Astrophysics (Index)About

kelvin

(K)
(unit of temperature scale starting at absolute zero)

A kelvin (K) is a (SI) unit of temperature, generally used to indicate an amount of temperature above absolute zero, i.e., above the physical lower bound on temperatures. The unit size is borrowed from the degree Celsius (centigrade) temperature scale (which pins zero degrees Celsius to water's freezing temperature and 100 degrees Celsius to water's boiling point for a unit of 9/5 a degree Fahrenheit) but among SI efforts is a more careful definition, based upon measurable physical values such as the speed of light and the Planck constant. Unless explicitly referring to a temperature difference, a number of kelvins refers to that number of kelvins above absolute zero. Physical relations tend to be based upon temperature scaled from absolute zero and kelvins provide a convenient scale for the sciences.

kelvins Celsius Fahrenheit
0 -273.15° -459.67° absolute zero
255.372 -17.8°
273.15 32°
294.261 21.1° 70°
5778 5505° 9941° surface temperature of the Sun

Regarding writing style, the unit kelvin is not capitalized, but the abbreviation K is capitalized: not the usual practice for SI units, but presumably a means to avoid potential confusion with "k for kilo". The term Kelvin scale for referring to the temperature scale in kelvins is capitalized. Terms like "MK" for millions of kelvins (or "kK" for thousands) are used, but it seems to me they are often avoided and readers aren't used to them: mK (millikelvin) and μK (microkelvin) seem more common, seen when referring to temperatures below 1 K. Unlike Fahrenheit and Celsius/centigrade (and Rankine), kelvins are not referred to as degrees, i.e., you do not write 100°K but 100 K. Referring to kelvins "a type of degree" (e.g., saying "10 degrees Kelvin") was formerly the practice, but SI standardization efforts declared in 1967 that the unit is a kelvin rather than a degree kelvin, so you say "10 kelvins".


(unit,temperature,SI)
Further reading:
https://en.wikipedia.org/wiki/Kelvin
https://www.britannica.com/science/kelvin
https://www.nist.gov/si-redefinition/kelvin-introduction
https://www.bipm.org/en/publications/si-brochure

Referenced by pages:
2M1207
51 Eridani b
51 Pegasi b (51 Peg b)
55 Cancri e (55 Cnc e)
A-type star (A)
ACBAR
antenna temperature
Arcminute Microkelvin Imager (AMI)
B-type star (B)
black-body radiation
bolometer
Boltzmann constant (k)
brown dwarf (BD)
carbon burning
chromosphere
CNO cycle
cold gas
cold spot
cosmic neutrino background (CNB)
cryogenic spectroscopy
DESHIMA
Earth
electron degeneracy
electron volt (eV)
emission line
Epsilon Indi (ε Indi)
equilibrium temperature (Teq)
F-type star (F)
far infrared (FIR)
Fermi sea
FIRSST
G-type star (G)
GJ 1132 b
GJ 1214 b
greenhouse effect
H-R diagram (HRD)
HD 189733 b
HD 209458 b
HD 80606 b
helium burning
HI region (HI)
HII region (HII)
HITEMP
HITRAN
horizontal branch (HB)
HR 8799
ice giant
ideal gas law
infrared (IR)
Io
K-type star (K)
KAGRA
Kepler-1625b
Kepler-186f
KID
L-type star (L)
LHS 3844 b
lithium depletion boundary (LDB)
Local Bubble
LUVOIR
M-type star (M)
neon burning
neutral atomic hydrogen (HI)
NIRCam
nucleosynthesis
O-type star (O)
Origins Space Telescope (OST)
PG 1159 star
Planck units
post-AGB star (pAGB)
Proxima b
red dwarf
refractory material
rp-process
shell
SI
spectral class
spectral energy distribution (SED)
SPICA
stellar atmosphere
Strömgren sphere
supershell
T-type star (T)
transition region
triple alpha process
Venus
volatile material
WASP-12b
WASP-33b
WASP-43b
WASP-67b
water (H2O)
Wien's displacement law
WISE 0855-0714 (W0855)
Wolf-Rayet star
Y-type star (Y)
ZTF J1539+5027

Index