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freezing point of erbium oxide

Input interpretation

erbium oxide | freezing point
erbium oxide | freezing point

Result

2420 °C (degrees Celsius)
2420 °C (degrees Celsius)

Unit conversions

2693 K (kelvins)
2693 K (kelvins)
4388 °F (degrees Fahrenheit)
4388 °F (degrees Fahrenheit)
4848 °R (degrees Rankine)
4848 °R (degrees Rankine)
1936 °Ré (degrees Réaumur)
1936 °Ré (degrees Réaumur)
1278 °Rø (degrees Rømer)
1278 °Rø (degrees Rømer)

Blackbody information

  perceived color |  peak wavelength | 1.076 µm (micrometers) peak frequency | 158.3 THz (terahertz)
perceived color | peak wavelength | 1.076 µm (micrometers) peak frequency | 158.3 THz (terahertz)

Corresponding main-sequence star properties

temperature class | M6.5 absolute magnitude | +13 (bolometric) mass | 0.097 M_☉ radius | 0.13 R_☉ luminosity | 7.6×10^-4 L_☉ B-V color index | 2.1 lifetime | 3.4 trillion yr end state | helium white dwarf
temperature class | M6.5 absolute magnitude | +13 (bolometric) mass | 0.097 M_☉ radius | 0.13 R_☉ luminosity | 7.6×10^-4 L_☉ B-V color index | 2.1 lifetime | 3.4 trillion yr end state | helium white dwarf

Examples of M6.5 main-sequence stars

DX Cancri
DX Cancri

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:  | 2.983×10^6 W/m^2 (watts per square meter)
Blackbody energy flux Φ from Φ = σT^4: | 2.983×10^6 W/m^2 (watts per square meter)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface:  | 3.636×10^7 lx (lux)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 3.636×10^7 lx (lux)