on display at Musée d'histoire des sciences de la Ville de Genève.

A navicula de Venetiis or "little ship of Venice" was an altitude dial used to tell time and which was shaped like a little ship. The cursor (with a plumb line attached) was slid up / down the mast to the correct latitude. The user then sighted the Sun through the pair of sighting holes at either end of the "ship's deck". The plumb line then marked what hour of the day it was.[citation needed]

Nodus-based sundials

[edit]
Kraków. 50°03′41″N 19°56′24″E / 50.0614°N 19.9400°E / 50.0614; 19.9400 (Kraków sundial) The shadow of the cross-shaped nodus moves along a hyperbola which shows the time of the year, indicated here by the zodiac figures. It is 1:50 P.M. on 16 July, 25 days after the summer solstice.

Another type of sundial follows the motion of a single point of light or shadow, which may be called the nodus. For example, the sundial may follow the sharp tip of a gnomon's shadow, e.g., the shadow-tip of a vertical obelisk (e.g., the Solarium Augusti) or the tip of the horizontal marker in a shepherd's dial. Alternatively, sunlight may be allowed to pass through a small hole or reflected from a small (e.g., coin-sized) circular mirror, forming a small spot of light whose position may be followed. In such cases, the rays of light trace out a cone over the course of a day; when the rays fall on a surface, the path followed is the intersection of the cone with that surface. Most commonly, the receiving surface is a geometrical plane, so that the path of the shadow-tip or light-spot (called declination line) traces out a conic section such as a hyperbola or an ellipse. The collection of hyperbolae was called a pelekonon (axe) by the Greeks, because it resembles a double-bladed ax, narrow in the center (near the noonline) and flaring out at the ends (early morning and late evening hours).

Declination lines at solstices and equinox for sundials, located at different latitudes

There is a simple verification of hyperbolic declination lines on a sundial: the distance from the origin to the equinox line should be equal to harmonic mean of distances from the origin to summer and winter solstice lines.[65]

Nodus-based sundials may use a small hole or mirror to isolate a single ray of light; the former are sometimes called aperture dials. The oldest example is perhaps the antiborean sundial (antiboreum), a spherical nodus-based sundial that faces true north; a ray of sunlight enters from the south through a small hole located at the sphere's pole and falls on the hour and date lines inscribed within the sphere, which resemble lines of longitude and latitude, respectively, on a globe.[66]

Reflection sundials

[edit]

Isaac Newton developed a convenient and inexpensive sundial, in which a small mirror is placed on the sill of a south-facing window.[67] The mirror acts like a nodus, casting a single spot of light on the ceiling. Depending on the geographical latitude and time of year, the light-spot follows a conic section, such as the hyperbolae of the pelikonon. If the mirror is parallel to the Earth's equator, and the ceiling is horizontal, then the resulting angles are those of a conventional horizontal sundial. Using the ceiling as a sundial surface exploits unused space, and the dial may be large enough to be very accurate.

Multiple dials

[edit]

Sundials are sometimes combined into multiple dials. If two or more dials that operate on different principles — such as an analemmatic dial and a horizontal or vertical dial — are combined, the resulting multiple dial becomes self-aligning, most of the time. Both dials need to output both time and declination. In other words, the direction of true north need not be determined; the dials are oriented correctly when they read the same time and declination. However, the most common forms combine dials are based on the same principle and the analemmatic does not normally output the declination of the sun, thus are not self-aligning.[68]

Diptych (tablet) sundial

[edit]
Diptych sundial in the form of a lute, c. 1612. The gnomons-style is a string stretched between a horizontal and vertical face. This sundial also has a small nodus (a bead on the string) that tells time on the hyperbolic pelikinon, just above the date on the vertical face.

The diptych consisted of two small flat faces, joined by a hinge.[69] Diptychs usually folded into little flat boxes suitable for a pocket. The gnomon was a string between the two faces. When the string was tight, the two faces formed both a vertical and horizontal sundial. These were made of white ivory, inlaid with black lacquer markings. The gnomons were black braided silk, linen or hemp string. With a knot or bead on the string as a nodus, and the correct markings, a diptych (really any sundial large enough) can keep a calendar well-enough to plant crops. A common error describes the diptych dial as self-aligning. This is not correct for diptych dials consisting of a horizontal and vertical dial using a string gnomon between faces, no matter the orientation of the dial faces. Since the string gnomon is continuous, the shadows must meet at the hinge; hence, any orientation of the dial will show the same time on both dials.[70]

Multiface dials

[edit]

A common type of multiple dial has sundials on every face of a Platonic solid (regular polyhedron), usually a cube.[71]

Extremely ornate sundials can be composed in this way, by applying a sundial to every surface of a solid object.

In some cases, the sundials are formed as hollows in a solid object, e.g., a cylindrical hollow aligned with the Earth's rotational axis (in which the edges play the role of styles) or a spherical hollow in the ancient tradition of the hemisphaerium or the antiboreum. (See the History section above.) In some cases, these multiface dials are small enough to sit on a desk, whereas in others, they are large stone monuments.

A Polyhedral's dial faces can be designed to give the time for different time-zones simultaneously. Examples include the Scottish sundial of the 17th and 18th centuries, which was often an extremely complex shape of polyhedral, and even convex faces.

Prismatic dials

[edit]

Prismatic dials are a special case of polar dials, in which the sharp edges of a prism of a concave polygon serve as the styles and the sides of the prism receive the shadow.[72] Examples include a three-dimensional cross or star of David on gravestones.

Unusual sundials

[edit]

Benoy dial

[edit]
Benoy Sun Clock showing 6:00 p.m.

The Benoy dial was invented by Walter Gordon Benoy of Collingham, Nottinghamshire, England. Whereas a gnomon casts a sheet of shadow, his invention creates an equivalent sheet of light by allowing the Sun's rays through a thin slit, reflecting them from a long, slim mirror (usually half-cylindrical), or focusing them through a cylindrical lens. Examples of Benoy dials can be found in the United Kingdom at:[73]

Bifilar sundial

[edit]
Stainless steel bifilar sundial in Italy

Invented by the German mathematician Hugo Michnik in 1922, the bifilar sundial has two non-intersecting threads parallel to the dial. Usually the second thread is orthogonal to the first.[75] The intersection of the two threads' shadows gives the local solar time.

Digital sundial

[edit]

A digital sundial indicates the current time with numerals formed by the sunlight striking it. Sundials of this type are installed in the Deutsches Museum in Munich and in the Sundial Park in Genk (Belgium), and a small version is available commercially. There is a patent for this type of sundial.[76]

Globe dial

[edit]

The globe dial is a sphere aligned with the Earth's rotational axis, and equipped with a spherical vane.[77] Similar to sundials with a fixed axial style, a globe dial determines the time from the Sun's azimuthal angle in its apparent rotation about the earth. This angle can be determined by rotating the vane to give the smallest shadow.

Noon marks

[edit]
Noon mark from the Greenwich Royal Observatory. The analemma is the narrow figure-8 shape, which plots the equation of time (in degrees, not time, 1°=4 minutes) versus the altitude of the Sun at noon at the sundial's location. The altitude is measured vertically, the equation of time horizontally.

The simplest sundials do not give the hours, but rather note the exact moment of 12:00 noon.[78] In centuries past, such dials were used to set mechanical clocks, which were sometimes so inaccurate as to lose or gain significant time in a single day. The simplest noon-marks have a shadow that passes a mark. Then, an almanac can translate from local solar time and date to civil time. The civil time is used to set the clock. Some noon-marks include a figure-eight that embodies the equation of time, so that no almanac is needed.

In some U.S. colonial-era houses, a noon-mark might be carved into a floor or windowsill.[79] Such marks indicate local noon, and provide a simple and accurate time reference for households to set their clocks. Some Asian countries had post offices set their clocks from a precision noon-mark. These in turn provided the times for the rest of the society. The typical noon-mark sundial was a lens set above an analemmatic plate. The plate has an engraved figure-eight shape, which corresponds to the equation of time (described above) versus the solar declination. When the edge of the Sun's image touches the part of the shape for the current month, this indicates that it is 12:00 noon.

Sundial cannon

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A sundial cannon, sometimes called a 'meridian cannon', is a specialized sundial that is designed to create an 'audible noonmark', by automatically igniting a quantity of gunpowder at noon. These were novelties rather than precision sundials, sometimes installed in parks in Europe mainly in the late 18th or early 19th centuries. They typically consist of a horizontal sundial, which has in addition to a gnomon a suitably mounted lens, set to focus the rays of the sun at exactly noon on the firing pan of a miniature cannon loaded with gunpowder (but no ball). To function properly the position and angle of the lens must be adjusted seasonally.[citation needed]

Meridian lines

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A meridian line in the Duomo of Milan. The position of the beam of sunlight indicates that it is almost solar noon and the start of Gemini season

A horizontal line aligned on a meridian with a gnomon facing the noon-sun is termed a meridian line and does not indicate the time, but instead the day of the year. Historically they were used to accurately determine the length of the solar year. Examples are the Bianchini meridian line in Santa Maria degli Angeli e dei Martiri in Rome, and the Cassini line in San Petronio Basilica at Bologna.[80]

Sundial mottoes

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The association of sundials with time has inspired their designers over the centuries to display mottoes as part of the design. Often these cast the device in the role of memento mori, inviting the observer to reflect on the transience of the world and the inevitability of death. "Do not kill time, for it will surely kill thee." Other mottoes are more whimsical: "I count only the sunny hours," and "I am a sundial and I make a botch / of what is done far better by a watch." Collections of sundial mottoes have often been published through the centuries.[citation needed]

Use as a compass

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If a horizontal-plate sundial is made for the latitude in which it is being used, and if it is mounted with its plate horizontal and its gnomon pointing to the celestial pole that is above the horizon, then it shows the correct time in apparent solar time. Conversely, if the directions of the cardinal points are initially unknown, but the sundial is aligned so it shows the correct apparent solar time as calculated from the reading of a clock, its gnomon shows the direction of True north or south, allowing the sundial to be used as a compass. The sundial can be placed on a horizontal surface, and rotated about a vertical axis until it shows the correct time. The gnomon will then be pointing to the north, in the northern hemisphere, or to the south in the southern hemisphere. This method is much more accurate than using a watch as a compass and can be used in places where the magnetic declination is large, making a magnetic compass unreliable. An alternative method uses two sundials of different designs. (See #Multiple dials, above.) The dials are attached to and aligned with each other, and are oriented so they show the same time. This allows the directions of the cardinal points and the apparent solar time to be determined simultaneously, without requiring a clock.[citation needed]

See also

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Angbuilgu, a portable sundial used in Korea during the Joseon period. The integrated magnetic compass aligns the instrument toward north pole.(National Museum of Korea)[81]

Notes

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References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
A sundial is a timekeeping device that indicates the time of day by the position of the shadow cast by the Sun on a marked surface, typically divided into hours or fractions of hours. It consists of a flat dial plate inscribed with hour lines and a projecting gnomon—usually a straight rod, triangular fin, or other style—whose shadow moves across the dial as the Sun progresses through the sky. Sundials operate on the principles of solar geometry, relying on the Earth's rotation to track apparent solar time, though their accuracy varies with latitude, season, and orientation. The history of sundials dates back over 3,500 years, with the earliest known examples emerging in ancient Egypt around 1500 BCE as simple shadow clocks or portable devices that divided the sunlit day into segments. By the late fifth century BCE, sundials had evolved from basic meridian lines into more complex instruments used across civilizations, including the Babylonians, Greeks, and Romans, who integrated them into architecture, obelisks, and public spaces for civic timekeeping. In Greco-Roman culture, sundials achieved high precision through designs that accounted for seasonal hours and latitude-specific adjustments, influencing advancements in astronomy and mathematics. Medieval and Renaissance Europe further refined them, often combining sundials with compasses or astrolabes for multifunctional use, while Islamic scholars preserved and enhanced the technology during the Middle Ages. Sundials come in diverse types tailored to different surfaces and environments, including horizontal dials placed flat on the ground or tables, vertical dials mounted on walls, equatorial dials aligned parallel to the celestial equator, polar dials tilted to match the observer's latitude, and analemmatic dials featuring a movable gnomon along an elliptical scale. Other variations, such as cylindrical or ring dials, were popular in portable forms during antiquity, allowing travelers to track time regardless of orientation. Construction materials historically ranged from stone and wood to bronze and marble, with modern examples often using durable metals or ceramics for longevity. Today, while largely superseded by mechanical and digital clocks, sundials retain cultural and educational significance as symbols of humanity's early mastery over time measurement, appearing in gardens, parks, and memorials worldwide. They continue to inspire interest in STEM fields by demonstrating concepts like trigonometry, Earth's tilt, and solar motion, and some contemporary designs incorporate equation-of-time corrections for greater accuracy. As passive, solar-powered instruments requiring no maintenance beyond calibration, sundials embody sustainable timekeeping principles in an era of electronic devices.

Fundamentals

Overview

A sundial is an instrument that indicates the time of day by the position of the shadow cast by the sun on a marked surface. It typically consists of a gnomon, a raised projection such as a rod or style that casts the shadow, and a dial plate, a flat surface engraved with hour lines to denote divisions of the day. This simple mechanism relies on the apparent motion of the sun across the sky to track solar time. The term "sundial" derives from the English words "sun" and "dial," while the ancient Latin equivalent was "solarium," referring to a device for observing the sun. Sundials have demonstrated remarkable ubiquity across human history, serving as primary timekeeping tools in ancient civilizations like Egypt and Rome, where they were installed in public spaces, temples, and private estates, and continuing into modern times as decorative elements in landscapes and structures. Their reliability stems from the predictable path of sunlight in clear weather, allowing accurate readings whenever direct sun is available, though they are inherently limited to daylight hours and ineffective under overcast conditions. Today, sundials maintain cultural and practical significance, often featured in gardens and architectural designs for aesthetic appeal and symbolic reminders of time's passage. They also play an educational role, helping learners grasp concepts of solar time and celestial mechanics through hands-on construction and observation.

Apparent Solar Motion

The apparent motion of the Sun across the sky is primarily due to the Earth's rotation on its axis from west to east, completing one full rotation relative to the fixed stars in approximately 23 hours, 56 minutes, and 4 seconds, known as a sidereal day. This rotation causes the Sun to appear to move from east to west, rising in the east and setting in the west each day. However, because the Earth also orbits the Sun, advancing about 1 degree eastward in its orbit daily, an additional 4 minutes of rotation is required for the Sun to return to the same position relative to the observer's meridian, resulting in an apparent solar day of 24 hours on average. Over the course of a year, the Sun's apparent path deviates from a simple daily circle due to two key factors: the Earth's axial tilt of 23.44 degrees relative to its orbital plane and the slight eccentricity of its elliptical orbit around the Sun (eccentricity ≈ 0.0167). These effects combine to produce the analemma, a figure-eight shaped locus traced by the Sun's position in the sky when observed at the same clock time each day over a full year. The northern loop of the analemma corresponds to the period when the Earth's orbital speed is slower (near aphelion in July), while the southern loop reflects faster orbital motion near perihelion in January; the tilt causes the Sun to reach higher declinations in summer and lower in winter, influencing both the timing and direction of shadows on a sundial. Solar noon occurs when the Sun reaches its highest altitude in the sky, crossing the local meridian and casting the shortest shadow, which aligns due north or south depending on the observer's hemisphere and latitude. A simple experiment demonstrates the Sun's apparent motion using a vertical gnomon, such as a stick placed in the ground. By marking the position of the shadow's tip at regular intervals (for example, every hour) on a sunny day, one can observe that the shadow is longest in the early morning and late afternoon, shortest at solar noon, and moves from west to east, pointing roughly north at noon in the Northern Hemisphere. Typical illustrations of this experiment show a central vertical stick with radiating lines or arcs representing the shadow positions at different times of day (such as 9 AM, 12 PM, and 3 PM), often labeled and accompanied by drawings of the Sun's daily path across the sky. Seasonal variations in the Sun's altitude arise from the axial tilt: in the Northern Hemisphere, the Sun's maximum altitude at noon is lower during winter (e.g., about 26.5 degrees at 40°N latitude on the winter solstice), producing longer midday shadows, while it peaks higher in summer (about 73.5 degrees at the same latitude on the summer solstice), yielding shorter shadows. Sundials inherently track apparent solar time, defined by the actual position of the Sun rather than the uniform mean solar time used in standard clocks, which averages the solar day's length over the year to account for the analemma's variations (up to ±16 minutes). This distinction means sundial readings must often be adjusted for practical use, as apparent solar time fluctuates daily due to the combined effects of orbital eccentricity and obliquity.

Basic Timekeeping

A sundial functions by casting the shadow of a gnomon—a fixed, straight-edged object—onto a marked surface called the dial plate, where the shadow's tip intersects hour lines to indicate the time. As the Sun moves across the sky due to Earth's rotation, the gnomon's shadow traces a path that corresponds to the progression of solar time, with the position of the shadow tip providing a direct reading of the hour. A simple demonstration of this principle is the sun shadow experiment: a vertical stick serving as a gnomon is placed in the ground, and the position of its shadow tip is marked at regular intervals, such as every hour, on a sunny day. In the Northern Hemisphere, the shadow is longest in the morning and late afternoon, shortest at solar noon when it points roughly north, and the tip moves progressively from west to east. These marked positions illustrate the apparent motion of the Sun and can be used to roughly read solar time on subsequent clear days by observing where the shadow tip falls relative to the marks. The day on a sundial is typically divided into 12 hours of daylight, starting from solar noon when the Sun is at its highest point and the shadow aligns with a central meridian line, with hours marked symmetrically on either side for morning and afternoon. In ancient designs, such as those used by the Egyptians around 1500 BCE, these hours were temporal or unequal, varying in length by season to divide the period from sunrise to sunset into 12 parts, longer in summer and shorter in winter. The shadow progresses across the dial in a consistent direction determined by the gnomon's orientation: in the Northern Hemisphere on a horizontal dial facing south, it moves from west to east (clockwise) as the Sun travels from east to west. The shadow shortens toward midday and lengthens afterward as it continues moving clockwise, with the gnomon aligned to true north. Accuracy in timekeeping relies on the gnomon's proper alignment with the observer's latitude; for a horizontal dial, the gnomon is tilted at an angle equal to the latitude to parallel Earth's axis, ensuring the shadow follows the correct path—misalignment introduces systematic errors in hour readings. A simple example is a basic gnomon tilted at the local latitude on a horizontal plate, which displays daylight hours from sunrise to sunset by having the shadow sweep across radial hour lines radiating from the gnomon base.

Historical Development

Ancient Origins

The earliest evidence of timekeeping devices resembling sundials dates to ancient Egypt around 3500 BCE, where towering obelisks served as rudimentary shadow clocks. These slender, four-sided monuments cast moving shadows that partitioned the day into temporal hours, varying in length with the seasons to reflect the sun's apparent path across the sky. Erected in public spaces and temple complexes, obelisks not only marked daily divisions but also aligned with solar observations for ritual purposes, emphasizing the sun's divine role in Egyptian cosmology. By around 2000 BCE, similar shadow-casting tools emerged in Mesopotamia and China, primarily as simple gnomons—vertical sticks or poles—used for tracking seasonal changes rather than precise hourly divisions. In Mesopotamia, Babylonian shadow clocks from approximately 1500 BCE measured midday shadows to determine solstices and equinoxes, aiding agricultural planning in the fertile river valleys. Chinese records indicate gnomons in use as early as 2300 BCE at sites like Taosi, where painted sticks recorded shadow lengths to calibrate calendars and predict planting seasons. These devices, often integrated into observational platforms, supported farming cycles by monitoring the sun's annual declination in consistently sunny regions. Archaeological discoveries from Egypt around 1500 BCE reveal more advanced portable sundials, typically L-shaped shadow clocks made of stone or wood, which divided daylight into 12 segments using a gnomon's projection. These artifacts, unearthed in tombs and temple sites, frequently appear alongside water clocks (clepsydrae) to extend timekeeping into nighttime or cloudy conditions, combining solar and hydraulic methods for greater reliability. Such portable designs facilitated basic daily timing for laborers and priests, while their ritual inscriptions linked time measurement to solar deities like Ra, underscoring their role in religious ceremonies and agricultural festivals. In the Greek world, the philosopher Anaximander of Miletus (c. 610–546 BCE) is credited with introducing Egyptian or Babylonian shadow clocks to Greece in the sixth century BCE, adapting them for systematic astronomical study. He erected gnomons in public spaces to observe solstices and equinoxes, bridging rudimentary Egyptian designs with emerging Greek interest in natural philosophy, though still focused on seasonal and ritual applications rather than equitable hours.

Classical and Medieval Periods

In the classical period, sundials reached a high level of architectural and functional integration, exemplified by the Tower of the Winds in Athens, constructed around 50 BCE by Andronicus of Cyrrhus. This octagonal marble structure featured eight sundial faces on its exterior, each oriented to a cardinal or intercardinal direction, allowing Athenians to read local solar time from multiple angles throughout the day. The dials combined with an internal water clock and a wind vane, serving as a public timekeeping and meteorological station in the Roman Agora. The Romans further advanced sundial design through systematic documentation and adaptation. In the 1st century BCE, the architect Vitruvius detailed various types in his treatise De Architectura, including equatorial dials that projected the sun's path onto a plane parallel to the celestial equator and vertical dials suited for building facades. Book IX of the work describes 13 sundial varieties, emphasizing their geometric construction and integration into urban architecture, which facilitated widespread adoption across the empire. During the Islamic Golden Age, sundials evolved with mathematical precision, particularly for religious purposes. From the 8th to 13th centuries, scholars developed designs that accounted for latitude-specific adjustments, enabling accurate timekeeping across diverse regions of the Islamic world. Sundials became ubiquitous in mosques, where shadows indicated prayer times such as midday (zuhr) and afternoon (asr), integrating astronomy with daily worship. In the 11th century, Al-Biruni advanced spherical and universal dials in works like Al-Qanun al-Mas'udi, incorporating trigonometric methods to create versatile instruments usable at multiple latitudes without recalibration. These innovations built on earlier Greek influences but refined for practical astronomy. In medieval Europe, sundials supported monastic life and portable travel. Monasteries installed simple stone dials, often called mass dials, to mark the canonical hours for prayers like terce, sext, and none, structuring the Benedictine day around solar time. These equinoctial designs, carved into church walls, emphasized equal hours for consistency in communal routines. Portable variants, such as ring dials, appeared from the late Saxon period onward, allowing individuals to determine time by aligning a gnomon with the sun's altitude, with examples dating to the 10th century in England. Latitude adjustments in these devices ensured portability across regions, reflecting the era's blend of scholarly transmission from Islamic sources and local adaptation.

Renaissance to Modern Era

During the Renaissance and into the 17th century, sundials underwent significant refinement through scholarly treatises that advanced their design and mathematical precision. Athanasius Kircher, a Jesuit scholar, published Ars Magna Lucis et Umbrae in 1646, a comprehensive work exploring the geometry and optics of shadows, including detailed constructions for various sundial types such as vertical, horizontal, and universal dials, which served as scientific tools for measuring time and celestial positions. This period saw an explosion of such publications across Europe, building on earlier Italian contributions like Giovanni Padovani's 1570 treatise, which introduced innovative layouts for polar and equatorial dials using algebraic methods. Sundials also became integral to landscape architecture, particularly in Italian estates, where they symbolized harmony between art, science, and nature; for instance, polyhedral sundials from around 1550 adorned gardens in Rome's Quirinal Hill, blending astronomical function with aesthetic ornamentation in sites like Villa Madama. By the 18th and 19th centuries, the rise of accurate mechanical clocks led to a decline in sundials' practical dominance for everyday timekeeping, as portable watches became more reliable and affordable, shifting sundials from essential tools to supplementary devices. Nonetheless, they persisted in specialized applications like navigation and land surveying, where portable ring and diptych dials provided orientation and latitude measurements during expeditions, complementing compasses and chronometers at institutions such as the Royal Observatory, Greenwich. In Britain, while direct evidence of Ordnance Survey reliance on sundials for mapping is limited, historical surveys often used them to establish true north and synchronize observations, aiding triangulation efforts until telegraphy standardized time in the mid-19th century. In the 20th and 21st centuries, sundials experienced a revival among hobbyists and educators, transitioning toward ornamental and cultural roles. The North American Sundial Society, founded in 1978, has promoted gnomonics through conferences, registries, and publications, fostering interest in design, history, and construction for public art installations and educational tools. Modern precision sundials, often incorporating laser-etched lines or projected shadows, appear in astronomical observatories for demonstrating solar motion, such as analemmatic dials in parks near facilities like the Very Large Array. This cultural shift emphasizes aesthetics over utility, with historical sites gaining international recognition; for example, the Jantar Mantar observatory in Jaipur, featuring the world's largest stone sundial built in 1734, was designated a UNESCO World Heritage Site in 2010 for its astronomical legacy.

Design and Operation

Gnomon and Dial Components

The gnomon is the primary shadow-casting element of a sundial, typically a rod, plate, or triangular projection fixed perpendicular to the dial face. Common types include the fixed axial gnomon, oriented parallel to the Earth's rotational axis for consistent alignment with celestial north; the vertical gnomon, positioned perpendicular to the local horizon; and the inclined gnomon, set at an angle specific to the installation's requirements. Historically, gnomons were crafted from durable stone or early metals like bronze to withstand environmental exposure, while modern designs often employ brass or corrosion-resistant alloys such as stainless steel for enhanced longevity. A key feature of the gnomon is the substyle, the precise edge or tip that produces the shadow used for time reading, often sharpened or beveled to minimize diffusion and ensure accuracy. For optimal performance, the gnomon's style must align such that its inclination matches the local latitude when configured for an equatorial dial, allowing the shadow to trace hour lines uniformly throughout the day. The dial plate serves as the surface receiving the gnomon's shadow, available in flat planes for simplicity, curved forms to accommodate non-planar designs, or even spherical shapes for specialized applications like armillary instruments. Its orientation—horizontal for ground-level installations, vertical for walls, or equatorial for polar alignment—is determined by the site's latitude to align with the gnomon's projection. In outdoor settings, both gnomon and dial materials prioritize weathering resistance, with options like anodized aluminum or granite ensuring stability against rain, wind, and temperature fluctuations over decades.

Hour Line Construction

Hour lines on a sundial dial plate indicate the positions where the gnomon's shadow falls to denote specific hours, radiating from the gnomon's root in patterns determined by the sundial's geometry and location. Construction of these lines requires either direct observation of shadows or precise geometric calculations to ensure accuracy in timekeeping. The empirical method for marking hour lines relies on observing and recording the actual path of the gnomon's shadow over time with a fixed gnomon properly aligned to the local latitude. By noting the shadow tip's position at regular intervals, such as hourly during a single day or across multiple days to average seasonal variations, the hour lines can be traced directly onto the dial plate, providing a practical approach for simple constructions without advanced mathematics. This technique captures the sun's apparent motion specific to the site, though it demands clear weather and known starting times for calibration. In contrast, the mathematical method employs trigonometry to determine hour line positions based on the sundial type and observer's latitude φ, ensuring reproducible results for any location. For equatorial sundials, where the dial plane is parallel to the celestial equator, hour lines are straight lines extending from the gnomon root at equal angular intervals of θ = 15° × n, with n representing the hours before or after noon, reflecting the Earth's 15° hourly rotation. Depending on the dial type, these lines may appear as straight radials in polar projections or as hyperbolic curves in non-planar or projected designs, adapting to the shadow's trajectory. Latitude dependence adjusts the line angles, such that lines radiate from the gnomon root with orientations calculated via formulas like tan(α) = sin(φ) / (cos(φ) × cos(15° × t)), where t is the time in hours from noon, accounting for the observer's position relative to the equator. For horizontal sundials, a common variant uses tan(θ) = tan(15° × n) × sin(φ) to find the angle θ of each line from the north-south meridian. Practical tools aid in applying these mathematical constructions accurately. A protractor measures and transfers the calculated angles from the gnomon root onto the plate, while a string stretched taut from the root at the specified angle can guide straight-line markings across the surface. For contemporary builders, software such as Shadows Expert computes and generates detailed diagrams of hour lines tailored to specific latitudes, orientations, and dial types, outputting printable templates for engraving or painting. Once hour lines are established, finer subdivisions for half-hours and minutes are marked using proportional spacing along each line, dividing the segments between hourly marks evenly either angularly or linearly to maintain consistent time intervals across the dial. This ensures readability without altering the primary geometric layout.

Time Corrections and Adjustments

Sundials measure apparent solar time, which differs from mean solar time—the uniform time used by clocks—due to variations in Earth's orbital speed and axial tilt. Even a correctly aligned sundial can differ from a wristwatch by several minutes because it measures apparent solar time (the real Sun) rather than averaged civil time. The equation of time (EoT) quantifies this discrepancy as the difference between apparent and mean solar time (EoT = apparent - mean), reaching a maximum of about ±16 minutes over the year. These variations arise from Earth's 23.4° axial obliquity, contributing up to ±10 minutes, and its elliptical orbit with an eccentricity of 0.0167, adding up to ±7.5 minutes. A common approximation for the EoT in minutes is given by EoT ≈ -7.7 sin(M) + 10 sin(2L), where M is the mean anomaly and L is the mean solar longitude (adjusted for radians or degrees as appropriate); more precise calculations use astronomical almanacs or software. To align sundial readings with local mean solar time, subtract the EoT from the apparent (sundial) time: if EoT is positive, the sundial is fast relative to mean time; if negative, the sundial is slow. Annual EoT values fluctuate predictably, as shown in the table below for approximate mid-month values (in minutes).
MonthApproximate EoT (minutes)
January-11
February-13
March-5
April-1
May+3
June+2
July-4
August-6
September-1
October+9
November+15
December+8
These values are averages and can vary slightly by year. Many precise sundials include a scale or graph of the equation of time or an analemma to allow direct correction without tables. Longitude correction accounts for the sundial's position relative to the standard meridian of its time zone, as standard time is based on mean solar time at that meridian (typically 15° longitude intervals, corresponding to 1 hour). The adjustment is 4 minutes of time per degree of longitude difference: if the location is west of the standard meridian, add the correction (local time lags); if east, subtract it. For example, a sundial at 5° west of the meridian requires adding 20 minutes to local mean time to obtain standard time. Daylight saving time (DST), observed in many regions during warmer months, advances clocks by 1 hour to extend evening daylight. For sundials, subtract 1 hour from the reading during DST periods to match adjusted clock time; no adjustment is needed outside DST. This applies seasonally, such as from March to November in parts of the United States. The complete conversion from sundial time (apparent solar time) to standard clock time is: clock time = (sundial time - EoT) + longitude correction ± DST adjustment. For instance, on November 15 at a location 3° east of the standard meridian (subtract 12 minutes for longitude) during non-DST, if the sundial reads 12:00 and EoT is +15 minutes, the mean time is 12:00 - 15 = 11:45, and standard time is 11:45 - 12 = 11:33. Such adjustments ensure sundial readings align with civil timekeeping.

Southern Hemisphere Variations

In the Southern Hemisphere, the apparent motion of the Sun differs from that in the Northern Hemisphere, leading to reversed shadow directions on sundials. The Sun rises in the east and follows an arc across the northern sky, causing the shadow on a horizontal sundial to move counterclockwise throughout the day, opposite to the clockwise progression observed in the Northern Hemisphere. The gnomon in Southern Hemisphere sundials must be oriented to align with the Earth's rotational axis, pointing toward the south celestial pole. This requires tilting the gnomon southward at an angle equal to the local latitude; for instance, at 30°S latitude, the inclination is 30° toward the south to ensure accurate time projection. Seasonal effects in the Southern Hemisphere result in longer daylight hours during the austral summer (December to February), but the solar analemma—the figure-eight path of the Sun's position at the same clock time over a year—appears inverted vertically compared to the Northern Hemisphere version, with the wider loop oriented toward the zenith. Design adjustments for Southern Hemisphere sundials primarily involve mirroring the hour lines to account for the reversed shadow motion, ensuring the markings progress counterclockwise from the noon position. Notable examples include the large horizontal sundial in Singleton, New South Wales, Australia, recognized as one of the largest in the Southern Hemisphere, and the horizontal sundial in the Kirstenbosch National Botanical Garden in Cape Town, South Africa, which demonstrates these adaptations in a public setting. A common error when installing sundials in the Southern Hemisphere is applying Northern Hemisphere templates without modification, which results in hour lines offset by up to 180°, rendering the device inaccurate as shadows fall on incorrect markings.

Fixed Gnomon Sundials

Horizontal Sundials

Horizontal sundials feature a flat, level dial plate oriented horizontally, typically placed on the ground, a pedestal, or a stable surface, with a polar gnomon that casts a shadow to indicate the time. The gnomon, often a thin plate or rod, is aligned parallel to Earth's rotational axis, tilting southward in the Northern Hemisphere at an angle equal to the local latitude to point toward the north celestial pole. This setup ensures the gnomon's shadow traces the sun's apparent motion across the sky, with the dial plate marked by hour lines radiating from a central point beneath the gnomon's elevated tip. A simple educational demonstration, often used to teach children about sundial principles and the Sun's apparent motion, involves placing a vertical stick in the ground to act as a gnomon and marking the position of the shadow's tip at hourly intervals on a sunny day. The shadow is longest in the morning and late afternoon, shortest at solar noon when it points roughly north (in the Northern Hemisphere), and moves generally from west to east as the day progresses. Illustrations of this experiment typically depict a central vertical stick with radiating lines or arcs indicating shadow positions at specific times (e.g., 9 AM, 12 PM, 3 PM), often accompanied by labels and depictions of the Sun's daily path. While this activity effectively illustrates daily variations in shadow length and direction due to the Sun's movement, it provides only qualitative observations and does not support accurate year-round timekeeping. Precise horizontal time indication requires a polar-aligned gnomon to project the Sun's motion onto the dial correctly, producing straight hour lines with appropriate spacing. The hour lines on the dial are constructed by calculating the angles at which the gnomon's shadow falls for each hour, derived from the geometric projection of an equatorial sundial onto the horizontal plane. These lines are straight rays emanating from the center but spaced unevenly, with angles increasing more rapidly away from the noon line, giving the appearance of fanning outward. The angle θ\theta of each hour line from the noon meridian is determined by the formula tanθ=sinϕtanh\tan \theta = \sin \phi \cdot \tan h, where ϕ\phi is the latitude and hh is the hour angle (multiples of 15° from solar noon, positive westward). For instance, at 40°N latitude, the 1 p.m. line (h = 15°) yields θ9.8\theta \approx 9.8^\circ, the 2 p.m. line (h = 30°) yields θ20.3\theta \approx 20.3^\circ, the 3 p.m. line (h = 45°) yields θ32.5\theta \approx 32.5^\circ, and the 4 p.m. line (h = 60°) yields θ48.0\theta \approx 48.0^\circ, illustrating the nonlinear spacing that requires trigonometric computation for accuracy. The shadow cast by the gnomon's edge moves across the dial in a predictable manner: it is shortest at local solar noon, when the sun is at its highest and the shadow aligns along the north-south meridian, then lengthens symmetrically eastward in the morning and westward in the afternoon, rotating clockwise in the Northern Hemisphere at approximately 15° per hour. This behavior stems from the sun's daily path parallel to the celestial equator, projected onto the horizontal plane, allowing time to be read where the shadow intersects the corresponding hour line. Horizontal sundials offer simplicity in design and installation, requiring no complex mounting beyond ensuring the plate remains level and the gnomon aligned to true north, making them stable and durable for outdoor settings like gardens or parks. Their widespread use arises from this ease and the clear visibility of the illuminated dial face throughout the day. However, they are limited to operation during daylight when the sun is above the horizon, providing no indication at night or in overcast conditions, and their utility diminishes near the poles where high latitudes cause extreme compression of the hour lines, rendering early and late hours difficult to distinguish due to the sun's low, nearly horizontal path.

Vertical Sundials

Vertical sundials are affixed to vertical surfaces, typically walls of buildings, and are oriented to face the equator—south in the Northern Hemisphere—to capture the sun's path effectively. The gnomon, which casts the shadow, is positioned horizontally and overhangs the dial plate perpendicularly, often in the form of a rod or plate extending from the dial face. The hour lines on these sundials feature a straight vertical line marking noon, with other lines curving symmetrically outward to indicate the progression of hours. A variant known as the polar decliner adjusts the gnomon by tilting it to an angle equal to the local latitude, aligning it more closely with the Earth's axis for enhanced precision in certain configurations. As the sun arcs across the sky, the gnomon's shadow traces a path downward from the eastern side of the dial toward the western side, reflecting the sun's apparent motion. These sundials function year-round, though shadows are notably shorter in summer due to the sun's higher elevation, limiting the visible range on the dial during midday. Such dials are prevalent on architectural facades worldwide, serving both practical and decorative purposes, as seen in historical church walls and public buildings. The polar vertical dial, with its gnomon parallel to the Earth's rotational axis, exemplifies an advanced form that minimizes seasonal distortions. For installation on declining walls not facing due south, azimuth corrections are applied to recalibrate the hour lines, accounting for the wall's angular deviation from the cardinal direction to maintain accuracy.

Equatorial Sundials

Equatorial sundials consist of a planar dial aligned parallel to the celestial equator, with the gnomon positioned perpendicular to the dial plane and oriented parallel to the Earth's rotational axis. To achieve this alignment at a given latitude φ, the dial is tilted at an angle of 90° - φ relative to the horizontal, ensuring the gnomon points toward the celestial pole. This configuration draws from fixed gnomon principles, where the style's direction matches the polar axis for seasonal accuracy. The hour lines on an equatorial sundial are straight and equally spaced at intervals of 15°, corresponding to the Earth's 360° rotation over 24 hours and yielding uniform divisions for apparent solar time. These lines radiate from the gnomon's base, typically marked from 6 a.m. to 6 p.m. on one side, with the noon line aligned perpendicular to the gnomon's shadow at local solar noon. A primary advantage of equatorial sundials is their uniform scale, which simplifies reading as the hour markings remain consistent throughout the year without seasonal distortions. This design also facilitates easy construction and portability, particularly in ring-shaped forms that can be handheld or mounted flexibly. In operation, the gnomon's shadow traces a circular arc, crossing the hour lines perpendicularly, advancing at a constant angular speed of 15° per hour due to the projection of the Sun's equatorial motion onto the dial plane. This predictable motion contrasts with the variable paths on other fixed dials, enhancing readability under direct sunlight. Variants include the bowstring gnomon, where a thin wire or rod replaces a solid style for reduced weight and simpler fabrication while maintaining precision. Such models are prevalent in educational settings, often used to demonstrate solar geometry and Earth's rotation in classroom or museum exhibits.

Inclined and Declining Sundials

Inclined sundials feature a dial plate positioned at an angle to the horizontal plane, distinct from fully horizontal or vertical orientations, allowing installation on sloped surfaces such as roofs. The gnomon for these dials must be adjusted so its angle to the dial plane equals the observer's latitude minus the inclination angle of the plate, ensuring the shadow traces accurate hour lines across the day. This adjustment maintains the gnomon parallel to the Earth's axis, similar to vertical dials but accounting for the tilt..pdf) Declining sundials are mounted on surfaces facing away from the cardinal direction, such as east or west, with the declination angle defined as the deviation from due south (zero degrees for south-facing walls). The co-declination angle, calculated as 90° minus the azimuth-based declination, determines the gnomon's rotation in the horizontal plane to align with the local meridian. Hour lines on declining dials are derived through projection methods, often using tables or graphical constructions to account for the offset orientation. Reclining or combined inclined-declining sundials incorporate both tilt and rotation, where the plate is inclined to the horizontal and declined from cardinal alignment; calculations involve double projection techniques to position hour lines correctly. These are common in portable pocket dials, which can be held at various angles for use in different locations, or empirically marked on irregular surfaces like building facades. For instance, a vertical slightly declining sundial on the Hôpital Laënnec in Paris demonstrates practical application on a non-cardinal wall..pdf) Challenges in designing these sundials include distorted hour lines due to the non-standard orientation, necessitating trigonometric adjustments for declination and inclination to ensure precision; without them, shadows may deviate significantly from true solar time. Empirical methods, such as direct shadow tracing over multiple days, can supplement calculations for irregular installations, though they require clear skies and extended observation periods.

Non-Planar Fixed Sundials

Non-planar fixed sundials feature curved or irregular surfaces that receive the shadow from a stationary gnomon, allowing for unique aesthetic integrations into architecture while maintaining timekeeping accuracy through geometric principles adapted from planar designs. These sundials exploit developable surfaces—such as cylinders, cones, and spheres—that can be mathematically unrolled onto a plane for easier construction of hour lines, which then appear as helices or other curves on the original form. Unlike planar variants, the shadow path wraps around the surface, providing a three-dimensional display of time that enhances visual appeal in settings like columns or monuments. Cylindrical dials consist of a vertical or inclined cylindrical surface with a gnomon parallel to the axis, where the shadow traces helical paths corresponding to hour lines. These lines are generated by projecting the sun's rays onto the unrolled rectangle of the cylinder, resulting in straight lines on the flat development that become helices when wrapped back. Historical examples date to medieval Europe, where cylindrical dials were popular for their portability in early forms, but fixed versions emerged in architectural contexts, such as engravings on stone columns to blend functionality with ornamentation. Conical dials employ an inward- or outward-facing conical surface, often with the gnomon aligned along the cone's axis at an angle matching the latitude or ecliptic obliquity for uniform hour spacing. On the conical surface, hour lines radiate from the apex and intersect solstice and equinox curves, enabling precise readings across seasons. Ancient Greek examples, such as the marble conical sundial from Piraeus (dated to the Roman period), feature 11 inscribed hour lines on a southern-oriented cone with a brass gnomon, demonstrating early mastery of conic sections for time division. Another artifact, the conical sundial from Thyrrheion in Greece (3rd century BCE), illustrates similar design with a fixed gnomon casting shadows on curved solstice arcs. Spherical dials project hour lines onto the surface of a globe, typically with a polar gnomon extending along the diameter parallel to Earth's axis, producing shadows that trace small circles parallel to the celestial equator. This configuration allows the dial to function like an equatorial sundial but in three dimensions, with meridians serving as hour lines spaced at 15-degree intervals for solar hours. The spherical form provides omnidirectional visibility and aesthetic symmetry, often seen in large-scale installations where the globe's curvature emphasizes the sun's apparent motion. Construction involves spherical trigonometry to position lines, ensuring the shadow aligns correctly regardless of the observer's viewpoint around the sphere. For developable surfaces like cylinders and cones, construction begins by unrolling the curved form into a planar net, where standard hour line calculations (similar to those for horizontal dials) are applied using the surface's local orientation and latitude. The resulting lines are then transferred back to the curved material, preserving distances and angles without distortion due to zero Gaussian curvature. This method simplifies engraving or painting on materials like stone or metal, offering advantages in three-dimensional aesthetics for architectural features, such as integrating dials into pillars or facades without compromising accuracy. Spheres, which are not developable due to their Gaussian curvature, require spherical trigonometry or approximations using developable patches for line placement. Notable examples include the Humbekk Sundial in Grimbergen, Belgium (2013), a fixed vertical cylindrical column of opal stone engraved with helical hour lines for local timekeeping in a public space. Similarly, the Mather Sundial at Princeton University features a cylindrical shaft with a southern-facing dial, combining classical architecture with precise shadow projection for educational display. These integrations highlight non-planar dials' role in enhancing built environments while adhering to traditional gnomon-shadow principles.

Movable Gnomon Sundials

Analemmatic Sundials

An analemmatic sundial is a type of horizontal sundial characterized by a flat dial plate marked with an elliptical scale of hour points and a vertical gnomon that is repositioned monthly along a north-south alignment to account for the sun's seasonal declination. This design allows the sundial to accurately indicate solar time throughout the year without requiring a fixed gnomon tilted at the local latitude. The gnomon, often a simple post or even a person's body in public installations, casts a shadow whose tip falls on the corresponding hour point on the ellipse. The underlying principle derives from the orthographic projection of an equatorial sundial onto the horizontal plane of the location, where the hour circle of the celestial equator is transformed into an ellipse to compensate for the observer's latitude. By moving the gnomon northward or southward from the ellipse's center by a distance proportional to the sun's declination, the design simulates the varying angle of the sun's rays as if the gnomon were fixed on an inclined equatorial plate. This movement effectively adjusts for the sun's path, ensuring the shadow aligns correctly with the hour points regardless of the season. The ellipse's major axis runs east-west and equals twice the radius of the projected equatorial circle adjusted for latitude, while the minor axis aligns north-south and is shortened by the sine of the latitude. Construction begins with determining the ellipse parameters based on the site's latitude ϕ\phi and a chosen gnomon height hh. The semi-major axis aa of the ellipse is given by a=hcosϕa = \frac{h}{\cos \phi}, which sets the distance from the center to the 6 a.m. or 6 p.m. points. The semi-minor axis bb is then b=htanϕb = h \tan \phi. For positioning the hour points, coordinates are calculated using parametric equations: for hour angle 15t15^\circ t (where tt is hours from noon), the x-coordinate (east-west) is x=asin(15t)x = a \sin(15^\circ t) and y-coordinate (north-south) is y=bcos(15t)y = b \cos(15^\circ t), with points plotted relative to the center. The gnomon's position for a given date is offset from the center by d=htanδd = h \tan \delta, where δ\delta is the sun's declination (ranging from -23.44° at winter solstice to +23.44° at summer solstice); tables or calculators provide δ\delta values, such as +23.44° offset northward for June 21. The dial is typically inscribed on a paved surface, with the north-south gnomon path marked as a straight line through the ellipse's minor axis, often including date indicators or a zodiacal scale for positioning. These sundials offer advantages in compactness and interactivity, as the elliptical layout fits well in limited spaces like parks or gardens, and the movable gnomon enables users to participate by standing in position to cast their shadow, making them educational tools for demonstrating solar motion and timekeeping. Their prevalence in public settings stems from this versatility, with the design scaling proportionally to gnomon height without altering the ellipse's shape, thus accommodating various installations from small plaques to large walkways.

Universal Equinoctial Ring Dials

Universal equinoctial ring dials are portable sundials engineered for use across a wide range of latitudes, featuring a primary circular ring oriented parallel to the celestial equator. The core structure comprises an outer equatorial ring, often made of brass, with an inner meridian ring or scale for time reading; a sliding bead, wire, or crosspiece serves as the adjustable gnomon, positioned along an engraved latitude scale to match the observer's location between 0° and 90° in either hemisphere. This design simplifies the armillary sphere into a compact, self-aligning instrument, allowing suspension from a ring or handle for vertical positioning. In operation, the dial is hung freely and rotated until the sun's rays align parallel to the equatorial plane, causing the shadow of the ring's edge or the internal gnomon to fall on the hour scale inscribed on the meridian ring, thereby indicating local solar time in equatorial hours. The instrument's portability stems from its latitude-adjustable mechanism and lightweight construction, making it ideal for travelers who could engrave or reference specific locations on the scale; it originated in the 16th century as a refinement of earlier astronomical rings, with roots tracing to medieval Islamic designs that emphasized universal applicability. When briefly referencing equatorial principles, the dial's efficacy relies on the sun's projection onto an equatorial coordinate system for consistent timekeeping regardless of location. Variants enhance simplicity and versatility, such as those employing a string gnomon—a taut cord stretched across the ring that casts the shadow—reducing mechanical complexity while maintaining functionality for quick setups in the field. These dials typically offer accuracy within 5 minutes of solar time under optimal sunlight, though performance depends on precise latitude setting and minimal obstructions. Historical examples include ornate 17th-century European models influenced by Islamic prototypes, preserved in institutions like the Whipple Museum, alongside modern replicas crafted for educational and navigational demonstrations that replicate the original precision.

Foster-Lambert Dials

The Foster-Lambert dial is a movable-gnomon sundial that employs a cylindrical projection to map the sun's equatorial motion onto a flat plane, enabling accurate timekeeping across varying latitudes through gnomon adjustment. Invented by English mathematician Samuel Foster in the mid-17th century, the design was independently rediscovered and refined by German polymath Johann Heinrich Lambert in 1775, who described it as a novel universal timepiece in his publication Photometria. This projection transforms the standard elliptical path of an analemmatic sundial into a circular hour ring by altering the projection direction, resulting in a compact, portable instrument suitable for diverse environments. The core design features a flat dial plate inscribed with a circular ring of equiangular hour points, spaced at 15-degree intervals to represent solar hours, along with a semicircular arc for positioning the gnomon. The gnomon itself is a slender rod mounted on a pivot that allows it to rotate along the latitude arc, where its base is set to the observer's latitude φ; the rod extends perpendicular to the arc's radius and is tilted such that its upper end aligns with the celestial pole direction. This setup projects cylindrical coordinates from the equatorial plane onto the dial, with the shadow cast by the gnomon's tip tracing the circular ring to indicate the sun's azimuth for time reading, while radial lines or auxiliary scales on the dial can denote solar altitude. The projection incorporates a scaling factor of sin(φ) to account for the gnomon's tilt relative to the horizontal, ensuring the shadow length and position accurately reflect the latitude-dependent solar path. A key mechanism of operation involves aligning the dial horizontally and north-south, then adjusting the gnomon to the local latitude before observing the shadow's intersection with the hour ring, which directly yields apparent solar time without needing fixed latitude-specific engravings. Unlike fixed-gnomon designs, this movability compensates for latitudinal variations in solar elevation, maintaining readability throughout the year. For enhanced functionality, some variants include date scales along the gnomon arc to correct for the equation of time, though the base design prioritizes simplicity. The primary advantages of the Foster-Lambert dial lie in its latitude independence, achieved via the simple gnomon rotation, which made it valuable for navigational applications among 18th- and 19th-century explorers and sailors requiring a reliable, portable timekeeper adaptable to global voyages. Its dual role as a solar compass—determining true north by aligning the gnomon's plane with the sun's path at noon—further enhanced its utility in orientation tasks. Historically, Lambert's refinement emphasized its mathematical elegance, deriving the circular projection to simplify construction and improve precision over earlier irregular dials.

Shadow and Altitude Sundials

Human Shadow Sundials

Human shadow sundials employ the human body as the gnomon, with the individual standing upright at a fixed point on a marked horizontal surface, allowing the shadow cast by the sun—typically from the head or feet—to indicate the approximate time of day. This method relies on the basic principle of solar shadows, where the position of the shadow relative to calibrated markings on the ground reveals the sun's apparent movement across the sky. The design of these sundials is adapted to human proportions, with the scale calibrated for an average adult height of about 1.7 meters to ensure the shadow tip aligns properly with hour lines. These lines are drawn in a semicircular or linear pattern on the ground, adjusted according to the local latitude to account for the sun's declination and provide reasonable accuracy for solar time throughout the year. Markings may be etched into pavement, drawn with chalk, or set with stones, making the setup portable and suitable for temporary use. Historically, human shadow sundials functioned as simple tools for nomadic peoples, enabling rough time estimation without permanent structures, and evidence of similar shadow-based methods appears in ancient Chinese practices where vertical gnomons measured shadows for calendrical and daily timing dating back to the 23rd century BCE. In Africa, early examples from ancient Egyptian civilizations around 1500 BCE demonstrate the use of shadow-casting devices for dividing the day. Despite their simplicity, human shadow sundials have limitations, including variations in individual height that can shift the shadow position by several degrees and reduce precision to rough hourly estimates rather than minutes. They are also ineffective during cloudy weather or at night and provide only approximate results due to the lack of adjustments for the equation of time. In modern contexts, human shadow sundials are primarily employed for educational purposes to demonstrate solar geometry and Earth's rotation, often in school activities where participants track their shadows over hours. They also appear in performance art installations, such as interactive public sculptures that invite viewers to engage as the gnomon for experiential timekeeping.

Shepherd's Dials and Timesticks

Shepherd's dials are portable altitude sundials designed for simplicity and practicality, primarily used by shepherds and travelers to determine local solar time based on the sun's elevation above the horizon. These devices consist of a vertical cylinder or stick, often made of wood or metal, with a small aperture or gnomon at the top that allows sunlight to project a shadow onto an internal or external scale marked with hour lines. Unlike equatorial or horizontal dials that rely on the sun's azimuth, shepherd's dials measure time through the varying length or position of the shadow, which correlates with solar altitude and thus the time of day. In operation, the dial is held or suspended vertically with the gnomon oriented toward the sun, ensuring the shadow falls directly onto the calibrated scale without needing alignment to true north. The scale features curved hour lines adjusted for the observer's latitude, and the shadow's endpoint or length indicates the hour on a linear or circular marking system. Seasonal variations are accounted for by sliding a movable peg along the axis or selecting pre-marked bands corresponding to the sun's declination, allowing the device to function throughout the year despite changes in the sun's path. This altitude-based method makes the dial independent of orientation but sensitive to latitude, limiting its portability to specific regions unless recalibrated. Historically, shepherd's dials emerged in medieval Europe, with evidence of their use dating back to the late Middle Ages as compact traveler's tools known as "chilindres" in French contexts. They were particularly prevalent among pastoral communities in the Pyrenees Mountains and rural France, where shepherds employed them for daily scheduling of flocks and travel from the 16th through the 19th centuries. These dials served as precursors to more elaborate portable instruments like astrolabes, bridging simple shadow-casting methods—such as those using a person's own shadow for rough estimates—with advanced mechanical designs. Their enduring popularity stemmed from ease of construction using local materials, though they gradually declined with the rise of mechanical clocks. Calibration involves inscribing the scale based on the sun's altitude formula, where hour marks account for solar declination (ranging from -23.5° to +23.5° annually) and the local latitude to ensure the shadow aligns correctly with mean solar time. Marks are typically etched or painted for key dates like solstices and equinoxes, with intermediate adjustments via the peg to compensate for the equation of time. These dials are less precise than fixed installations due to manual adjustments and atmospheric effects. Variants include basic notched sticks, known as timesticks, which simplify the design to a tapered wooden rod with incisions along its length; the shadow's tip falls on a notch corresponding to the hour after seasonal peg placement. More advanced cylindrical timesticks incorporate rotating rings or internal vanes for finer declination tuning, as seen in 19th-century Tibetan examples crafted from hardwood in octagonal forms for high-altitude herding. These adaptations maintained the core altitude principle while enhancing durability in rugged environments.

Ring and Card Dials

Ring dials are compact, portable altitude sundials consisting of a small metal hoop equipped with a sighting hole on the outer edge and a thin wire or thread stretched across the interior diameter. The inner surface of the ring features an engraved scale with hour lines calibrated for a specific latitude, allowing the device to indicate time based on the sun's elevation. To operate, the user holds the ring vertically with the sighting hole aligned toward the sun, causing the wire to cast a shadow that falls on the inner scale; the position of this shadow corresponds to the hour, as the sun's altitude varies predictably throughout the day. These dials emerged in the 16th century, with notable examples attributed to instrument makers like Erasmus Habermel, and were favored by European scholars and travelers for their simplicity and ease of use in determining local time without fixed installation. Card dials, exemplified by the Capuchin variant, are hinged, folding instruments typically formed from two rectangular plates of ivory, card, or metal, connected at one edge to form an adjustable angle. A short string or thread serves as the gnomon, attached between the plates near the hinge, while the primary plate bears an altitude scale with hour markings, often including equinoctial divisions for seasonal adjustments. Operation involves setting the angle between the plates to match the user's latitude using a graduated edge or scale, then positioning the device so the sun shines through a small aperture or directly illuminates the string; the shadow cast by the string on the scale reveals the time derived from solar altitude. Originating in 16th-century France and associated with the Capuchin order of Franciscan monks—who adapted them for calculating prayer times—these dials spread among clergy and academics as lightweight alternatives to larger instruments. Both ring and card dials represent evolutions from earlier portable altitude devices, such as shepherds' dials, but prioritize compactness for personal carry. Their primary advantages include pocket-sized portability, enabling discreet timekeeping in varied locations, and the ability to display canonical hours or prayer times alongside civil hours, making them particularly valuable for religious observance in pre-mechanical clock eras. The navicula de Venetiis, or "little ship of Venice," is a portable altitude sundial originating in 15th-century Europe, particularly associated with Venice, where it was employed for determining prayer times and aiding navigation among travelers and seafarers. This rare instrument represents a sophisticated evolution in movable gnomon designs, allowing users to calculate local solar time based on the sun's altitude regardless of location, provided the latitude is adjusted accordingly. The design consists of a typically brass, ship- or boat-shaped plate, often formed by two joined engraved plates, with a central nodus in the form of a hinged rod or pin that serves as the shadow-casting gnomon. A rotatable index arm or cursor, adjustable along a latitude scale, is set to the observer's location to align the dial properly; the front face features curved hour lines for diurnal time, a zodiacal scale for solar declination, and arcs for seasonal adjustments to enhance accuracy. The reverse side integrates a compass rose for orientation, sometimes with additional sighting vanes to align the instrument toward the meridian. In operation, the user first orients the dial to the north-south meridian using the built-in compass and sights, then adjusts the index to the local latitude and the sun's approximate declination via the zodiac scale. With the dial held horizontally and facing the sun, the central nodus casts a shadow onto the curved scale, where the position indicates the local solar time in hours from noon. This method relies on the predictable daily variation in solar altitude, providing readings accurate to within a few minutes under clear conditions, though it requires knowledge of the date for declination correction. Variants of the navicula include models replacing the fixed nodus with a portable string or thread suspending a small bead or weight, which hangs vertically to cast the shadow and improves compactness for travel without compromising functionality. These adaptations highlight the instrument's emphasis on portability, with surviving examples from the late 15th to 17th centuries demonstrating its widespread use in both scholarly and practical contexts across Europe.

Reflection and Nodus Sundials

Reflection Sundials

Reflection sundials operate on the principle that a mirror serves as an equivalent to a traditional gnomon, where the reflected beam of sunlight forms a spot of light that traces a path analogous to a shadow on the dial surface. The position of this light spot indicates the time based on the sun's apparent motion across the sky. The path of the reflected beam mirrors the trajectory a direct shadow would follow, governed by the law of reflection, which states that the angle of incidence equals the angle of reflection relative to the normal at the point of incidence. In design, a small plane mirror is typically positioned to capture sunlight and direct it onto a receiving surface, such as a wall, ceiling, or floor, marked with hour lines and other indicators. For enhanced precision, concave mirrors can focus the sunlight into a sharper spot, similar to the concentrating effect in solar devices. A representative example is the large reflection sundial in Seattle, Washington, where a small circular mirror outside a south-facing window projects a light spot onto an 11-by-17-foot painted ceiling dial, incorporating local solar time, analemmas, and zodiac symbols. Calculations for the dial involve adjusting the mirror's orientation so the reflected ray aligns with the gnomon's shadow path for the specific latitude and declination, often using gnomonic projections adapted for reflection geometry. One key advantage of reflection sundials is their ability to function in shaded locations, as the mirror can be placed in direct sunlight while the dial remains indoors or protected from direct exposure, allowing timekeeping in environments unsuitable for conventional shadow-based designs. This setup also enables the creation of large, accurate dials with minimal physical material, as the light spot is easily visible and adjustable. Historically, reflection sundials emerged in 18th-century Europe, with documented examples from Swiss regions like Tessin, where they were integrated into architectural features such as windows for indoor timekeeping. Modern adaptations draw from solar concentrator technology, such as those in solar cookers, where parabolic or concave mirrors focus sunlight efficiently onto a target, enabling compact yet precise reflection dials for educational or decorative purposes. Unlike nodus-based designs that rely on direct shadows from a protruding element, reflection sundials invert this by projecting light beams, offering versatility in shaded or indoor settings.

Nodus-Based Designs

Nodus-based designs, which originated in ancient Greek astronomy, were further developed in medieval Islamic science and employ a raised nodus, such as a small pin, sphere, or bead positioned along the gnomon or at the dial's center, to cast a three-dimensional shadow whose edges trace both hour lines and declination lines on the receiving surface. This mechanism allows the sundial to simultaneously display the time of day via the intersection of the shadow with hour lines and the date via the position along seasonal declination lines, which form parabolic paths except at the equinoxes where they are straight. These sundials typically feature curved receiving surfaces, including cylindrical or conical shapes, which are developable and thus easier to construct by unrolling into flat patterns for line projection. On a cylindrical surface, for instance, the nodus shadow traces paths that indicate time and solar declination in a compact, portable form suitable for universal use across latitudes. In the 16th century, Johann Schöner further developed these concepts through stereographic projections, enabling multifunctional dials that incorporated nodus shadows on cylindrical or conical surfaces for broader European adoption. The advantages of nodus-based designs include their multifunctionality—revealing time, season, and sometimes azimuth direction—along with aesthetically complex patterns formed by the interwoven lines. In construction, the nodus height above the surface critically determines line separation and shadow clarity, influencing the dial's precision and visual balance.

Multifaceted Sundials

Diptych and Tablet Dials

Diptych dials are portable timekeeping devices consisting of two hinged leaves crafted from materials such as ivory or wood, designed to fold flat for transport and open like a book for use. The inner faces bear engraved scales for reading shadows, while a string gnomon stretches taut between small pegs or holes on the opposing leaves when deployed. The outer face of the lower leaf typically incorporates a compass to confirm orientation during operation. Many diptych dials also include a compass on the lower leaf for proper north-south alignment. To operate a diptych dial, the user adjusts the hinge to form an angle equal to the local latitude, ensuring the lower leaf rests horizontal. The string gnomon is then aligned toward the sun, casting a shadow onto the concave hour scale on the inner surface of the upper leaf, which indicates the time in seasonal or equinoctial hours. The compass aids in orienting the device, combining solar observation with a rudimentary alignment mechanism for portability. Historical examples of ivory diptych and tablet dials trace back to the 15th century, with artifacts such as those incorporating wax writing surfaces for dual utility as notepads and timepieces. These evolved into more refined medieval portable versions, often produced in regions like Nuremberg by the 16th century, reflecting advancements in craftsmanship for travelers. Key features include the use of equinoctial projection on the scales, enabling consistent hour divisions regardless of the season, alongside markings for declination to track solar position and seasonal changes. Such designs allowed users to determine not only daytime hours but also approximate dates based on shadow length variations. Despite their ingenuity, diptych and tablet dials were limited by the fragility of ivory construction, prone to cracking or warping.

Multiface and Prismatic Dials

Multiface sundials integrate multiple dial faces into a single compact structure, such as a pillar or cube, enabling time readings from various angles and orientations throughout the day. These designs commonly feature 4 to 8 dials, with a horizontal dial on the top face for overhead sun positions and vertical dials on the side faces oriented to cardinal directions. Each face is engraved with hour lines calibrated for the local latitude, allowing the structure to function across different times and viewer positions without repositioning. The gnomons—typically slender rods or wires—are either shared across faces or dedicated to each, aligned parallel to the Earth's polar axis to cast accurate shadows regardless of the sun's path. This configuration provides versatility for fixed installations, where a single artifact can serve multiple viewing perspectives, often with shared structural support for stability. In historical contexts, multiface sundials evolved from Renaissance polyhedral designs, scaling up to pillar forms by the 18th century for garden use. Notable examples include 18th-century English garden pillars, such as the four-sided sundial at Houghton Hall in Norfolk, erected around 1720 as a decorative element in formal landscapes, combining utility with ornamental stonework. These pillars allowed all-day time readings by selecting the appropriate face based on the observer's location, enhancing their practicality in expansive outdoor settings. Prussian precision variants, influenced by German instrument-making traditions, incorporated multifaceted polyhedra for refined designs, as seen in 16th- to 18th-century octahedral prism sundials from Augsburg workshops. Prismatic sundials, often polyhedral in shape, feature multiple dial faces where a gnomon casts shadows to indicate time on the appropriate face. This design shares gnomonic principles but allows for multi-directional setups, often with each face tuned to specific latitudes via adjustable mounts. Historical examples from the 16th to 18th century emphasized precision craftsmanship, using wood or metal for durable forms in portable or pedestal configurations. The advantages of both multiface and prismatic dials include comprehensive all-day functionality without needing multiple separate instruments, as well as aesthetic appeal for architectural integration. They extend the basic diptych concept to more complex arrays, prioritizing decorative elegance in gardens and public spaces while maintaining horological accuracy.

Specialized Applications

Meridian Lines and Noon Marks

Meridian lines are architectural features consisting of a precisely oriented north-south line inscribed or embedded in the floor of a building, typically a large indoor space like a cathedral, where a gnomon—often a small hole in a distant window or roof—projects a beam of sunlight that casts a shadow or spot along the line at solar noon. These lines allowed observers to track the sun's position with high accuracy, serving as simple astronomical instruments for determining local solar time and seasonal variations. Noon marks represent a simplified variant, often just a single line, hole, or notch on a wall, floor, or pavement aligned to the meridian, designed to indicate the moment of daily solar culmination when the sun reaches its highest point. Unlike full sundials with hour markings, noon marks focus solely on pinpointing midday, enabling quick visual confirmation of true solar noon without complex calculations. They were commonly incorporated into the facades or interiors of historical buildings, such as churches and observatories, to aid in timekeeping for religious or practical purposes. Historically, meridian lines proliferated in Italian cathedrals during the 16th and 17th centuries as tools for and astronomical , particularly to measure the date of the vernal equinox for accurate Easter calculations under the . A prominent example is the meridian line in the Cathedral of Santa Maria del Fiore in , established in 1755 by Leonardo Ximenes to measure the obliquity of the . Another influential installation is the Clementine Gnomon in the Basilica of Santa Maria degli Angeli in Rome, constructed between 1700 and 1702 under the direction of astronomer Francesco Bianchini on behalf of Pope Clement XI, which used solar observations to study Earth's obliquity and precession. These lines often extended tens of meters in length, with markings for solstices and equinoxes, and were vital for producing some of the most precise solar data available before the widespread adoption of telescopes. The construction of meridian lines demanded meticulous alignment to the true north-south meridian, achieved by observing the passage of stars across the sky, such as Polaris or circumpolar stars, to ensure the line's orientation matched the Earth's rotational axis. A pinhole gnomon, typically a small aperture (around 5-10 cm in diameter) positioned high in a southern wall or roof, was then fitted to project a focused beam of sunlight onto the line, minimizing distortion and allowing the solar spot's position to reveal noon and seasonal shifts with millimeter precision. Materials like brass rods or inlaid marble ensured durability, and the setup required stable architecture to avoid shifts from settling foundations. In modern contexts, meridian lines persist in observatories as educational and functional markers, such as the 150-foot meridian arc at Griffith Observatory in Los Angeles, where embedded photoelectric sensors detect the sun's transit to display real-time solar positions on an adjacent chart. Similarly, the prime meridian line at the Royal Observatory Greenwich serves as a visible reference for astronomical demonstrations, illuminated by a laser at night. Digital analogs, like solar noon calculators from the National Oceanic and Atmospheric Administration (NOAA), provide instantaneous computations of solar culmination times based on GPS location, replicating the meridian's function through algorithms without physical infrastructure.

Sundial Cannons

Sundial cannons, also known as noon cannons or meridian cannons, are specialized devices that combine a sundial with a small cannon, using focused sunlight to ignite gunpowder precisely at solar noon. The mechanism relies on a magnifying lens or burning glass positioned above the sundial plate, which concentrates the sun's rays onto a touchhole filled with black powder in the cannon's barrel. When the sun reaches its zenith, aligned with the local meridian, the intensified light ignites the powder, producing a loud report to signal midday. This pyrotechnic function served both practical and demonstrative purposes, such as announcing mealtimes on estates or entertaining in gardens. These devices emerged in Europe during the 17th century and remained popular through the 19th century, often as decorative garden ornaments in parks and private grounds. In Sweden, they were referred to as "solar guns" and used to mark noon in public spaces, with notable examples from the 18th century onward. A prominent French design was invented by clockmaker Rousseau around 1786, featuring a large-scale meridian cannon installed in the Palais-Royal gardens in Paris, where it fired daily at noon. Production continued into the early 20th century, with ornate brass and marble versions crafted in France circa 1820 and British examples by makers like Negretti & Zambra in the 19th century. Designs typically feature a horizontal or inclined dial plate calibrated for hours around noon, with adjustable supports for the lens to account for latitude and seasonal variations in the sun's path. Some later models incorporated mirrors instead of lenses to reduce fire risk and improve safety during ignition. Examples include a 19th-century British noon cannon restored by the British Sundial Society, featuring brass components and a small barrel, and an American pedestal version from 1800–1860 held by the Smithsonian National Museum of American History, with a marble base and brass cannon. Modern replicas, such as one at the Musée des Arts et Métiers in Paris, demonstrate the device's operation for educational purposes. Despite their ingenuity, sundial cannons were inherently limited by weather conditions, functioning only on clear, sunny days without clouds obstructing the sun. Their reliance on direct solar alignment also made them symbolic rather than reliable timepieces, highlighting early experiments with concentrated for practical effects.

Compass and Navigation Uses

Sundials serve as reliable tools for determining cardinal directions through the alignment of a gnomon's shadow with the sun's position, particularly at solar noon when the shadow points directly along the north-south meridian in the northern hemisphere. This method exploits the sun's apparent daily motion across the sky, allowing users to orient the device by observing the shortest shadow cast by the gnomon, which aligns with true north-south without requiring additional instruments under clear conditions. For more advanced directional applications, the hour angle—derived from the sun's position relative to the local meridian—can be converted to azimuth bearings, enabling precise orientation relative to any desired heading. In the , explorers employed portable equatorial sundials, adjustable for , during voyages to ascertain time at various latitudes, which facilitated calculations when combined with chronometers and supported overall positional . Integrated sundial-compass designs emerged historically to enhance navigational , featuring a magnetic needle embedded in the base to initially align the device to magnetic north before fine-tuning with solar observations for . Such 17th-century French examples combined a hinged for shadow casting with a compass rose, providing dual functionality for direction-finding in exploratory contexts where magnetic variation could be corrected using the sundial's solar reference. Folding variants with built-in compasses were particularly valued by navigators before the widespread adoption of mechanical watches, offering compact reliability for at-sea orientation. The directional accuracy of sundials typically achieves ±1° under clear when aligning the noon shadow, limited primarily by the observer's precision in identifying the shortest shadow point. For bearings derived from hour angles, accounting for the equation of time— which represents the discrepancy between apparent and mean , varying up to about 16 minutes annually—ensures for precise azimuthal readings relative to . In contemporary settings, sundials supplement GPS in survival training programs, where participants learn to construct improvised shadow-stick compasses for direction-finding in environments where electronic devices fail or batteries deplete. These techniques emphasize low-tech redundancy, teaching skills for wilderness navigation that align solar observations with basic tools to maintain orientation when modern systems are unavailable.

Cultural Mottoes and Inscriptions

Sundials have long featured inscriptions that imbue them with symbolic and philosophical depth, often drawing on themes of time's transience and the value of the present moment. Common Latin phrases such as tempus fugit ("time flies"), derived from Virgil's Georgics, and carpe diem ("seize the day"), from Horace's Odes, appear frequently to evoke the fleeting nature of life and encourage mindful living. Another prevalent motto, "Horologia sola umbras numerat" or "I count only the sunny hours," underscores the device's dependence on light while metaphorically suggesting a focus on joyful moments. In historical contexts, particularly during the Renaissance, sundials in European gardens served as moralistic elements, with engravings reminding viewers of mortality and divine order. These installations, popular in Italian and English estates, integrated mottos like "Memento mori" ("remember death") to align with the era's humanistic reflections on time. In Islamic traditions, sundials often bore geometric inscriptions in Kufic script, combining functional markers for prayer times with decorative Quranic verses or astrological symbols, as seen in the Alhambra's sundial, which includes zodiac signs and prayer notations to harmonize astronomy with faith. Notable examples illustrate regional variations and artistic intent. The sundial on Oxford's All Souls College, designed by Christopher Wren around 1658, bears the inscription "Pereunt et imputantur" ("They [the hours] pass and are reckoned to our account"), emphasizing accountability for time spent. In France, horological puns played on words like "heure" (hour), such as "Je ne compte que les heures sereines" ("I count only serene hours"), blending wit with temporal philosophy in 18th-century dials. These engravings served to remind observers of time's inexorable passage, fostering contemplation while enhancing the sundial's aesthetic role in landscapes or architecture. In modern contexts, personalized engravings continue this tradition in public art, where artists commission custom mottos for commemorative or symbolic pieces. For instance, contemporary sculptors like John L. Carmichael create monumental sundials with bespoke inscriptions, such as poetic reflections on sustainability, installed in urban parks to blend functionality with cultural commentary. This evolution maintains the inscription's purpose of artistic integration, adapting ancient motifs to contemporary themes like environmental awareness.

Unusual and Modern Variants

Bifilar and Digital Sundials

A bifilar sundial employs two taut wires or threads, typically oriented north-south and east-west at slightly different heights above a horizontal dial plate, serving as the in place of a traditional style. The shadows cast by these wires intersect to form a moving point that traces a hyperbolic path across the dial, with equiangular hour lines separated by exactly 15 degrees to indicate solar time. This design, invented by German mathematician Hugo Michnik in 1922, allows for precise adjustments to latitude by varying the height of the east-west wire, enabling its use across a range of locations without redesign. One key advantage is the absence of physical wear on a solid , as the flexible wires maintain their alignment over time, and the hyperbolic trace can visually demonstrate the equation of time by plotting the sun's irregular motion relative to mean solar time. Modern reproductions, such as universal bifilar models, have been constructed for educational purposes, appearing in museum displays like those of the North American Sundial Society to illustrate advanced gnomonics. Digital sundials extend the principle of shadow-based timekeeping into numerical displays, often using shaped apertures or projections to form digit-like patterns from sunlight since the late 20th century. An early example is the 1984 invention by Steve Hines, which employs a cylindrical encoder with slits that direct sunlight through optical fibers to illuminate a true 7-segment numerical readout on a distant surface, providing at-a-glance time readability without electronic power. Building on this, a 1994 prototype developed in Germany utilized light projection through masks to render digits directly, patented for its ability to write numbers with illumination rather than shadows alone. More recent designs, emerging in the 2000s and 2010s, incorporate LED or laser elements for enhanced visibility and programmability; for instance, Julien Coyne's 2015 3D-printed gnomon casts shadows forming digital numerals from 10:00 to 16:00 in 20-minute increments, adjustable for latitude via scalable components. These programmable variants can apply corrections for the equation of time algorithmically, projecting adjusted lines or digits to align solar time with civil standards, and avoid gnomon degradation through non-contact light emission. Interactive digital sundials have found applications in educational and public settings, such as installations where laser-projected displays simulate traditional dials on walls or floors for visitor engagement. Complementary mobile apps, developed since the early , emulate these physical mechanisms by overlaying virtual shadows and digital readouts on cameras pointed at the sun, allowing users to explore bifilar traces or numerical projections without hardware.

Spherical and Globe Dials

Spherical and globe dials represent a sophisticated class of three-dimensional sundials, featuring a hollow sphere as the dial face with a polar gnomon—a slender rod aligned parallel to the Earth's axis, extending from pole to pole through the sphere's center. The sphere's surface is inscribed with hour circles that function as meridians, converging at the poles to mark the progression of solar time, while lines of declination serve as parallels, analogous to lines of latitude on a terrestrial globe. This configuration transforms the sundial into a miniature model of the celestial sphere, where the Sun's position relative to the observer's latitude determines the shadow's path. In operation, the tip of the polar gnomon casts a shadow onto the sphere's interior surface as the Earth rotates. The shadow traces great circles across the sphere, intersecting the hour meridians to indicate local solar time; at noon, the shadow aligns with the observer's meridian. These dials can accommodate dual time zones by incorporating offset markings or auxiliary gnomons adjusted for longitudinal differences, allowing simultaneous display of times for locations separated by specific hours, such as standard meridians. The design's reliance on spherical geometry ensures accuracy across a wide range of latitudes, provided the gnomon's orientation matches the local coordinates. Historical examples trace back to ancient Greek innovations, where spherical sundials, often roofed for protection and portability, were constructed using bronze or marble to demonstrate advanced geometric principles; a notable 1st-century AD specimen from Baelo Claudia, Spain, exemplifies this with precisely curved hour lines derived from conic sections. By the 18th century, these dials were frequently integrated into armillary spheres—elaborate skeletal models of the heavens—enhancing their role in astronomical education and garden ornamentation, as seen in European estates and observatories. The primary advantages of spherical and globe dials lie in their visual analogy to the celestial sphere, offering intuitive insights into solar motion, equinoxes, and solstices beyond mere timekeeping, while their elegant, sculptural form makes them prized for decorative purposes in landscapes and architecture. Construction involves calculating the spacing of declination lines using the cosine of the angle δ (where δ is the declination), given by the formula for the radius of the declination parallel circle from the polar axis: r=Rcosδr = R \cos \delta Here, R is the sphere's radius, ensuring the lines project the Sun's path accurately for the installation latitude; artisans typically employ spherical trigonometry or templates for etching these curves onto the surface material, such as metal or stone.

Contemporary Uses and Innovations

In contemporary architecture, sundials are integrated into sustainable designs to promote awareness of passive solar principles and environmental harmony. For instance, the Dezhou New Energy City Solar Park in China, completed in 2011, features a massive sundial-inspired structure that serves as the world's largest solar-powered office building, emphasizing renewable energy through its shadow-casting form that tracks the sun's path. Similarly, modern eco-parks incorporate sundials as functional art, such as the analemmatic dials in urban green spaces, which educate visitors on solar geometry while aligning with LEED-certified buildings' focus on natural light optimization. Sundials play a significant role in STEM education, particularly in teaching astronomy and geometry to students. They serve as hands-on tools for understanding Earth's rotation, latitude effects on shadows, and basic trigonometry, often used in classroom activities to construct simple horizontal or vertical dials. Digital applications enhance this by allowing virtual sundial design; for example, Shadows Pro software enables users to simulate and customize dials for specific locations, integrating geographic data to demonstrate time zones and equinoxes. Augmented reality kits, like those from educational suppliers, let students project and interact with 3D sundial models indoors, bridging ancient principles with modern computing. Innovations in sundial technology blend traditional shadow mechanics with contemporary engineering, such as solar-powered hybrids that combine analog dials with digital clocks for reliability in varied conditions. The HELIOS SATELLITE sundial, introduced by a German manufacturer, uses photovoltaic cells to power a 12-hour display while maintaining classical gnomon functionality, inspired by space probes for precision. Since the 2010s, 3D printing has enabled customizable dials, with open-source designs like the Mojoptix Digital Sundial on Thingiverse allowing users to produce shadow-projected numerical timepieces without electronics, fostering maker education and personalization for gardens or wearables. Concepts like the solar-powered wall clock prototype further innovate by harnessing ambient light to mimic sundial shadows on indoor surfaces. Recent large-scale projects include the Arch of Time in Houston, Texas, completed in 2024, designed by Riccardo Mariano as the world's largest sundial and an arts venue incorporating solar panels for energy generation. Professional organizations sustain interest through symposia and public projects; the North American Sundial Society (NASS), established in 1997, hosts annual conferences and maintains a registry of installations, promoting research since the late 20th century. Post-2000 public examples include the Sundial Bridge in Redding, California (2004), a pedestrian span by Santiago Calatrava that functions as a large-scale gnomon over the Sacramento River, integrating art, engineering, and timekeeping in urban renewal. The British Sundial Society, active since 1965, supports similar global efforts with journals and events. Urban challenges impact sundial efficacy, as scatters sunlight and diffuses shadows, reducing accuracy in densely built environments where artificial glare overwhelms direct solar rays during twilight hours. exacerbates this through altered sunlight patterns, including increased cloud cover from shifting weather regimes, which can shorten viable observation periods and necessitate recalibration for long-term installations. These factors underscore the need for adaptive designs in light-sensitive locations.

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