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Twilight
Twilight
from Wikipedia
Twilight is the time period between dawn and sunrise, and between sunset and dusk.
Morning twilight: astronomical, nautical, and civil stages at dawn. The apparent disk of the Sun is shown to scale.[1]
Evening twilight: civil, nautical, and astronomical stages at dusk. The solar disk is shown to scale.

Twilight is daylight illumination produced by diffuse sky radiation when the Sun is below the horizon as sunlight from the upper atmosphere is scattered in a way that illuminates both the Earth's lower atmosphere and also the Earth's surface. Twilight also may be any period when this illumination occurs, including dawn and dusk.

The lower the Sun is beneath the horizon, the dimmer the sky (other factors such as atmospheric conditions being equal). When the Sun reaches 18° below the horizon, the illumination emanating from the sky is nearly zero, and evening twilight becomes nighttime. When the Sun approaches re-emergence, reaching 18° below the horizon, nighttime becomes morning twilight. Owing to its distinctive quality, primarily the absence of shadows and the appearance of objects silhouetted against the lit sky, twilight has long been popular with photographers and painters, who often refer to it as the blue hour, after the French expression l'heure bleue.

By analogy with evening twilight, sometimes twilight is used metaphorically to imply that something is losing strength and approaching its end. For example, very old people may be said to be "in the twilight of their lives". The collateral adjective for twilight is crepuscular, which may be used to describe the behavior of animals that are most active during this period.

Definitions by geometry

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Twilight occurs according to the solar elevation angle θs, which is the position of the geometric center of the Sun relative to the horizon. There are three established and widely accepted subcategories of twilight: civil twilight (nearest the horizon), nautical twilight, and astronomical twilight (farthest from the horizon).[2]

Civil twilight

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Midtown Manhattan during civil twilight, demonstrating blue hour

Civil twilight is the period of time for which the geometric center of the Sun is between the horizon and 6° below the horizon.[3][4][5]

Civil twilight is the period when enough natural light remains so that artificial light in towns and cities is not needed.[6] In the United States' military, the initialisms BMCT (begin morning civil twilight, i.e., civil dawn) and EECT (end evening civil twilight, i.e., civil dusk) are used to refer to the start of morning civil twilight and the end of evening civil twilight, respectively.[7] Civil dawn is preceded by morning nautical twilight and civil dusk is followed by evening nautical twilight.

Civil twilight in a small town in the Mojave Desert

Under clear weather conditions, civil twilight approximates the limit at which solar illumination suffices for the human eye to clearly distinguish terrestrial objects. Enough illumination renders artificial sources unnecessary for most outdoor activities. At civil dawn and at civil dusk, sunlight clearly defines the horizon while the brightest stars and planets can appear. As observed from the Earth (see apparent magnitude), sky-gazers know Venus, the brightest planet, as the "morning star" or "evening star" because they can see it during civil twilight.[6]

Although civil dawn marks the time of the first appearance of civil twilight before sunrise, and civil dusk marks the time of the first disappearance of civil twilight after sunset, civil twilight statutes typically denote a fixed period after sunset or before sunrise (most commonly 20–30 minutes) rather than how many degrees the Sun is below the horizon. Examples include when drivers of automobiles must turn on their headlights (called lighting-up time in the UK), when hunting is restricted, or when the crime of burglary is to be treated as nighttime burglary, which carries stiffer penalties in some jurisdictions.

The period may affect when extra equipment, such as anti-collision lights, is required for aircraft to operate.[8] In the US, civil twilight for aviation is defined in Part 1.1 of the Federal Aviation Regulations (FARs)[9] as the time listed in the American Air Almanac.[10]

Nautical twilight

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Evening nautical twilight on Lake Ontario, Canada

Nautical twilight occurs when the geometric center of the Sun is between 12° and 6° below the horizon.[11][3][5]

Long exposure of nautical twilight in a small town in the Mojave Desert

After nautical dusk and before nautical dawn, sailors cannot navigate via the horizon at sea as they cannot clearly see the horizon.[1][failed verification] At nautical dawn and nautical dusk, the human eye finds it difficult, if not impossible, to discern traces of illumination near the sunset or sunrise point of the horizon (first light after nautical dawn but before civil dawn and nightfall after civil dusk but before nautical dusk).[citation needed]

At the beginning of nautical twilight, artificial lighting must be used to see terrestrial objects clearly.

Sailors can take reliable star sightings of well-known stars, during the stage of nautical twilight when they can distinguish a visible horizon for reference (i.e. after astronomic dawn or before astronomic dusk).

Under good atmospheric conditions with the absence of other illumination, during nautical twilight, the human eye may distinguish general outlines of ground objects but cannot participate in detailed outdoor operations.[12]

Nautical twilight has military considerations as well. The initialisms BMNT (begin morning nautical twilight, i.e. nautical dawn) and EENT (end evening nautical twilight, i.e. nautical dusk) are used and considered when planning military operations. A military unit may treat BMNT and EENT with heightened security, e.g. by "standing to", for which everyone assumes a defensive position.

Astronomical twilight

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Long exposure of astronomical twilight in a small town in the Mojave Desert
Astronomical twilight (dusk) with a crescent moon, as seen from Kuala Lumpur, Malaysia

Astronomical twilight is defined as when the geometric center of the Sun is between 18° and 12° below the horizon.[3][4][2] During astronomical twilight, the sky is dark enough to permit astronomical observation of point sources of light such as stars, except in regions with more intense skyglow due to light pollution, moonlight, auroras, and other sources of light. Some critical observations, such as of faint diffuse items such as nebulae and galaxies, may require observation beyond the limit of astronomical twilight. Theoretically, the faintest stars detectable by the naked eye (those of approximately the sixth magnitude) will become visible in the evening at astronomical dusk, and become invisible at astronomical dawn.[13]

Times of occurrence

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World map showing limiting latitudes of each type of twilight during the solstices

Between day and night

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Observers within about 48°34' of the Equator can view twilight twice each day on every date of the year between astronomical dawn, nautical dawn, or civil dawn, and sunrise as well as between sunset and civil dusk, nautical dusk, or astronomical dusk. This also occurs for most observers at higher latitudes on many dates throughout the year, except those around the summer solstice. However, at latitudes closer than 8°35' (between 81°25’ and 90°) to either Pole, the Sun cannot rise above the horizon nor sink more than 18° below it on the same day on any date, so this example of twilight cannot occur because the angular difference between solar noon and solar midnight is less than 17°10’.

Observers within 63°26' of the Equator can view twilight twice each day on every date between the month of the autumnal equinox and the month of vernal equinox between astronomical dawn, nautical dawn, or civil dawn, and sunrise as well as between sunset and civil dusk, nautical dusk, or astronomical dusk, i.e., from September 1 to March 31 of the following year in the Northern Hemisphere and from March 1 to September 30 in the Southern Hemisphere.

The nighttime/twilight boundary solar midnight's latitude varies depending on the month:

  • In January or July, astronomical dawn to sunrise or sunset to astronomical dusk occurs at latitudes less than 48°50' North or South, because then the Sun's declination is less than 23°10' from the Equator;
  • In February or August, astronomical dawn to sunrise or sunset to astronomical dusk occurs at latitudes less than 53°47' North or South, because then the Sun's declination is less than 18°13' from the Equator;
  • In March or September before the equinoxes, astronomical dawn to sunrise or sunset to astronomical dusk occurs at latitudes less than 63°26' North or South, because before the equinoxes the Sun's declination is then less than 8°34' from the Equator;
  • During the equinoxes, astronomical dawn to sunrise or sunset to astronomical dusk occurs at latitudes less than 72°00' North or South, because during the equinoxes the Sun is crossing the Equator line;
  • In March or September after the equinoxes, astronomical dawn to sunrise or sunset to astronomical dusk occurs at latitudes less than 67°45' North or South, because after the equinoxes the Sun's declination is then less than 4°15' from the Equator;
  • In April or October, astronomical dawn to sunrise or sunset to astronomical dusk occurs at latitudes less than 57°09' North or South, because the Sun's declination is then less than 14°51' from the Equator;
  • In May or November, astronomical dawn to sunrise or sunset to astronomical dusk occurs at latitudes less than 50°03' North or South, because the Sun's declination is then less than 21°57' from the Equator;

Lasting from one day to the next

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Timelapse video of twilight and sunrise in Gjøvik in February 2021

At latitudes greater than about 48°34' North or South, on dates near the summer solstice (June 21 in the Northern Hemisphere or December 21 in the Southern Hemisphere), twilight can last from sunset to sunrise, since the Sun does not sink more than 18 degrees below the horizon, so complete darkness does not occur even at solar midnight. These latitudes include many densely populated regions of the Earth, including the entire United Kingdom and other countries in northern Europe and even parts of central Europe. This also occurs in the Southern Hemisphere, but occurs on December 21. This type of twilight also occurs between one day and the next at latitudes within the polar circles shortly before and shortly after the period of midnight sun. The summer solstice in the Northern Hemisphere is on June 21st, while the summer solstice in the Southern Hemisphere is on December 21st.

Between one night and the next

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In Arctic and Antarctic latitudes in wintertime, the polar night only rarely produces complete darkness for 24 hours each day. This can occur only at locations within about 5.5 degrees of latitude of the Pole, and there only on dates close to the winter solstice. At all other latitudes and dates, the polar night includes a daily period of twilight, when the Sun is not far below the horizon. Around winter solstice, when the solar declination changes slowly, complete darkness lasts several weeks at the Pole itself, e.g., from May 11 to July 31 at Amundsen–Scott South Pole Station.[a] North Pole has the experience of this from November 13 to January 29.

Solar noon at civil twilight during a polar night: between about 67°24' and 72°34' north or south.

Solar noon at nautical twilight during a polar night: between about 72°34' and 78°34' north or south.

Solar noon at astronomical twilight during a polar night: between about 78°34' and 84°34' north or south.

Solar noon at night during a polar night: between approximately 84°34' and exactly 90° north or south.

Lasting for 24 hours

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At latitudes greater than 81°25' North or South, as the Sun's angular elevation difference is less than 18 degrees, twilight can last for the entire 24 hours. This occurs for one day at latitudes near 8°35’ from the Pole and extends up to several weeks the further toward the Pole one goes. This happens both near the North Pole and near the South Pole. The only permanent settlement to experience this condition is Alert, Nunavut, Canada, where it occurs from February 22–26, and again from October 15–19.

Duration

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The number of daylight hours depends on the latitude and time of year. Each pole has continuous daylight near its summer solstice.
Carpet plot of sunshine at latitude 70° north
Carpet plot of sunshine at latitude 50° north
Carpet plot of sunshine at the equator
Twilight at Paranal Observatory in Chile[15]

The duration of twilight depends on the latitude and the time of the year. The apparent travel of the Sun occurs at the rate of 15 degrees per hour (360° per day), but sunrise and sunset happen typically at oblique angles to the horizon and the actual duration of any twilight period will be a function of that angle, being longer for more oblique angles. This angle of the Sun's motion with respect to the horizon changes with latitude as well as the time of year (affecting the angle of the Earth's axis with respect to the Sun).

At Greenwich, England (51.5°N), the duration of civil twilight will vary from 33 minutes to 48 minutes, depending on the time of year. At the equator, civil twilight can last as little as 24 minutes. This is true because at low latitudes the Sun's apparent movement is perpendicular to the observer's horizon. But at the poles, civil twilight can be as long as 2–3 weeks. In the Arctic and Antarctic regions, twilight (if there is any) can last for several hours. There is no astronomical twilight at the poles near the winter solstice (for about 74 days at the North Pole and about 80 days at the South Pole). As one gets closer to the Arctic and Antarctic circles, the Sun's disk moves toward the observer's horizon at a lower angle. The observer's earthly location will pass through the various twilight zones less directly, taking more time.

Within the polar circles, twenty-four-hour daylight is encountered in summer, and in regions very close to the poles, twilight can last for weeks on the winter side of the equinoxes. Outside the polar circles, where the angular distance from the polar circle is less than the angle which defines twilight (see above), twilight can continue through local midnight near the summer solstice. The precise position of the polar circles, and the regions where twilight can continue through local midnight, varies slightly from year to year with Earth's axial tilt. The lowest latitudes at which the various twilights can continue through local midnight are approximately 60.561° (60°33′43″) for civil twilight, 54.561° (54°33′43″) for nautical twilight and 48.561° (48°33′43″) for astronomical twilight.[16][17]

Lowest-latitude twilight observed at local midnight by month
Month Midnight Sun Civil Nautical Astronomical
January 66°00’36.0”S 60°50’36.0”S 54°50’36.0”S 48°50’36.0”S
February 70°57’19.5”S 65°47’19.5”S 59°47’19.5”S 53°47’19.5”S
March
(before equinox)
80°36’07.0”S 75°26’07.0”S 69°26’07.0”S 63°26’07.0”S
March
(after equinox)
84º55’53.0”N 79º45’53.0”N 73º45’53.0”N 67º45’53.0”N
April 74°19’50.5”N 69°09’50.5”N 63°09’50.5”N 57°09’50.5”N
May 67°13’25.0”N 62°03’25.0”N 56°03’25.0”N 50°03’25.0”N
June 65°43’38.6”N 60°33’38.6”N 54°33’38.6”N 48°33’38.6”N
July 66°00’36.0”N 60°50’36.0”N 54°50’36.0”N 48°50’36.0”N
August 70°57’19.5”N 65°47’19.5”N 59°47’19.5”N 53°47’19.5”N
September
(before equinox)
80°36’07.0”N 75°26’07.0”N 69°26’07.0”N 63°26’07.0”N
September
(after equinox)
84º55’53.0”S 79º45’53.0”S 73º45’53.0”S 67º45’53.0”S
October 74°19’50.5”S 69°09’50.5”S 63°09’50.5”S 57°09’50.5”S
November 67°13’25.0”S 62°03’25.0”S 56°03’25.0”S 50°03’25.0”S
December 65°43’38.6”S 60°33’38.6”S 54°33’38.6”S 48°33’38.6”S

These are the largest cities of their respective countries where the various twilights can continue through local solar midnight:

Although Helsinki, Oslo, Stockholm, Tallinn, and Saint Petersburg also enter into nautical twilight after sunset, they do have noticeably lighter skies at night during the summer solstice than other locations mentioned in their category above, because they do not go far into nautical twilight. A white night is a night with only civil twilight which lasts from sunset to sunrise.[18]

At the winter solstice within the polar circle, twilight can extend through solar noon at latitudes below 72.561° (72°33′43″) for civil twilight, 78.561° (78°33′43″) for nautical twilight, and 84.561° (84°33′43″) for astronomical twilight.

On other planets

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Twilight on Mars is longer than on Earth, lasting for up to two hours before sunrise or after sunset. Dust high in the atmosphere scatters light to the night side of the planet. Similar twilights are seen on Earth following major volcanic eruptions.[19]

In culture

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Twilight in the Wilderness by Frederic Edwin Church, a 19th century masterpiece of nature and landscape depiction.

Christianity

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American Benedictine monks around an Easter fire preparing to light the Paschal candle prior to Easter Vigil Mass

In Christian practice, "vigil" observances often occur during twilight on the evening before major feast days or holidays. For example, the Easter Vigil is held in the hours of darkness between sunset on Holy Saturday and sunrise on Easter Day – most commonly in the evening of Holy Saturday or midnight – and is the first celebration of Easter, days traditionally being considered to begin at sunset.[citation needed]

Hinduism

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Hinduism prescribes the observance of certain practices during twilight, a period generally called sandhya.[20] The period is also called by the poetic form of gōdhūḷi in Sanskrit, literally 'cow dust', referring to the time cows returned from the fields after grazing, kicking up dust in the process.[21] Many rituals, such as Sandhyavandanam and puja, are performed at the twilight hour. Consuming food is not advised during this time. According to some adherents, asuras are regarded to be active during these hours. One of the avatars of Vishnu, Narasimha, is closely associated with the twilight period. According to Hindu scriptures, an asura king, Hiranyakashipu, performed penance and obtained a boon from Brahma that he could not be killed during day or night, neither by human nor animal, neither inside his house nor outside. Vishnu appeared in a half-man half-lion form (neither human nor animal), and ended Hiranyakashipu's life at twilight (neither day nor night) while he was placed in the threshold of his house (neither inside nor outside).[22]

Islam

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Twilight is important in Islam as it determines when certain universally obligatory prayers are to be recited. Morning twilight is when morning prayers (Fajr) are done, while evening twilight is the time for evening prayers (Maghrib prayer). Also during Ramadhan, the time for suhoor (morning meal before fasting) ends at morning twilight, while fasting ends after sunset. There is also an important discussion in Islamic jurisprudence between "true dawn" and "false dawn".[citation needed]

Judaism

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In Judaism, twilight is considered neither day nor night; consequently it is treated as a safeguard against encroachment upon either. It can be considered a liminal time. For example, the twilight of Friday is reckoned as Sabbath eve, and that of Saturday as Sabbath day; and the same rule applies to festival days.[23]

See also

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References

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Footnotes

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Further reading

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Twilight is the period of daylight illumination produced by when the Sun is below the horizon, as from the upper atmosphere is scattered, providing partial light and after sunset. It is classified into three types—civil twilight (Sun 0–6° below horizon), nautical twilight (6–12° below), and astronomical twilight (12–18° below)—with durations varying from about 20–30 minutes near the to several hours at mid-latitudes, and extending for weeks or months in polar regions where the Sun remains close to the horizon during solstices. This phenomenon also occurs on other celestial bodies, such as with atmospheres (e.g., Mars) and moons, influenced by their , , and atmospheric composition. Twilight has held cultural and symbolic significance across societies, often representing transition, ambiguity, or spiritual moments in religion, , , and modern media.

Definitions and Types

Geometric Basis

Twilight refers to the period of partial illumination of the Earth's surface following sunset or preceding sunrise, resulting from scattered by molecules in the upper atmosphere while the Sun's disk remains below the horizon. This scattering occurs because direct no longer reaches the observer's location, but the upper atmospheric layers continue to be illuminated, redirecting diffuse light toward the ground. The geometric basis of twilight is defined by the solar depression angle θs\theta_s, which measures the angular position of the Sun's geometric center below the observer's horizon, equivalent to the negative of the solar elevation angle or the zenith distance minus 90°. Atmospheric refraction alters the apparent position of the Sun, effectively raising it by approximately 0.57° near the horizon due to the bending of light rays through denser lower air layers, which must be accounted for in precise calculations. Rayleigh scattering serves as the primary mechanism for the diffuse illumination of the twilight sky, where interacts with air molecules much smaller than the of visible , preferentially scattering shorter blue wavelengths while allowing longer red wavelengths to penetrate deeper. This process produces the characteristic gradient of sky brightness from the horizon toward the , with the intensity decreasing as the Sun's depression increases and fewer atmospheric paths contribute to . Twilight transitions end when θs\theta_s reaches specific geometric thresholds, such as -18° for astronomical twilight, beyond which residual sky glow becomes negligible for most observations; these angles incorporate the correction to define the Sun's true geometric position. Civil, nautical, and astronomical twilight represent applications of progressively deeper depression angles (-6°, -12°, and -18°, respectively). An illustrative diagram of twilight geometry typically depicts the observer at ground level, with the horizon line, the Sun's center at a depression angle θs\theta_s below it, and layered atmospheric strata showing incoming sunlight grazing the upper layers for scattering toward the observer; arrows indicate ray paths bent by refraction and scattered light paths contributing to sky illumination.

Civil Twilight

Civil twilight is the brightest phase of twilight, occurring when the geometric center of the Sun is between 0° and 6° below the horizon. This period marks the transition from full daylight to night, with morning civil twilight—also known as civil dawn—beginning when the Sun reaches 6° below the horizon and ending at sunrise, while evening civil twilight, or civil dusk, starting at sunset and concluding when the Sun descends to 6° below the horizon. The 6° threshold is geometrically defined to account for the Sun's angular diameter and atmospheric refraction, ensuring the solar disk is fully obscured while maintaining adequate surface illumination. During civil twilight, natural illumination remains sufficient for most outdoor activities without artificial lighting, allowing clear visibility of the horizon and surrounding landscape features. Distant objects are discernible, and brighter celestial bodies such as become observable against the fading sky. This light level supports everyday tasks like walking or reading outdoors, as well as recreational activities such as completing the last few holes of golf in diminishing light, as the overall brightness is comparable to a well-lit day. Practically, civil twilight delineates the boundaries for civil dawn and civil dusk, serving key roles in sectors like , where operations do not require position lights due to the ambient . In , it provides optimal soft lighting for capturing landscapes and portraits, enhancing color contrasts without harsh shadows. Daily scheduling in , transportation, and also relies on this phase for timing activities that bridge day and night. The sky's appearance evolves during civil twilight, shifting from a overhead to deeper orange and red hues near the horizon, a result of preferentially removing shorter blue wavelengths from the sunlight passing through a longer atmospheric path. Under clear skies with scattered clouds, —beams of sunlight piercing through gaps—may appear, adding dramatic contrast to the scene. At mid-latitudes, this phase typically lasts 20 to 40 minutes, shorter in summer and longer in winter due to the Sun's path.

Nautical Twilight

Nautical twilight is the intermediate phase of evening or morning twilight that occurs when the geometric center of the Sun is between 6° and 12° below the horizon. This period follows civil twilight and precedes astronomical twilight, providing a transitional illumination level suitable for specific observational tasks. During this time, the sky darkens further, but sufficient light remains for distinguishing key features against the horizon. Visibility during nautical twilight allows for the horizon to remain discernible, though it becomes less distinct than in civil twilight, posing challenges for precise navigation. Brighter stars, known as nautical stars—primarily those of magnitude 1 to 3 used in celestial navigation—become visible, enabling sailors to take sextant sights by aligning these stars with the horizon. Fainter stars up to approximately magnitude 4 can also be observed toward the end of this phase under clear conditions, facilitating the identification of constellations for orientation. This twilight phase holds significant practical applications in maritime and contexts. It defines nautical dawn, the beginning of morning nautical twilight when the Sun reaches 12° below the horizon, and nautical dusk, the end of evening nautical twilight at the same depression. Critical for sailors, it provides the window to identify the before full darkness, allowing safe passage and accurate positioning via celestial methods. In operations, terms like Begin Morning Nautical Twilight (BMNT)—the start of morning nautical twilight at 12° solar depression—and End Evening Nautical Twilight (EENT) mark periods for low-light activities such as . Atmospheric during nautical twilight results in a darker sky, as shorter blue wavelengths dominate the remaining sunlight refracted through the upper atmosphere. This effect contributes to the "," a brief interval prized in for its deep blue hues and soft lighting, often overlapping with the early or late stages of nautical twilight. The term "nautical twilight" originates from historical naval practices, where almanacs like provided tables of twilight times to aid in timing safe voyages and celestial observations at sea.

Astronomical Twilight

Astronomical twilight is the darkest phase of twilight, occurring when the geometric center of the Sun is between 12° and 18° below the horizon. This period follows nautical twilight and marks the transition to full astronomical night, during which the sky illumination from scattered diminishes to levels comparable to or below . At this stage, the horizon becomes indiscernible to the , and the overall sky brightness approaches that of true night under non-light-polluted conditions. During astronomical twilight, visibility conditions allow for the observation of fainter celestial objects, with stars up to the 6th magnitude becoming discernible as the phase progresses. This makes it an ideal time for astronomical observations of dim sources, such as distant galaxies or nebulae, particularly in locations free from artificial interference, as the remaining solar glow no longer significantly hinders performance. The , a faint diffuse glow from interplanetary dust reflecting sunlight, may become faintly visible toward the end of this phase in clear, . In practical terms, astronomical twilight defines the boundaries of astronomical dusk in the evening and dawn in the morning, serving as the operational threshold for professional observatories to commence or conclude nighttime observing sessions. For instance, telescopes at sites like typically open their domes at the start of astronomical twilight to maximize dark-sky time. This phase ends when the Sun reaches 18° below the horizon, at which point sunlight no longer substantially illuminates the upper atmosphere, and any residual sky glow arises primarily from natural phenomena such as or aurorae. Technically, with the Sun's center at -18°, the of the solar disk is fully obscured below the horizon, further minimizing direct interference with observations.

Occurrence and Duration

Daily and Seasonal Timing

Evening twilight commences immediately at sunset and advances through the phases of civil dusk, nautical dusk, and astronomical dusk until the onset of full astronomical night, when the Sun is more than 18° below the horizon. This progression reflects the gradual dimming of scattered sunlight in the atmosphere as the Sun descends further beneath the horizon. Morning twilight, in contrast, concludes at sunrise and originates from the reverse sequence, beginning with astronomical dawn when the Sun is 18° below the horizon, followed by nautical dawn and civil dawn. These phases mark the increasing illumination prior to direct sunlight, with civil, nautical, and astronomical twilight serving as distinct intervals based on the Sun's angular depression. Seasonal variations in twilight timing arise from Earth's orbital position and , resulting in shorter twilight periods near the equinoxes—when the Sun's path is more perpendicular to the horizon—and longer periods near the solstices, when the path is shallower. At the , twilight occurs twice daily with minimal seasonal fluctuation, as day and night remain approximately equal throughout the year. Latitude significantly influences twilight timing, with higher experiencing extended transitions due to the Sun's more oblique approach to the horizon; around solstices, evening twilight at these locations can merge seamlessly with morning twilight, producing continuous dim illumination. The timing of these events is fundamentally derived from solar position calculations, which account for Earth's of 23.44° and its effects on the Sun's throughout the year.

Duration Factors

The duration of twilight phases is primarily influenced by an observer's , the time of year, and the constant rate of . At higher latitudes, twilight lasts longer because the Sun's path across the sky is more parallel to the horizon, requiring a greater for the Sun to traverse the necessary depression angles defining each phase. Near the , the Sun descends nearly vertically, resulting in shorter durations. Seasonally, at mid-latitudes, twilight extends longer during summer months due to the Sun's higher , which increases the obliquity of its path relative to the horizon, while winter durations are shorter as the path is steeper. Earth's rotation at a steady rate of 15° per hour provides the baseline temporal scale for these changes. Mathematically, the approximate duration of a twilight phase can be estimated as the spanned by the Sun's center (e.g., 6° for civil twilight from horizon to -6° depression) divided by rate: duration ≈ ( / 15° per hour). This yields about for civil twilight under equatorial conditions, but the effective angular path lengthens with and seasonal , extending the time accordingly. Representative examples illustrate these variations: at the , civil twilight typically lasts 20-30 minutes year-round, while at 50° , it can extend to 1-2 hours during periods. In mid-latitude regions such as Guangzhou, China (23°N; approximately 20-25 minutes), Shanghai, China (31°N; 25-30 minutes), and Beijing, China (40°N; 30-40 minutes), durations vary by season (longer in summer) and are influenced by weather conditions such as atmospheric refraction and aerosols. Atmospheric conditions also play a secondary role in modifying durations. bends sunlight, effectively lifting the apparent and slightly prolonging twilight by 1-2 minutes on average, with greater variability at high latitudes where the Sun skims the horizon. Aerosols in the atmosphere, such as those from natural dust or , enhance and can subtly extend perceived twilight by maintaining illumination longer; major volcanic eruptions, like the 1883 event, inject stratospheric sulfates that increase , leading to brighter and potentially longer-lasting twilights observable globally for months. Global patterns of average civil twilight durations vary systematically by bands, as summarized below (values represent typical ranges across seasons, with summer maxima noted where applicable):
Latitude BandAverage Duration (minutes)Notes
0°-20° (Equatorial)20-30Minimal seasonal variation
20°-40° (Tropical/Subtropical)25-40Slightly longer in summer
40°-60° (Mid/High)30-90Up to 1-2 hours in summer at higher end
60°+ (Polar)60-180+Merges with daylight in summer; shorter in winter
These patterns are derived from astronomical computations accounting for geometric and rotational factors.

Polar Twilight Phenomena

In polar regions within the and Circles, approximately 66.5° north and , the Earth's leads to extreme variations in solar illumination, where twilight phenomena deviate significantly from equatorial patterns. During the summer , the Sun remains above the horizon for 24 hours or more, but transitional zones experience prolonged twilight that can extend from apparent sunset to sunrise, creating periods of continuous dim light rather than full darkness. Conversely, in winter , the Sun stays below the horizon for extended durations, yet civil, nautical, or astronomical twilight may persist around midday, providing faint illumination from atmospheric of . These effects intensify closer to the poles, where twilight can last the entire day or night cycle during solstices. White nights exemplify continuous civil twilight at high latitudes south of the , such as in , where the Sun dips just below the horizon during summer, preventing full darkness and maintaining a soft, pervasive glow for weeks. This phenomenon occurs between roughly late May and mid-July in locations like or , with the Sun's maximum depression limited to less than 6° below the horizon at , ensuring the sky never achieves nautical or astronomical darkness. In these regions, the extended twilight supports outdoor activities into the "night" hours but disrupts traditional day-night cycles. Twilight circles define latitudinal boundaries where persistent twilight dominates around solstices, as the Sun's path skims near the horizon without fully setting or rising. The civil twilight circle, around 60°34' N/S, marks where the Sun remains above -6° elevation all night during , producing unending civil twilight; further south, the nautical twilight circle at about 54° N/S allows continuous nautical twilight, and the astronomical twilight circle near 48°33' N/S ensures the sky never reaches full astronomical darkness. These circles shift slightly with the Earth's but create prolonged dim light in polar-adjacent zones, enhancing the ethereal quality of high-latitude summers. The persistent glow of polar twilight poses challenges for astronomical observations, as scattered elevates sky brightness, reducing contrast for faint celestial objects and limiting deep-sky imaging or to brief windows during . However, this same dim illumination enhances aurora viewing by providing a subtle backdrop that highlights the auroral curtains without overwhelming their colors, particularly during strong geomagnetic activity when auroras remain visible against the twilight. Historical polar explorers frequently documented encounters with endless twilight, underscoring its psychological and navigational impacts. During Roald Amundsen's 1910–1912 Antarctic expedition, his team described the "grey twilight" persisting for weeks as they approached the , with the sudden return of direct sunlight dazzling after acclimation to the dim, unending light. Similarly, Ernest Shackleton's 1914–1917 recorded nine hours of twilight daily during winter months aboard the , providing "good light at noon" amid the pack ice but evoking isolation in the perpetual half-light. Fridtjof Nansen's 1893–1896 Fram expedition accounts in Farthest North detail the "endless twilight" during drifts, where faint horizon glows blurred day-night boundaries, testing endurance in the transitional seasons.

Twilight on Other Celestial Bodies

Twilight on Planets

Twilight on other planets differs significantly from Earth's due to variations in atmospheric composition, , and planetary rotation rates, which alter the and duration of during the transition from day to night. On Mars, twilight periods are notably longer than on Earth, often extending up to two hours after sunset or before sunrise, primarily because the planet's dust-laden atmosphere sunlight over greater distances. This dust, suspended high in the atmosphere, creates a persistent glow similar to conditions on Earth following major volcanic eruptions that loft aerosols into the . Venus experiences prolonged and hazy twilight effects owing to its thick atmosphere, which diffuses and shrouds the surface in a dim, reddish illumination resembling perpetual twilight. Surface observations from Soviet landers in the and revealed this orange-red glow, resulting from the atmosphere's filtering of shorter wavelengths and the planet's extreme surface pressures and temperatures. The slow rotation of further extends these phases, with a sidereal day lasting 243 days, causing the Sun to traverse the sky gradually and prolonging the civil twilight period dramatically compared to 's 24-hour cycle. For gas giants like , twilight analogs occur in the upper cloud layers rather than on a solid surface, where scatters through and other aerosols. However, the planet's rapid rotation—completing a day in about 10 hours—results in brief transition phases, with twilight lasting only minutes as sweeps across the atmosphere at high speeds. Similar dynamics apply to other gas giants such as Saturn, , and , where fast rotations (ranging from 10 to 16 hours) minimize the duration of these illuminated boundary regions in the outer atmospheric layers. Orbital and rotational influences play a key role across planets; slower rotations, as on Venus, dramatically lengthen twilight by reducing the angular speed of the Sun's apparent motion, while faster rotations on gas giants compress these periods. Mission data from NASA's Perseverance rover, equipped with the Mars Environmental Dynamics Analyzer (MEDA), has confirmed extended civil twilight visibility on Mars through observations of atmospheric dust and mesospheric clouds during dawn and dusk, spanning multiple sols and providing insights into light scattering behaviors.

Twilight on Moons and Exoplanets

On Earth's , the absence of an atmosphere results in an abrupt transition from day to night at sunrise and sunset, with no gradual twilight phase as passes directly from full illumination to complete darkness without . This stark shift occurs because the lacks the air molecules that bend and diffuse on , leading to immediate darkness once the Sun dips below the horizon. However, during the lunar night, faint illumination from Earthshine— reflected off Earth's oceans, clouds, and land surfaces onto the Moon's unlit side—can mimic a subtle twilight glow, particularly visible during phases. This reflected , known as , provides the primary source of diffuse illumination on the 's dark hemisphere, varying in intensity based on Earth's phase as seen from the . Among Jupiter's moons, Io experiences an extended effective twilight due to the persistent glow from its hundreds of active volcanoes, which emit and sulfurous plumes that illuminate the surface beyond direct . These volcanic eruptions, driven by from Jupiter's gravity, produce lava flows and gas emissions that create a hazy, glowing atmosphere of , faintly and prolonging dim conditions at the terminator. In contrast, Europa's highly reflective icy surface, with an of approximately 0.64, causes sharp contrasts between lit and shadowed regions, effectively shortening any transitional twilight phase as bounces directly off the frozen terrain without significant atmospheric diffusion. Europa's tenuous oxygen offers minimal , resulting in abrupt light changes similar to the Moon's, though radiation-induced from Jupiter's can add a faint greenish glow to the nightside. For exoplanets, hot Jupiters—gas giants orbiting very close to their stars—are often tidally locked, with one hemisphere in perpetual daylight and the other in endless night, creating a narrow, intense twilight zone where temperatures drop rapidly over short distances. This locking synchronizes rotation with , leading to extreme that compresses the twilight region into a band of high winds and , with durations on the order of minutes rather than hours. In exoplanets, models suggest twilight durations akin to Earth's, influenced by , which drives seasonal variations in illumination and scattering; for instance, a 23-degree tilt like Earth's can extend twilight by up to 20-30 minutes through obliquity-induced day length changes. Theoretical simulations of twilight zones on systems like , a compact multi-planet setup around an , predict extended dim periods on inner worlds, where synchronous rotation and thin atmospheres could create perpetual twilight bands lasting hours due to the star's low luminosity. As of September 2025, (JWST) observations indicate that is unlikely to have a thick - or Mars-like atmosphere but may possess a thinner one or water vapor, potentially affecting in its terminator zone. These models incorporate orbital resonances and effects to forecast terminator regions on planets like , potentially habitable with surface temperatures allowing liquid water in transitional zones. Observational challenges in studying exoplanet twilights stem from the rarity of direct imaging, relying instead on phase curve analyses of light variations, where stellar spots and instrumental noise obscure subtle dimming signals indicative of atmospheric . Inferred twilight effects appear as gradual flux changes in transit light curves, but contamination from the host star's activity complicates detection, limiting precision to systems with high signal-to-noise ratios like hot Jupiters.

Cultural and Symbolic Significance

In Religion

In , twilight holds significance in liturgical practices, particularly through the , a night-time ceremony originating in early Church traditions that begins at twilight to symbolize Christ's and the triumph of light over darkness. This vigil, historically devoted to baptisms and communal prayer, marks the transition from death to new life, with the lighting of the representing the risen Christ dispelling the shadows of . In monastic traditions, twilight aligns with , the evening prayer that serves as a liminal moment for reflection on the day's end and preparation for rest, fostering spiritual introspection during this threshold between day and night. Hinduism regards twilight as a sacred interval for rituals, most notably in the practice of sandhya vandana, a daily devotional act performed at dawn and dusk to honor the divine through mantras and offerings, emphasizing the balance of vital energies during these transitional periods. In , the deity , an avatar of , emerges at twilight from a palace pillar to slay the demon king , circumventing the demon's boon of invulnerability by acting in this neither-day-nor-night liminal space, thus protecting devotee and restoring cosmic order. In , twilight defines key prayer times, with Fajr commencing at true dawn's twilight when the sun is 18 degrees below the horizon, and Maghrib beginning immediately after sunset, both calculated using astronomical twilight angles to ensure precise observance of the five daily prayers. During , fasting concludes at Maghrib with , the breaking of the fast, marking the end of the day's spiritual discipline as the sun dips below the horizon. Judaism associates twilight, termed bein ha-arbayim or "between the evenings," with pivotal rituals, such as the lamb sacrifice on the 14th of , performed in the early evening shortly after sunset until total darkness sets in, symbolizing redemption and transition. This timing also governs the onset of the and festivals, where candles are lit 18 minutes to welcome the holy day before full twilight arrives, ensuring the sacred period begins without delay. Across these faiths, twilight embodies a sacred threshold between day and night, a liminal space invoking divine intervention, renewal, and precise ritual timing often informed by geometric solar calculations.

In , Art, and Modern Media

In Romantic literature, twilight frequently serves as a symbol of melancholic transition, evoking the impermanence of existence amid shifting light and mood. captures this in poems like "Mutability," underscoring themes of change and introspection. Similarly, in "," twilight "blazed" marks perceptual shifts during evening scenes, blending awe with a sense of fleeting beauty. Gothic novels further associate twilight with eternal dusk in vampire lore, portraying it as the liminal realm where the undead awaken. Bram Stoker's Dracula (1897) depicts the Count active at night, his castle shrouded in dim light that blurs mortality and immortality, heightening the horror of unending night. Impressionist art harnesses twilight's ephemeral colors to explore light's transformative effects, prioritizing atmosphere over detail. Claude Monet's San Giorgio Maggiore at Dusk (1908) renders Venice's church in deepening violets and blues, capturing the hazy interplay of fading sunlight and emerging shadows to convey serenity and transience. In Renaissance works, twilight symbolizes liminality as a threshold between earthly and divine realms, often through celestial motifs that evoke ambiguity and spiritual passage, as seen in paintings integrating dusk skies to represent human vulnerability. Modern media amplifies twilight's motifs for emotional and atmospheric depth. The Twilight saga films (2008–2012) set their narrative in the perpetually overcast Forks, Washington, where endless dusk enables vampires' daylight avoidance while symbolizing romantic limbo and eternal youth. In sci-fi horror, John Carpenter's The Thing (1982) leverages Antarctica's polar twilight—prolonged low light during endless nights—to intensify isolation and paranoia, framing the alien threat against a backdrop of unrelenting dimness. Photography techniques during twilight's "golden hour" (warm post-sunrise or pre-sunset glow) and "blue hour" (cool nautical twilight) exploit diffused light for vibrant, romantic compositions, softening contrasts to evoke intimacy or mystery. Twilight embodies as a boundary state in creative works, fostering romance through its intimate, uncertain glow while hinting at apocalyptic closure in narratives of decline. In Japanese culture, yozakura—cherry blossom viewing at twilight during festivals—celebrates sakura's brief bloom under evening lights, symbolizing life's transience and harmonious reflection.

References

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