Temperature Converter — All 7 Scales Simultaneously Live
Type any temperature in any unit — all other scales update instantly in real-time. Or pick a conversion mode for step-by-step formulas
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Isaac Newton, 1700
°F = (°C × 9/5) + 32 · K = °C + 273.15 · °R = (°C + 273.15) × 9/5
All 7 Temperature Scales — Simultaneously
Key Conversions at a Glance
Complete Conversion Table with Formulas
Detailed Results — All Units
Relative Temperature — Visual Comparison
Step-by-Step Conversion Working
What Is Temperature? — Complete Science Guide
Understanding temperature, thermodynamic scales, absolute zero, and why different units exist
Temperature is a physical quantity that expresses the degree of hotness or coldness of a body. On the molecular level, temperature is a direct measure of the average kinetic energy of the particles in a substance — the faster the particles move and vibrate, the higher the temperature. This definition, rooted in statistical mechanics and thermodynamics, explains why there is a lower limit to temperature (absolute zero) but no theoretical upper limit.
Temperature is measured using a thermometric scale — a standardised system with defined reference points and equal-interval divisions. All common temperature scales are defined by two fixed reference points: the freezing point of pure water at standard atmospheric pressure (101.325 kPa), and either the boiling point of water or absolute zero. The interval between these points is then divided into equal units called degrees.
The three scales in everyday use are Celsius (used by most of the world), Fahrenheit (used primarily in the United States), and Kelvin (the SI unit of thermodynamic temperature used in science and engineering). Kelvin is unique in that it is an absolute scale — zero Kelvin represents the complete absence of thermal energy, meaning it has no negative values.
Celsius (°C) — The Global Standard
Developed by Swedish astronomer Anders Celsius in 1742. Originally defined with 0°C at water's boiling point and 100°C at freezing — later inverted by Linnaeus. Today, 0°C = freezing point of water, 100°C = boiling point at sea level. Used as the primary temperature scale in 195 countries. Formally defined since 1954 relative to the Kelvin scale: °C = K − 273.15.
Fahrenheit (°F) — The US Standard
Proposed by German physicist Daniel Gabriel Fahrenheit in 1724. Originally defined with 0°F as the coldest temperature achievable with a salt-ice mixture, and 96°F as body temperature. Modern definition: 32°F = water's freezing point, 212°F = water's boiling point. Used daily in the United States, Bahamas, Cayman Islands, and Palau. The 180° interval between freeze and boil corresponds to 100° in Celsius.
Kelvin (K) — The Scientific Standard
Named after Lord Kelvin (William Thomson), who proposed the absolute temperature scale in 1848. The SI unit of thermodynamic temperature. Kelvin uses the same degree size as Celsius but starts at absolute zero (0 K = −273.15°C). The Kelvin scale has no degree symbol — just "K". Used in all scientific, astrophysical, and engineering calculations. Absolute zero (0 K) is the theoretical minimum temperature where molecular kinetic energy equals zero.
Rankine (°R or °Ra) — Engineering Absolute
Proposed by Scottish engineer William Rankine in 1859. An absolute temperature scale (like Kelvin) but uses Fahrenheit-size degrees. 0°R = absolute zero = −459.67°F. Water freezes at 491.67°R and boils at 671.67°R. Used primarily in thermodynamic engineering in the United States — particularly in aeronautical and combustion engineering where absolute temperature is required in Fahrenheit-unit equations.
Réaumur (°Ré) — The Wine Scale
Proposed by René Antoine Ferchault de Réaumur in 1730. Water freezes at 0°Ré and boils at 80°Ré (the scale is divided into 80 degrees). Historically important in France and Germany, where it was used in food production — particularly in cheese-making, brewing, and jam production. Still occasionally referenced in European food science. Conversion: °C = °Ré × 1.25.
Newton (°N) — Isaac Newton's Scale
Created by Isaac Newton around 1700, published posthumously in 1701. Water freezes at 0°N and the boiling point of water is 33°N. Newton is said to have used linseed oil as his thermometric fluid. Historically significant as one of the first attempts at a systematic temperature scale. Rarely used today outside historical contexts. Conversion: °C = °N × 100/33.
Delisle (°De) — The Inverted Scale
Created by French astronomer Joseph-Nicolas Delisle in 1732. Uniquely, the Delisle scale runs in the opposite direction — higher numbers mean colder temperatures. Water boils at 0°De and freezes at 150°De. Absolute zero is at 559.725°De. Used in Russia until the mid-18th century before being replaced by Celsius. A historical curiosity — the only common scale where temperature decreases as the number increases.
Absolute Zero — The Ultimate Lower Limit
Absolute zero (0 K, −273.15°C, −459.67°F) is the theoretical lower limit of temperature — the point at which all thermal motion of atoms would cease. It is physically unattainable: the third law of thermodynamics states that no finite series of processes can reduce the temperature of a system to absolute zero. The coldest measured object in the universe is a lab-created Bose-Einstein condensate — approximately 100 picokelvin (0.0000000001 K) above absolute zero.
Complete Temperature Conversion Formulas — All 42 Combinations
Every formula for converting between all 7 temperature scales, with worked examples
With 7 temperature scales, there are 42 possible directed conversions (7 × 6). All of them can be derived from a single intermediate conversion through Celsius: any unit → Celsius → any other unit. Below are the key direct formulas grouped by source unit.
| From → To | Formula | Example (100°C / 212°F) |
|---|---|---|
| °C → °F | °F = (°C × 9/5) + 32 | 100°C → (100×1.8)+32 = 212°F |
| °C → K | K = °C + 273.15 | 100°C → 100+273.15 = 373.15 K |
| °C → °R | °R = (°C + 273.15) × 9/5 | 100°C → 373.15×1.8 = 671.67°R |
| °C → °Ré | °Ré = °C × 4/5 | 100°C → 100×0.8 = 80°Ré |
| °C → °N | °N = °C × 33/100 | 100°C → 100×0.33 = 33°N |
| °C → °De | °De = (100 − °C) × 3/2 | 100°C → (100−100)×1.5 = 0°De |
| °F → °C | °C = (°F − 32) × 5/9 | 212°F → (212−32)×5/9 = 100°C |
| °F → K | K = (°F − 32) × 5/9 + 273.15 | 212°F → 373.15 K |
| K → °C | °C = K − 273.15 | 373.15K → 373.15−273.15 = 100°C |
| K → °F | °F = (K − 273.15) × 9/5 + 32 | 373.15K → 212°F |
| °R → K | K = °R × 5/9 | 671.67°R → 671.67×5/9 = 373.15 K |
| °R → °C | °C = (°R − 491.67) × 5/9 | 671.67°R → 100°C |
| °Ré → °C | °C = °Ré × 5/4 | 80°Ré → 80×1.25 = 100°C |
| °N → °C | °C = °N × 100/33 | 33°N → 33×100/33 = 100°C |
| °De → °C | °C = 100 − (°De × 2/3) | 0°De → 100−0 = 100°C |
Real-Life Temperature Reference — Key Landmarks in All Scales
Important temperatures in everyday life, science, cooking, medicine, and nature
Temperature in Science, Cooking, Medicine & the Universe
From absolute zero to the temperature of the Sun's core — a complete guide to extreme temperatures
Temperature spans an extraordinary range in the natural and scientific world — from the theoretical coldness of absolute zero to the scorching plasma of stellar cores. Understanding the extremes of the temperature scale illuminates fundamental physics, chemistry, biology, and engineering.
Cryogenics — Ultra-Low Temperatures
Cryogenics studies matter at temperatures below −150°C (123 K). Liquid nitrogen (−196°C / 77 K) is used for food preservation, dermatology, and electronics cooling. Liquid helium (−269°C / 4 K) enables MRI machines and particle accelerators. At temperatures near 0 K, quantum effects dominate: superfluidity, superconductivity, and Bose-Einstein condensates emerge. The coldest natural temperature in the known universe is the Boomerang Nebula at 1 K (−272°C).
High-Temperature Science
Tungsten melts at 3,422°C (6,192°F) — the highest melting point of any pure element. Plasma, the fourth state of matter, forms above ~10,000°C. The surface of the Sun is ~5,500°C (9,932°F); its core reaches 15,000,000°C (27,000,000°F). Nuclear fusion requires temperatures of 100,000,000°C (100 million°C) to occur. The Big Bang's temperature 10⁻⁴³ seconds after inception was approximately 10³² Kelvin.
Cooking Temperature Guide
Temperature is critical in cooking chemistry. Maillard reaction (browning): 140–165°C. Caramelisation: 160–180°C. Bread baking: 190–230°C. Deep frying: 175–190°C. Protein denaturation begins ~60°C — why eggs solidify. Pasteurisation: 72°C for 15 seconds. Safe minimum internal temperatures: poultry 74°C, beef 63°C, fish 63°C. Sugar syrup stages: soft ball 112°C → hard crack 149°C → caramel 170°C.
Medical Temperature Reference
Normal human body temperature: 36.1–37.2°C (97–99°F), with an average of 37°C (98.6°F). Core temperature varies by 0.5°C through the day (lowest at 4 AM, highest at 4 PM). Fever: >38°C (100.4°F). Hyperthermia/heat stroke: >40°C (104°F) — medical emergency. Hypothermia: <35°C (95°F) — life-threatening below 32°C. Clinical thermometers measure in tenths of a degree because small changes are diagnostically significant.
Earth's Temperature Extremes
Hottest recorded air temperature: 56.7°C (134°F) at Furnace Creek, Death Valley, USA (1913). Coldest recorded air temperature: −89.2°C (−128.6°F) at Vostok Station, Antarctica (1983). The global average surface temperature is approximately 15°C (59°F). Earth's core temperature is estimated at 5,100–6,000°C — similar to the Sun's surface. The troposphere temperature drops ~6.5°C per 1,000 m of altitude.
Industrial & Materials Temperature
Iron melts at 1,538°C (2,800°F); steel castings require 1,560–1,600°C. Glass softens at ~700°C. Common industrial processes: steam turbines operate at 500–600°C; gas turbine combustion chambers reach 1,300–1,500°C. Rocket engines: liquid oxygen (LOX) fuel engines reach 3,300°C in the combustion chamber. Portland cement kiln: 1,400–1,500°C. Aluminium smelting: 660°C. The temperature-resistance properties of materials determine their engineering applications.
Frequently Asked Questions — Temperature Conversion
Expert answers to the most searched temperature conversion and science questions