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freezing point of cerium(III) sulfide

Input interpretation

cerium(III) sulfide | freezing point
cerium(III) sulfide | freezing point

Result

2450 °C (degrees Celsius)
2450 °C (degrees Celsius)

Unit conversions

2723 K (kelvins)
2723 K (kelvins)
4442 °F (degrees Fahrenheit)
4442 °F (degrees Fahrenheit)
4902 °R (degrees Rankine)
4902 °R (degrees Rankine)
1960 °Ré (degrees Réaumur)
1960 °Ré (degrees Réaumur)
1294 °Rø (degrees Rømer)
1294 °Rø (degrees Rømer)

Blackbody information

  perceived color |  peak wavelength | 1.064 µm (micrometers) peak frequency | 160.1 THz (terahertz)
perceived color | peak wavelength | 1.064 µm (micrometers) peak frequency | 160.1 THz (terahertz)

Corresponding main-sequence star properties

temperature class | M6 absolute magnitude | +12 (bolometric) mass | 0.1 M_☉ radius | 0.13 R_☉ luminosity | 8.3×10^-4 L_☉ B-V color index | 2.1 lifetime | 3.1 trillion yr end state | helium white dwarf
temperature class | M6 absolute magnitude | +12 (bolometric) mass | 0.1 M_☉ radius | 0.13 R_☉ luminosity | 8.3×10^-4 L_☉ B-V color index | 2.1 lifetime | 3.1 trillion yr end state | helium white dwarf

Examples of M6 main-sequence stars

V1365 Orionis | Gl 860 B
V1365 Orionis | Gl 860 B

Corresponding quantities

Thermodynamic energy E from E = kT:  | 23 ceV (centielectronvolts)
Thermodynamic energy E from E = kT: | 23 ceV (centielectronvolts)
Blackbody energy flux Φ from Φ = σT^4:  | 3.118×10^6 W/m^2 (watts per square meter)
Blackbody energy flux Φ from Φ = σT^4: | 3.118×10^6 W/m^2 (watts per square meter)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface:  | 4.031×10^7 lx (lux)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 4.031×10^7 lx (lux)