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Scale of temperature
Scale of temperature
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Equivalent temperatures in the Kelvin (K), Celsius (°C), and Fahrenheit (°F) scales

Scale of temperature is a methodology of calibrating the physical quantity temperature in metrology. Empirical scales measure temperature in relation to convenient and stable parameters or reference points, such as the freezing and boiling point of water. Absolute temperature is based on thermodynamic principles: using the lowest possible temperature as the zero point, and selecting a convenient incremental unit.

Celsius, Kelvin, and Fahrenheit are common temperature scales. Other scales used throughout history include Rankine, Rømer, Newton, Delisle, Réaumur, Gas mark, Leiden, and Wedgwood.

Technical definition

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The zeroth law of thermodynamics describes thermal equilibrium between thermodynamic systems in form of an equivalence relation. Accordingly, the set of all thermal systems may be divided into a quotient set of equivalence classes, denoted as , where any element of collects all systems that are in thermal equilibrium with one another.

If the set has cardinality at most (the cardinality of the continuum), then one can construct an injective function into the real numbers by which every thermal system has a parameter – a specific real number – associated with it: the property of temperature. By definition, when two systems are in thermal equilibrium, they belong to the same equivalence class, hence to the same element of , and are assigned the same temperature. Conversely, two systems not in thermal equilibrium belong to different equivalence classes, and since is injective, they are assigned different temperatures.

Temperature depends on the specific choice of , and any suitable – any specific way of assigning numerical values for temperature – establishes a scale of temperature.[1][2][3] In practical terms, a temperature scale is always based on usually a single physical property of a simple thermodynamic system, called a thermometer, that defines a scaling function for mapping the temperature to the measurable thermometric parameter. Such temperature scales that are purely based on measurement are called empirical temperature scales.

The second law of thermodynamics provides a fundamental, natural definition of thermodynamic temperature starting with a null point of absolute zero. A scale for thermodynamic temperature is established similarly to the empirical temperature scales, however, needing only one additional fixing point.

Empirical scales

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Empirical scales are based on the measurement of physical parameters that express the property of interest to be measured through some formal, most commonly a simple linear, functional relationship. For the measurement of temperature, the formal definition of thermal equilibrium in terms of the thermodynamic coordinate spaces of thermodynamic systems, expressed in the zeroth law of thermodynamics, provides the framework to measure temperature.

All temperature scales, including the modern thermodynamic temperature scale used in the International System of Units, are calibrated according to thermal properties of a particular substance or device. Typically, this is established by fixing two well-defined temperature points and defining temperature increments via a linear function of the response of the thermometric device. For example, both the old Celsius scale and Fahrenheit scale were originally based on the linear expansion of a narrow mercury column within a limited range of temperature,[4] each using different reference points and scale increments.

Different empirical scales may not be compatible with each other, except for small regions of temperature overlap. If an alcohol thermometer and a mercury thermometer have the same two fixed points, namely the freezing and boiling point of water, their readings will not agree with each other except at the fixed points, as the linear 1:1 relationship of expansion between any two thermometric substances may not be guaranteed.

Empirical temperature scales are not reflective of the fundamental, microscopic laws of matter. Temperature is a universal attribute of matter, yet empirical scales map a narrow range onto a scale that is known to have a useful functional form for a particular application. Thus, their range is limited. The working material only exists in a form under certain circumstances, beyond which it no longer can serve as a scale. For example, mercury freezes below 234.32 K, so temperatures lower than that cannot be measured in a scale based on mercury. Even ITS-90, which interpolates among different ranges of temperature, has a range of only 0.65 K to approximately 1358 K (−272.5 °C to 1085 °C).

Ideal gas scale

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When pressure approaches zero, all real gas will behave like ideal gas, that is, pV of a mole of gas relying only on temperature. Therefore, we can design a scale with pV as its argument. Of course any bijective function will do, but for convenience's sake a linear function is the best. Therefore, we define it as[5]

The ideal gas scale is in some sense a "mixed" scale. It relies on the universal properties of gas, a big advance from just a particular substance. But still it is empirical since it puts gas at a special position and thus has limited applicability—at some point no gas can exist. One distinguishing characteristic of ideal gas scale, however, is that it precisely equals thermodynamical scale when it is well defined (see § Equality to ideal gas scale).

International temperature scale of 1990

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ITS-90 is designed to represent the thermodynamic temperature scale (referencing absolute zero) as closely as possible throughout its range. Many different thermometer designs are required to cover the entire range. These include helium vapor pressure thermometers, helium gas thermometers, standard platinum resistance thermometers (known as SPRTs, PRTs or Platinum RTDs) and monochromatic radiation thermometers.

Although the Kelvin and Celsius scales are defined using absolute zero (0 K) and the triple point of water (273.16 K and 0.01 °C), it is impractical to use this definition at temperatures that are very different from the triple point of water. Accordingly, ITS–90 uses numerous defined points, all of which are based on various thermodynamic equilibrium states of fourteen pure chemical elements and one compound (water). Most of the defined points are based on a phase transition; specifically the melting/freezing point of a pure chemical element. However, the deepest cryogenic points are based exclusively on the vapor pressure/temperature relationship of helium and its isotopes whereas the remainder of its cold points (those less than room temperature) are based on triple points. Examples of other defining points are the triple point of hydrogen (−259.3467 °C) and the freezing point of aluminum (660.323 °C).

Thermometers calibrated per ITS–90 use complex mathematical formulas to interpolate between its defined points. ITS–90 specifies rigorous control over variables to ensure reproducibility from lab to lab. For instance, the small effect that atmospheric pressure has upon the various melting points is compensated for (an effect that typically amounts to no more than half a millikelvin across the different altitudes and barometric pressures likely to be encountered). The standard even compensates for the pressure effect due to how deeply the temperature probe is immersed into the sample. ITS–90 also draws a distinction between "freezing" and "melting" points. The distinction depends on whether heat is going into (melting) or out of (freezing) the sample when the measurement is made. Only gallium is measured while melting, all the other metals are measured while the samples are freezing.

There are often small differences between measurements calibrated per ITS–90 and thermodynamic temperature. For instance, precise measurements show that the boiling point of VSMOW water under one standard atmosphere of pressure is actually 373.1339 K (99.9839 °C) when adhering strictly to the two-point definition of thermodynamic temperature. When calibrated to ITS–90, where one must interpolate between the defining points of gallium and indium, the boiling point of VSMOW water is about 10 mK less, about 99.974 °C. The virtue of ITS–90 is that another lab in another part of the world will measure the very same temperature with ease due to the advantages of a comprehensive international calibration standard featuring many conveniently spaced, reproducible, defining points spanning a wide range of temperatures.

OV

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OV is a specialized scale used in Japan to measure female basal body temperature for fertility awareness. The range of 35.5 °C (OV 0) to 38.0 °C (OV 50) is divided into 50 equal parts.[6]

Celsius scale

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Celsius (known until 1948 as centigrade) is a temperature scale that is named after the Swedish astronomer Anders Celsius (1701–1744), who developed a similar temperature scale two years before his death. The degree Celsius (°C) can refer to a specific temperature on the Celsius scale as well as a unit to indicate a temperature interval (a difference between two temperatures).

From 1744 until 1954, 0 °C was defined as the freezing point of water and 100 °C was defined as the boiling point of water, both at a pressure of one standard atmosphere.[citation needed]

Although these defining correlations are commonly taught in schools today, by international agreement, between 1954 and 2019 the unit degree Celsius and the Celsius scale were defined by absolute zero and the triple point of VSMOW (specially prepared water). This definition also precisely related the Celsius scale to the Kelvin scale, which defines the SI base unit of thermodynamic temperature with symbol K. Absolute zero, the lowest temperature possible, is defined as being exactly 0 K and −273.15 °C. Until 19 May 2019, the temperature of the triple point of water was defined as exactly 273.16 K (0.01 °C). This means that a temperature difference of one degree Celsius and that of one kelvin are exactly the same.

On 20 May 2019, the kelvin was redefined so that its value is now determined by the definition of the Boltzmann constant rather than being defined by the triple point of VSMOW. This means that the triple point is now a measured value, not a defined value. The newly defined exact value of the Boltzmann constant was selected so that the measured value of the VSMOW triple point is exactly the same as the older defined value to within the limits of accuracy of contemporary metrology. The degree Celsius remains exactly equal to the kelvin, and 0 K remains exactly −273.15 °C.

Thermodynamic scale

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Thermodynamic scale differs from empirical scales in that it is absolute. It is based on the fundamental laws of thermodynamics or statistical mechanics instead of some arbitrary chosen working material. Besides it covers full range of temperature and has simple relation with microscopic quantities like the average kinetic energy of particles (see equipartition theorem). In experiments ITS-90 is used to approximate thermodynamic scale due to simpler realization.

Definition

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Lord Kelvin devised the thermodynamic scale based on the efficiency of heat engines as shown below:

The efficiency of an engine is the work divided by the heat introduced to the system or

where wcy is the work done per cycle. Thus, the efficiency depends only on qC/qH.

Because of Carnot theorem, any reversible heat engine operating between temperatures T1 and T2 must have the same efficiency, meaning, the efficiency is the function of the temperatures only:

In addition, a reversible heat engine operating between temperatures T1 and T3 must have the same efficiency as one consisting of two cycles, one between T1 and another (intermediate) temperature T2, and the second between T2 and T3. This can only be the case if

Specializing to the case that is a fixed reference temperature: the temperature of the triple point of water. Then for any T2 and T3,

Therefore, if thermodynamic temperature is defined by

then the function f, viewed as a function of thermodynamic temperature, is

and the reference temperature T1 has the value 273.16. (Of course any reference temperature and any positive numerical value could be used—the choice here corresponds to the Kelvin scale.)

Equality to ideal gas scale

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It follows immediately that

Substituting Equation 3 back into Equation 1 gives a relationship for the efficiency in terms of temperature:

This is identical to the efficiency formula for Carnot cycle, which effectively employs the ideal gas scale. This means that the two scales equal numerically at every point.

Conversion table between different temperature scales

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Kelvin

Celsius

Fahrenheit

Rankine scale

Rømer scale

Newton scale

Delisle scale

Réaumur scale

See also

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Notes and references

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
A temperature scale is defined as a for measuring temperature, where specific reference points, such as the ice point and steam point, are assigned fixed numerical values to enable consistent quantification of thermal states. These scales provide a standardized framework for comparing temperatures across physical phenomena, from everyday to scientific experiments, by relating them to reproducible fixed points like phase transitions in substances. The most widely used temperature scales include the (°C), (°F), and (K) scales. The scale, adopted internationally for general use, sets the freezing point of at 0 °C and the at 100 °C under standard , making it intuitive for human-perceived temperatures. In contrast, the scale, primarily used , assigns 32 °F to 's freezing point and 212 °F to its , with a smaller degree interval (1 °C equals 1.8 °F). The scale serves as the (SI) base unit for temperature and is an starting at (0 K), the theoretical point where molecular motion ceases, equivalent to -273.15 °C. One interval matches one degree , but the scale avoids negative values in thermodynamic contexts, with the of defined at exactly 273.16 K for precise calibration. This absolute nature makes essential in physics and engineering for calculations involving and . Historically, temperature scales evolved from empirical observations, with early versions like the in the , but modern standards are governed by the International Temperature Scale of 1990 (ITS-90), which approximates the using platinum resistance thermometers and gas thermometers calibrated at defined fixed points. ITS-90 ensures global consistency in measurements from 0.65 to the highest achievable temperatures, supporting advancements in fields like and high-temperature materials.

Basic Principles

Technical Definition

Temperature in physics is fundamentally a measure of the average energy associated with the random motion of particles in a , encompassing translational, rotational, vibrational, and other . This concept arises from the and , where the TT is proportional to the average energy per degree of freedom, given by 12kBT\frac{1}{2} k_B T for each quadratic term in the energy (with kBk_B as the )./12%3A_Temperature_and_Kinetic_Theory/12.02%3A_Temperature_and_Temperature_Scales) A temperature scale is a standardized system for assigning ordered numerical values to the states of systems, enabling quantitative comparisons of hotness or coldness. These scales are calibrated using reproducible fixed points, such as the of water or phase transitions of pure substances, to define intervals between reference temperatures. The scale provides a way to interpolate and extrapolate measurements beyond the fixed points, ensuring consistency in scientific and practical applications./Book%3A_University_Physics_II_-Thermodynamics_Electricity_and_Magnetism(OpenStax)/01%3A_Temperature_and_Heat/1.02%3A_Thermometers_and_Temperature_Scales) Temperature scales can be classified as interval scales or ratio scales based on their measurement properties. Interval scales, such as the scale, have equal intervals between values but lack a true , meaning ratios of temperatures (e.g., one temperature being "twice as hot" as another) are not physically meaningful. Ratio scales, like the Kelvin scale, include an — the lowest possible temperature where thermal motion ceases—allowing meaningful ratios and multiples. This distinction is crucial in , where absolute scales align with the second law and calculations./01%3A_Introduction_to_Statistics/1.02%3A_Levels_of_Measurement) The development of standardized scales emerged in the 18th and 19th centuries to address inconsistencies in early thermometry for advancing and . Prior to , various arbitrary scales led to errors in scientific experiments and observations; for instance, the need for precise became evident during the formulation of the and steam engine efficiency studies in the . International agreements, such as those by the International Committee of Weights and Measures, established uniform scales to facilitate global research and engineering.

Properties of Temperature Scales

A temperature scale must exhibit monotonicity, ensuring that higher numerical values correspond to hotter states of a , thereby preserving the order of thermal intensities observed in . This arises from the fundamental ordering of hotness, where any empirical scale is defined as a that maps the sequence of increasingly hot bodies to increasing numerical values. For instance, in constructing such a scale, a thermometric (like the volume of a ) must vary continuously and monotonically with the degree of hotness to allow reliable comparisons. Linearity and additivity are essential for practical utility, requiring that equal intervals on the scale represent equal increments in differences, enabling arithmetic operations such as and of intervals. This interval scale property, first formalized in the , ensures that the difference between two temperatures is independent of the reference point, allowing consistent of changes across the scale. Additivity specifically means that the difference between points A and C equals the sum of differences from A to B and B to C, which underpins the of instruments using reproducible reference points. Transitivity in temperature comparisons is guaranteed by the zeroth law of thermodynamics, which states that if two systems are each in with a third, they are in with each other, implying they share the same . This transitive relation allows the definition of a unique for systems in , forming the basis for consistent ordering without cycles or inconsistencies in hotness assessments. Temperature is fundamentally an intensive , independent of the size or amount of the system, unlike extensive properties such as or that scale with . This distinguishes temperature as a measure of the average per degree of freedom in a system's molecules, ensuring it remains uniform across subsystems in equilibrium regardless of total or particle number. Fixed points play a crucial role in defining and calibrating scales by providing reproducible reference states where phase transitions occur at invariant temperatures, such as the of at 273.16 , which serves as the anchor for the scale. These points, including freezing or transitions of pure substances under standard conditions, allow the subdivision of the scale into equal intervals with high precision, ensuring international consistency in measurements as outlined in standards like the International Scale of 1990 (ITS-90).

Thermodynamic Temperature

Definition

The establishes the concept of , stating that if two systems are each in with a third system, then they are in with each other. This law defines as the property that determines whether systems are in , allowing for the consistent of across different systems. The second law of thermodynamics introduces as a related to , where for a reversible , the change in entropy dSdS is given by dS=dQrevTdS = \frac{dQ_\text{rev}}{T}, with dQrevdQ_\text{rev} as the reversible and TT as the absolute . This relation positions temperature as the reciprocal of the rate at which entropy changes with heat addition in reversible processes, forming the basis for the scale. Thermodynamic temperature is an absolute scale where values are positive, and absolute zero corresponds to the point where the entropy of a perfect crystal in its ground state is zero, implying no further decrease in entropy upon cooling. In 2019, the —the unit of this scale—was redefined by fixing the at k=1.380649×1023k = 1.380649 \times 10^{-23} J/K, decoupling it from empirical fixed points such as the of and linking it directly to fundamental physical constants. This redefinition ensures the scale's universality. is independent of any particular substance or measurement method, relying solely on thermodynamic principles rather than material properties. The scale serves as its practical realization in scientific and applications.

Kelvin Scale

The Kelvin scale serves as the (SI) implementation of , with the (symbol: K) designated as its base unit. Prior to the 2019 SI revision, the kelvin was defined as the temperature interval equal to 1/273.16 of the thermodynamic temperature at the of (approximately 0.01 °C). Following the redefinition effective May 20, 2019, the kelvin is now defined by fixing the kk to the exact value 1.380649×10231.380649 \times 10^{-23} J/K, thereby defining one kelvin as the temperature change corresponding to a increase of kTkT by this fixed amount, where TT is in kelvins. This redefinition ensures the kelvin's stability by tying it to fundamental physical constants rather than a specific material property. Absolute zero is fixed at 0 on the Kelvin scale, representing the point of minimum where molecular motion theoretically ceases, and the scale inherently prohibits negative temperatures. The triple point of , previously the defining anchor, now measures approximately 273.16 with a relative standard uncertainty of about 0.4 × 10^{-6}, serving as a practical . In scientific contexts, the Kelvin scale underpins key thermodynamic relations, notably the PV=nRTPV = nRT, where PP, VV, and nn relate through the R=8.314462618R = 8.314462618 J/(mol·K). This usage is prevalent in fields like chemistry and physics for calculations involving heat capacities, reaction equilibria, and , as the absolute nature of the scale aligns with entropy-based formulations. The Kelvin scale contrasts with the , another absolute temperature system used primarily in Anglo-American engineering; while both start at 0 for , the Rankine degree equals 5/9 of a , such that temperatures in Rankine are 9/5 times those in (e.g., 300 K = 540 °R). High-precision calibration of the Kelvin scale, especially at low temperatures, relies on primary thermometry methods like Johnson thermometry, which measures the random thermal fluctuations () in a conductor's voltage or current, proportional to temperature via kk, achieving uncertainties below 1 mK near 1 K and extending to sub-millikelvin regimes. This technique supports realizations across the scale without fixed points, complementing practical scales like ITS-90 for everyday . The Kelvin scale relates to the Celsius scale through a simple offset, with 0 °C defined as 273.15 K.

Empirical Temperature Scales

Ideal Gas Scale

The ideal gas temperature scale is an empirical scale that approximates by leveraging the behavior of gases assumed to follow the , particularly , which posits that for a fixed amount of gas at constant pressure, the volume VV is directly proportional to the absolute temperature TT: VTV \propto T. This proportionality allows temperature to be defined as T=(VV0)T0T = \left( \frac{V}{V_0} \right) T_0, where V0V_0 is the volume at a reference temperature T0T_0. In practice, the scale is calibrated using fixed points such as the ice point (0 °C) and steam point (100 °C) of water, with the temperature interval between them set to 100 units, and extrapolated linearly to at 0 K based on the observed volume contraction. The fundamental equation underlying this scale derives from the ideal gas law, PV=nRTPV = nRT, where PP is pressure, VV is volume, nn is the amount of substance, RR is the universal gas constant, and TT is the temperature in kelvins. Rearranging for temperature yields T=PVnRT = \frac{PV}{nR}, providing a direct measure of temperature proportional to the product of pressure and volume for a given amount of gas. To ensure the measurement approaches the true thermodynamic temperature and minimizes deviations from ideality, the limit as pressure approaches zero is taken, as low-pressure conditions suppress intermolecular forces, making the gas behave more ideally: T=273.16KlimP0(PPtr)T = 273.16 \, \mathrm{K} \lim_{P \to 0} \left( \frac{P}{P_\mathrm{tr}} \right), where PtrP_\mathrm{tr} is the pressure at the triple point of water (273.16 K). Despite its foundational role, the scale has limitations when applied to real gases, which deviate from ideal behavior at high pressures or low temperatures due to finite molecular volume and intermolecular attractions. These deviations are accounted for using corrections like the , (P+an2V2)(Vnb)=nRT\left(P + \frac{an^2}{V^2}\right)(V - nb) = nRT, where aa and bb are empirical constants representing attractive forces and molecular volume, respectively, highlighting the need for low-density conditions to maintain accuracy. The International Temperature Scale of 1990 (ITS-90) refines this approach with practical interpolation methods beyond pure gas thermometry.

International Temperature Scale of 1990

The International Temperature Scale of 1990 (ITS-90) serves as the prevailing international metrological standard for realizing and disseminating measurements in practical applications, closely approximating the scale across the range from 0.65 to 1357.77 . Adopted by the International Committee for Weights and Measures (CIPM) in 1989 and implemented effective January 1, 1990, it supersedes the International Practical Temperature Scale of 1968 (IPTS-68) and the Extension of the International Practical Temperature Scale to 1976 (EPT-76/90), enhancing precision, continuity, and reproducibility in calibration. The scale defines International Kelvin Temperatures (T90) and International Temperatures (t90) using a set of 17 defining fixed points and specified methods, ensuring high fidelity to absolute thermodynamic values while enabling routine laboratory realizations. ITS-90 establishes its reference framework through 17 carefully selected fixed points, primarily phase transitions that provide stable, reproducible temperature anchors. These include a vapor-pressure formulation for isotopes in the range 0.65 to 5 (calibrated at higher points), vapor-pressure points of equilibrium at approximately 17.035 and 20.27 , the triple points of equilibrium (13.8033 ), (24.5561 ), oxygen (54.3584 ), (83.8058 ), mercury (234.3156 ), and (273.16 ), the melting point of (302.9146 ), and the freezing points of metals such as (429.7485 ), tin (505.078 ), (692.677 ), aluminum (933.473 ), silver (1234.93 ), (1337.33 ), and (1357.77 ). These points are realized using sealed cells containing high-purity substances under controlled conditions, with assigned numerical values that deviate minimally from thermodynamic temperatures—typically by less than 1 mK for most points. Between these fixed points, ITS-90 employs range-specific procedures to derive temperatures with optimal accuracy and practicality. In the cryogenic range below 5 , temperatures are interpolated using vapor-pressure equations for helium isotopes, calibrated against the and other low-temperature fixed points. From 13.8033 to 1234.93 , capsule-standard or long-stem resistance thermometers (PRTs) are used, with deviation functions fitted to data from multiple fixed points in subranges such as 13.8033 to 273.16 (using , , oxygen, , mercury, and s) and 273.16 to 1234.93 (incorporating , , tin, , aluminum, and silver points). Above 1234.93 , relies on the Planck applied to optical or acoustic pyrometers, referenced to the silver, , and freezing points, extending the scale to higher temperatures where contact thermometry becomes impractical. The ITS-90 achieves an accuracy of 0.1 mK to a few millikelvins relative to the thermodynamic scale across its range, with realization uncertainties varying by method—for instance, 0.03 mK at the water triple point and up to 25 mK at the freezing point—while offering reproducibility better than 0.001 through standardized procedures. As of 2025, no major revisions to ITS-90 have been adopted by the CIPM, maintaining its status as the baseline standard; however, ongoing research by the Consultative Committee for Thermometry (CCT) explores extensions for sub-0.65 cryogenics using advanced gas thermometry and for temperatures beyond 1357.77 via improved radiation-based techniques to address emerging needs in quantum technologies and . Recent updates, such as the 2022 CCT estimates, provide improved values for differences between ITS-90 and thermodynamic temperatures below 335 .

Common Conventional Scales

Celsius Scale

The Celsius scale, also known as the centigrade scale, was proposed by Swedish astronomer in 1742 as a relative temperature scale based on the . In its original formulation, Celsius assigned 0° to the of and 100° to the freezing point at standard , dividing the interval into 100 equal degrees. This inversion was reversed in 1743 by French astronomer Jean-Pierre Christin, who proposed the modern configuration with the freezing point at 0° and the at 100°, facilitating intuitive everyday use. The scale defines 0°C as the ice point—the temperature at which pure freezes into ice at a of 1 standard atmosphere (101.325 kPa)—and 100°C as the steam point—the temperature at which boils into under the same conditions—with the interval subdivided into 100 degrees of equal size. This empirical definition, established in the International Practical Temperature Scale of 1948 (IPTS-48), provided a practical approximation to until refined in later scales. The Celsius scale relates to the absolute thermodynamic scale via the Kelvin temperature, where the zero point of Celsius corresponds to 273.15 , though full conversions are detailed elsewhere. As the standard metric temperature scale, is widely applied in for weather forecasts, in for recipe instructions, and in scientific contexts requiring relative measurements rather than absolute values, such as chemistry and experiments. The 9th General Conference on Weights and Measures (CGPM) in 1948 formally adopted "degree Celsius" as the official name, replacing "centigrade," and it has since become the legal standard in nearly all countries except the for non-scientific uses. For enhanced precision in metrology, the International Temperature Scale of 1990 (ITS-90) introduces variations to the conventional fixed points; notably, it replaces the point with the of water at exactly 0.01°C (273.16 K) as a primary reference, while the steam point is approximated through among multiple fixed points rather than direct , ensuring better alignment with thermodynamic values across a broader range. These adjustments minimize uncertainties in , particularly for industrial and research thermometry, without altering the everyday utility of the 0–100°C water-based interval.

Fahrenheit Scale

The Fahrenheit scale was proposed in 1724 by the Polish-German physicist (1686–1736), who was working as an instrument maker in . To establish his scale, Fahrenheit calibrated his mercury thermometers using three key reference points: 0°F for the lowest reproducible temperature he could achieve with a brine mixture of ice, water, and ammonium chloride (in a 1:1:1 ratio, known as the Amsterdam mixture); 32°F for the freezing point of pure water (an ice-and-water mixture in a 1:1 ratio); and approximately 96°F for average , measured under the armpit. This initial setup drew from earlier work, including Fahrenheit's adaptation of the Danish astronomer Ole Rømer's scale from around 1701, which he multiplied by four to create finer divisions while retaining similar reference points. The scale is defined with the ice point (freezing of water at standard atmospheric pressure) at 32°F and the steam point (boiling of water at 1 atm) at 212°F, resulting in 180 degrees between these fixed points—smaller intervals than the 100 degrees on the Celsius scale. Over time, the body temperature reference was adjusted to 98.6°F for greater accuracy, but the core fixed points of 32°F and 212°F, established by Fahrenheit's successors to preserve the degree size, became standard. These points provided a practical relative scale for everyday and scientific measurements in the 18th century, particularly in English-speaking regions where Fahrenheit's thermometers gained popularity through the Royal Society. Today, the Fahrenheit scale remains in use primarily for reporting, household appliances like ovens and refrigerators (e.g., freezers set to 0°F), and some contexts. In the , it appears occasionally alongside in forecasts but is not official. Its non-metric nature poses disadvantages, including conversion errors in international scientific and trade contexts, higher costs for dual-scale manufacturing in the US, and complications in global standardization efforts. The serves as the relative counterpart to the absolute , which uses the same degree size but shifts the zero point by adding an offset of 459.67 to Fahrenheit values to align with (-459.67°F = 0°R).

Rankine Scale

The is an absolute scale named after the Scottish and William John Macquorn Rankine, who proposed it in as a counterpart to the , defining 0°R as with the same degree interval size as Fahrenheit. This scale anchors temperatures to the absence of molecular motion at its zero point, providing a framework for absolute measurements in . Key fixed points on the include the point, defined as the equilibrium temperature of and at standard , at 491.67°R, and the point, the temperature of under the same conditions, at 671.67°R. These reference points align directly with 32°F and 212°F, respectively, facilitating compatibility with Fahrenheit-based systems while extending to absolute values. The scale is primarily applied in engineering fields, particularly in the United States, for thermodynamic calculations involving customary units, such as steam tables used in power generation and nuclear facility analyses. In these contexts, it supports evaluations of energy transfer, cycle efficiency, and property determinations like and for steam-water systems. The Rankine temperature relates to the scale by the formula TR=95TKT_R = \frac{9}{5} T_K, yielding larger numerical values owing to the finer Fahrenheit degree subdivision compared to the Celsius interval underlying . Adoption of the remains limited to imperial-unit environments in English-speaking regions, as the (SI) prioritizes the scale for global standardization in scientific and engineering practice.

Conversions Between Scales

Conversion Formulas

Temperature scales are related through linear transformations of the form T2=aT1+bT_2 = a T_1 + b, where aa and bb are constants specific to the pair of scales being converted. This general form arises because temperature scales differ in their zero points and unit sizes, but maintain proportionality for intervals away from the zero. For example, the conversion from to uses a=1a = 1 and b=273.15b = 273.15, reflecting that the degree sizes are identical while the zero points differ by the of water offset. The standard conversion from to is given by TK=tC+273.15,T_\mathrm{K} = t_{^\circ\mathrm{C}} + 273.15, where TKT_\mathrm{K} is the temperature in kelvins and tCt_{^\circ\mathrm{C}} is the temperature in degrees . This exact relation defines the scale relative to the scale, with the addition of 273.15 ensuring alignment at . Conversely, the to conversion is tC=TK273.15t_{^\circ\mathrm{C}} = T_\mathrm{K} - 273.15. For Fahrenheit and Celsius, the conversion accounts for both differing unit sizes (1°C = 1.8°F) and zero points. The formula from Fahrenheit to Celsius is tC=59(tF32),t_{^\circ\mathrm{C}} = \frac{5}{9} (t_{^\circ\mathrm{F}} - 32), and the reverse is tF=95tC+32.t_{^\circ\mathrm{F}} = \frac{9}{5} t_{^\circ\mathrm{C}} + 32. These derive from the fixed points: the ice point (freezing of water at 0°C = 32°F) and the steam point (boiling of water at 100°C = 212°F). To derive, note the interval between fixed points is 100°C = 180°F, so the scale factor is 180100=95\frac{180}{100} = \frac{9}{5}. Using the ice point as a reference, solve the linear equation tF=95tC+bt_{^\circ\mathrm{F}} = \frac{9}{5} t_{^\circ\mathrm{C}} + b; substituting 0°C = 32°F yields b=32b = 32. Similarly, for the reverse, tC=59tF+bt_{^\circ\mathrm{C}} = \frac{5}{9} t_{^\circ\mathrm{F}} + b'; using 32°F = 0°C gives b=59×32=1609b' = - \frac{5}{9} \times 32 = - \frac{160}{9}, but the standard form shifts to the subtracted 32 for simplicity. The , an absolute counterpart to , converts from via TR=95TK,T_\mathrm{R} = \frac{9}{5} T_\mathrm{K}, since the degree size matches (1 = 1.8°) and both start at . From , it is TR=tF+459.67,T_\mathrm{R} = t_{^\circ\mathrm{F}} + 459.67, where 459.67 is the equivalent of (-459.67° = 0°), derived from the - relation at zero: 0 = -459.67°, so adding this offset aligns the scales. The reverse conversions follow by rearranging these equations. These linear formulas handle negative temperatures without issue, as the transformations preserve the ordering and intervals across scales; for instance, -40°C equals -40°F, a coincidence from the specific coefficients. Absolute zero (0 K = 0°R) remains invariant under absolute scale conversions but shifts to negative values on conventional scales like Celsius (-273.15°C) and Fahrenheit (-459.67°F), emphasizing that conventional scales allow readings below their arbitrary zeros while absolute scales do not. Care must be taken in thermodynamic contexts, where only absolute scales (Kelvin, Rankine) are used to avoid negative values in equations like the ideal gas law.

Comparison Table

The following table presents equivalent temperatures at selected fixed points and reference values across the (K), (°C), (°F), and Rankine (°R) scales, based on standard definitions and conversions. These points include , the of water, the ice point, approximate , the of water at standard , and an example high temperature of 1000 K. Values are exact where defined by the (SI) post-2019 redefinition, with the scale serving as the .
DescriptionKelvin (K)Celsius (°C)Fahrenheit (°F)Rankine (°R)
Absolute zero0-273.15-459.670
Triple point of 273.160.0132.018491.68
Ice point (freezing of )273.15032491.67
Human body temperature (approx.)310.153798.6558.27
Boiling point of (at 1 )373.15100212671.67
High temperature example1000726.851340.331800
To read the table, note the consistent intervals: a change of 1 equals 1 °C, 1.8 °F, or 1.8 °R, but absolute values differ due to zero points—e.g., 100 °C corresponds exactly to 373.15 , 212 °F, and 671.67 °R. Precision reflects SI definitions, where the of is exactly 273.16 , and the ice point is defined as 0 °C = 273.15 (0.01 below the ); is an approximate physiological average.

References

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