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freezing point of lutetium(III) oxide

Input interpretation

lutetium(III) oxide | freezing point
lutetium(III) oxide | freezing point

Result

2510 °C (degrees Celsius)
2510 °C (degrees Celsius)

Unit conversions

2783 K (kelvins)
2783 K (kelvins)
4550 °F (degrees Fahrenheit)
4550 °F (degrees Fahrenheit)
5010 °R (degrees Rankine)
5010 °R (degrees Rankine)
2008 °Ré (degrees Réaumur)
2008 °Ré (degrees Réaumur)
1325 °Rø (degrees Rømer)
1325 °Rø (degrees Rømer)

Blackbody information

  perceived color |  peak wavelength | 1.041 µm (micrometers) peak frequency | 163.6 THz (terahertz)
perceived color | peak wavelength | 1.041 µm (micrometers) peak frequency | 163.6 THz (terahertz)

Corresponding main-sequence star properties

temperature class | M6 absolute magnitude | +12 (bolometric) mass | 0.11 M_☉ radius | 0.13 R_☉ luminosity | 8.9×10^-4 L_☉ B-V color index | 2.0 lifetime | 2.8 trillion yr end state | helium white dwarf
temperature class | M6 absolute magnitude | +12 (bolometric) mass | 0.11 M_☉ radius | 0.13 R_☉ luminosity | 8.9×10^-4 L_☉ B-V color index | 2.0 lifetime | 2.8 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:  | 24 ceV (centielectronvolts)
Thermodynamic energy E from E = kT: | 24 ceV (centielectronvolts)
Blackbody energy flux Φ from Φ = σT^4:  | 3.402×10^6 W/m^2 (watts per square meter)
Blackbody energy flux Φ from Φ = σT^4: | 3.402×10^6 W/m^2 (watts per square meter)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface:  | 4.923×10^7 lx (lux)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 4.923×10^7 lx (lux)