Input interpretation
![boron nitride | freezing point](../image_source/fd241843dabaf93d6ee503767a9e664a.png)
boron nitride | freezing point
Result
![2527 °C (degrees Celsius)](../image_source/7f0da092fdde1c411eb73d204a03bb32.png)
2527 °C (degrees Celsius)
Unit conversions
![2800 K (kelvins)](../image_source/5f70c6baafa0cc835d456226994d9a8a.png)
2800 K (kelvins)
![4581 °F (degrees Fahrenheit)](../image_source/74a1b81d12816cfbf9eedbf3819081e4.png)
4581 °F (degrees Fahrenheit)
![5040 °R (degrees Rankine)](../image_source/a3420d73a6c0985f7cc085c2cce032af.png)
5040 °R (degrees Rankine)
![2022 °Ré (degrees Réaumur)](../image_source/154a07a2064664e7fddb7ad8d0382d24.png)
2022 °Ré (degrees Réaumur)
![1334 °Rø (degrees Rømer)](../image_source/942667752dc2fa2fcef205c23b32478a.png)
1334 °Rø (degrees Rømer)
Blackbody information
![perceived color | peak wavelength | 1.035 µm (micrometers) peak frequency | 164.6 THz (terahertz)](../image_source/c061df7dabe258a6efdcbd9b6e080f4b.png)
perceived color | peak wavelength | 1.035 µm (micrometers) peak frequency | 164.6 THz (terahertz)
Corresponding main-sequence star properties
![temperature class | M6 absolute magnitude | +12 (bolometric) mass | 0.11 M_☉ radius | 0.13 R_☉ luminosity | 9×10^-4 L_☉ B-V color index | 2.0 lifetime | 2.7 trillion yr end state | helium white dwarf](../image_source/bb20be4a7923b4ad1b7cedd643f23f53.png)
temperature class | M6 absolute magnitude | +12 (bolometric) mass | 0.11 M_☉ radius | 0.13 R_☉ luminosity | 9×10^-4 L_☉ B-V color index | 2.0 lifetime | 2.7 trillion yr end state | helium white dwarf
Examples of M6 main-sequence stars
![V1365 Orionis | Gl 860 B](../image_source/3d2d061b9e3394eccff31d7ced5d904e.png)
V1365 Orionis | Gl 860 B
Corresponding quantities
![Thermodynamic energy E from E = kT: | 24 ceV (centielectronvolts)](../image_source/3901cbea6d4f8eb3cf55b6cbaebd6529.png)
Thermodynamic energy E from E = kT: | 24 ceV (centielectronvolts)
![Blackbody energy flux Φ from Φ = σT^4: | 3.486×10^6 W/m^2 (watts per square meter)](../image_source/0fa855f891f65308578c95e64d32f892.png)
Blackbody energy flux Φ from Φ = σT^4: | 3.486×10^6 W/m^2 (watts per square meter)
![Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 5.201×10^7 lx (lux)](../image_source/5d7e02cda1d8c0cb48655c872c56f125.png)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 5.201×10^7 lx (lux)