Input interpretation
![thorium nitride | freezing point](../image_source/a9bfc86d2bb54a285af57451094a8bc7.png)
thorium nitride | freezing point
Result
![2820 °C (degrees Celsius)](../image_source/8e9ae647e3e3d31652445ff5a50f1855.png)
2820 °C (degrees Celsius)
Unit conversions
![3093 K (kelvins)](../image_source/236a2acc9d385072409319eaee98610c.png)
3093 K (kelvins)
![5108 °F (degrees Fahrenheit)](../image_source/829a636b61baab7dc624e26a2969836c.png)
5108 °F (degrees Fahrenheit)
![5568 °R (degrees Rankine)](../image_source/9c597d051e69b4a9ea8bda08cd110321.png)
5568 °R (degrees Rankine)
![2256 °Ré (degrees Réaumur)](../image_source/e35065b44a2e92709aa6766609b2caae.png)
2256 °Ré (degrees Réaumur)
![1488 °Rø (degrees Rømer)](../image_source/6c145b865812813959db1330ef2bb6c9.png)
1488 °Rø (degrees Rømer)
Blackbody information
![perceived color | peak wavelength | 936.8 nm (nanometers) peak frequency | 181.8 THz (terahertz)](../image_source/28caaba5f7c4cf0b4e13dcf1978ba2e3.png)
perceived color | peak wavelength | 936.8 nm (nanometers) peak frequency | 181.8 THz (terahertz)
Corresponding main-sequence star properties
![temperature class | M4.5 absolute magnitude | +11 (bolometric) mass | 0.18 M_☉ radius | 0.24 R_☉ luminosity | 0.0047 L_☉ B-V color index | 1.7 lifetime | 760 billion yr end state | helium white dwarf](../image_source/a713830025f4e1d7744dfe5b3dffc353.png)
temperature class | M4.5 absolute magnitude | +11 (bolometric) mass | 0.18 M_☉ radius | 0.24 R_☉ luminosity | 0.0047 L_☉ B-V color index | 1.7 lifetime | 760 billion yr end state | helium white dwarf
Examples of M4.5 main-sequence stars
![Ross 128 | Gl 83.1 | GJ 1151](../image_source/f8a367f2468c247aea1c8204bf201fce.png)
Ross 128 | Gl 83.1 | GJ 1151
Corresponding quantities
![Thermodynamic energy E from E = kT: | 27 ceV (centielectronvolts)](../image_source/301839fd02ade0f16e8d48bf3b4db89b.png)
Thermodynamic energy E from E = kT: | 27 ceV (centielectronvolts)
![Blackbody energy flux Φ from Φ = σT^4: | 5.191×10^6 W/m^2 (watts per square meter)](../image_source/78c1bf726ceb2cd1062870a35c354aed.png)
Blackbody energy flux Φ from Φ = σT^4: | 5.191×10^6 W/m^2 (watts per square meter)
![Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 1.225×10^8 lx (lux)](../image_source/e730c94c9f3c8bbaf249a68abaa89a69.png)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 1.225×10^8 lx (lux)