Langbahn Team – Weltmeisterschaft

Orders of magnitude (temperature): Difference between revisions

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|273.15 K||0 [[Celsius|°C]]||32 °F||align=left|melting point of [[water]] (at [[standard conditions for temperature and pressure|STP]])
|273.15 K||0 [[Celsius|°C]]||32 °F||align=left|melting point of [[water]] (at [[standard conditions for temperature and pressure|STP]])
|- bgcolor="#E0E0E0" align=right
|- bgcolor="#E0E0E0" align=right
|287 K||14 °C||57 °F||align=left|mean surface temperature of [[Earth]]
|287 K||14 °C||57 °F||align=left|mean surface temperature of the [[Earth]]
|- bgcolor="#E0E0E0" align=right
|- bgcolor="#E0E0E0" align=right
|293.15 K||20 °C||68 °F||align=left|room temperature
|293.15 K||20 °C||68 °F||align=left|room temperature

Revision as of 05:49, 4 April 2007

List of orders of magnitude for temperature
Factor Multiple Item
10−∞ absolute zero: free-bodies are still, no interaction within or without a thermodynamic system
10−30 particular speeds bound paths to exceed size and lifetime of the universe
(see least-energy in orders of magnitude (energy))
10−18 1 aK macroscopic teleportation of matter
10−15 1 fK atomic waves coherent over inches
atomic particles decoherent over inches
10−12 1 pK 100 pK, lowest temperature ever produced, during an experiment on nuclear magnetic ordering at Helsinki University of Technology's Low Temperature Lab
450 pK, lowest temperature sodium Bose-Einstein condensate gas ever achieved in the laboratory, at MIT[1]
10−9 1 nK 50 nK, Fermi melting point of potassium-40
Bose melting point of bosonic atomic gasses
Doppler-locked refrigerants in laser cooling and magneto-optical traps
10−6 1 μK nuclear demagnetization
10−3 1 mK radio excitations
2.5 mK, Fermi melting point of helium-3
cinetic dilution sorting of isotopes
adiabatic demagnetization of paramagnetic molecules
300 mK in evaporative cooling of helium-3
950 mK, melting point of helium
microwave excitations
100 1 K 1 K, temperature at the Boomerang nebula, the coldest natural environment known
1.5 K, melting point of overbound helium
2.19 K, lambda point of overbound superfluid helium
2.725 K, cosmic microwave background
4.1 K, superconductivity point of mercury
4.22 K, boiling point of bound helium
5.19 K, critical temperature of helium
7.2 K, superconductivity point of lead
9.3 K, superconductivity point of niobium
101 10 K Fermi melting point of valence electrons for superconductivity
14.01 K, melting point of bound hydrogen
20.28 K, boiling point of bound hydrogen
33 K, critical temperature of hydrogen
44 K, mean surface temperature of Pluto
53 K, mean surface temperature of Neptune
63 K, melting point of bound nitrogen
68 K, mean surface temperature of Uranus
77.35 K, boiling point of bound nitrogen
90.19 K, boiling point of bound oxygen
92 K, superconductivity point of Y-Ba-Cu-oxide (YBCO)
everyday substances near liquid air's temperature with incipient Fermi-condensate populations result in spontaneous luminescence, loss or lack of hysteresis, inductive and capacitive electronic moments that readily adsorb or expel or float upon unlike substances: [2]
102 100 K infrared excitations
165 K, glass point of supercooled water
183.75 K (–89.4 °C), coldest ground level air temperature recorded on Earth
273.15 K (0 °C), melting point of bound water
about 293 K, room temperature
373.15 K (100 °C), boiling point of bound water
647 K, critical point of superheated water
See detailed list below
103 1 kK visible light excitations
1170 K, large log fire flames
1670 K, blue candle flame
1808 K, melting point of bound iron (lower for steel)
1870 K, Bunsen burner flame
1900 K, the Space Shuttle Orbiter hull temperature in 8km/s dive
2013 K, boiling point of lead
2320 K, open hydrogen flame
3683 K, melting point of tungsten
3925 K, sublimation point of carbon
4160 K, melting point of bound hafnium carbide
4700 K, triple point of overbound carbon
5100 K, cyanogen-dioxygen flame
5516 K, dicyanoacetylene (carbon subnitride)-ozone flame
5650 K, Earth's Inner Core Boundary
5780 K, surface temperature of the Sun
5828 K, boiling point of tungsten
6000 K, mean temperature of the Universe 300,000 years after the Big Bang
7736 K, temperature at which a monatomic ideal gas has one electron volt of kinetic energy
ultraviolet excitations
anionic sparks
104 10 kK 10 kK, surface temperature of Sirius A
10-15 kK, in mononitrogen recombination
25 kK, mean temperature of the Universe 10,000 years after the Big Bang
28 kK, in record cationic lightning over Earth
32 kK, surface temperature of Sirius B
37 kK, in proton-electron reactions
about 300 kK, estimated temperature 17 meters from Little Boy's detonation
Fermi boiling point of valence electrons
X-ray excitations
106 1 MK γ-ray excitations
5 MK, temperature of the Sun's corona
13.6 MK, temperature at Sun's core
100 MK, temperature needed for controlled nuclear fusion
109 1 GK 1 GK, temperature 100 seconds after the Big Bang
3 GK, electron-positron reactions
10 GK, estimated temperature in supernova explosions
10 GK, temperature 1 second after the Big Bang
1012 1 TK 0.5–1.2 TK, Fermi melting point of quarks into quark-gluon plasma
3-5 TK, proton-antiproton reactions
Z0 electronuclear excitations
10 TK, temperature 100 microseconds after the Big Bang
300–900 TK, proton-nickel conversions in the Tevatron's Main Injector
1015 1 PK .3–2.2 PK, proton-antiproton collisions in the Tevatron's Main Injector
1018 1 EK 2–13 EK, temperature at heavy nuclear conversions in the Large Hadron Collider
1021 1 ZK heart of galactic clusters-mergers
1024 1 YK 0.5–7 YK at Oh-My-God particular collisions
1027 grand symmetry-breaking unified fieldly excitations
temperature 10−35 seconds after the Big Bang
1030 1.4×1032 K, Planck temperature of micro black holes
temperature 5×10−44 seconds after the Big Bang
1033 all fieldly excitations
Landau poles
extradimensional gauge freedom

Detailed list of temperatures from 100 K to 1000 K

Kelvins Degrees
Celsius
Degrees
Fahrenheit
Condition
100 K -173.15 °C -279.67 °F
125 K -148 °C -234.4 °F superconductivity point of Tl-Ba-Cu-oxide
138 K -135 °C -211 °F superconductivity point of Hg-Tl-Ba-Ca-Cu-oxide
143 K -130 °C -202 °F mean "surface" temperature of Saturn
152 K -121 °C -185.8 °F mean "surface" temperature of Jupiter
184 K -89 °C -128.6 °F coldest natural surface temperature recorded on Earth
194.6 K -78.5 °C -109.3 °F sublimation point of carbon dioxide (dry ice)
210 K -63 °C -81.4 °F mean surface temperature of Mars
234.32 K -38.83 °C -37.9 °F melting point of mercury
255.37 K -17.78 °C 0 °F coldest brine-ice solution found by Fahrenheit
273.15 K 0 °C 32 °F melting point of water (at STP)
287 K 14 °C 57 °F mean surface temperature of the Earth
293.15 K 20 °C 68 °F room temperature
310 K 37 °C 98.6 °F human body temperature
331 K 58 °C 136.4 °F hottest natural surface temperature recorded on Earth
373.15 K 100 °C 212 °F boiling point of water
400 K 127 °C 260.6 °F hottest temperature of Concorde nose tip
452 K 179 °C 354.2 °F mean surface temperature of Mercury
600.65 K 327.50 °C 621.5 °F melting point of lead
737 K 464 °C 867.2 °F mean surface temperature of Venus
755 K 482 °C 900 °F temperature of a typical electric oven on the self-cleaning cycle
933.47 K 660.32 °C 1220.6 °F melting point of aluminium
1000 K 727.15 °C 1340.87 °F

Circumstances where water naturally occurs in liquid form are shown in light grey.

References

  1. ^ http://www.cbc.ca/stories/2003/09/11/cold_sodium030911
  2. ^ http://1911encyclopedia.org/Liquid_Gases "Liquid Gases". Encyclopædia Britannica, 11th edition: Classic Encyclopedia. (1911, 2006)