Input interpretation
![holmium(III) oxide | freezing point](../image_source/452c003c97e0732db6b0f73e54fa79c6.png)
holmium(III) oxide | freezing point
Result
![2330 °C (degrees Celsius)](../image_source/03eeb9360c04ca88aef1d420693aa114.png)
2330 °C (degrees Celsius)
Unit conversions
![2603 K (kelvins)](../image_source/f323636c293a7849af27a435436b03d8.png)
2603 K (kelvins)
![4226 °F (degrees Fahrenheit)](../image_source/613bd4f180fca726f282948ad68168b8.png)
4226 °F (degrees Fahrenheit)
![4686 °R (degrees Rankine)](../image_source/9373236ca5166d52ebfae963a74eee7f.png)
4686 °R (degrees Rankine)
![1864 °Ré (degrees Réaumur)](../image_source/930aa77faccb267d31815e07fe7ba46e.png)
1864 °Ré (degrees Réaumur)
![1231 °Rø (degrees Rømer)](../image_source/62c0f076bc33e91505ebb73914d165d0.png)
1231 °Rø (degrees Rømer)
Blackbody information
![perceived color | peak wavelength | 1.113 µm (micrometers) peak frequency | 153 THz (terahertz)](../image_source/df8b11ac601e85622a8d88f122300869.png)
perceived color | peak wavelength | 1.113 µm (micrometers) peak frequency | 153 THz (terahertz)
Corresponding main-sequence star properties
![temperature class | M7 absolute magnitude | +13 (bolometric) mass | 0.081 M_☉ radius | 0.11 R_☉ luminosity | 5.2×10^-4 L_☉ B-V color index | 2.2 lifetime | 5.4 trillion yr](../image_source/4926ff49e0366fe7963579cc5f049ca5.png)
temperature class | M7 absolute magnitude | +13 (bolometric) mass | 0.081 M_☉ radius | 0.11 R_☉ luminosity | 5.2×10^-4 L_☉ B-V color index | 2.2 lifetime | 5.4 trillion yr
Units
Corresponding quantities
![Thermodynamic energy E from E = kT: | 22 ceV (centielectronvolts)](../image_source/18e370465e3d8e0787141e667ef28c2d.png)
Thermodynamic energy E from E = kT: | 22 ceV (centielectronvolts)
![Blackbody energy flux Φ from Φ = σT^4: | 2.604×10^6 W/m^2 (watts per square meter)](../image_source/16a5346f3257d818445f84d6231debdc.png)
Blackbody energy flux Φ from Φ = σT^4: | 2.604×10^6 W/m^2 (watts per square meter)
![Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 2.632×10^7 lx (lux)](../image_source/67ec16befa2404f35340de91211d65e4.png)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 2.632×10^7 lx (lux)