Input interpretation
![graphite | freezing point](../image_source/98471d2c739fee0e1cba53278446e9d2.png)
graphite | freezing point
Result
![3675 °C (degrees Celsius)](../image_source/50d59509b120ff1bd93863dcb4731911.png)
3675 °C (degrees Celsius)
Unit conversions
![3948 K (kelvins)](../image_source/e82d3ca401af9e0559d2108c8c551ff4.png)
3948 K (kelvins)
![6646 °F (degrees Fahrenheit)](../image_source/b0f9d4e581cdd57f91b769bf7e7aafe3.png)
6646 °F (degrees Fahrenheit)
![7106 °R (degrees Rankine)](../image_source/3bb425803a27991e2c2415de59c71e07.png)
7106 °R (degrees Rankine)
![2940 °Ré (degrees Réaumur)](../image_source/04e4d9a9c1bf0a606ce79a5ba301a716.png)
2940 °Ré (degrees Réaumur)
![1937 °Rø (degrees Rømer)](../image_source/02dc1a76f86a324821f831162d933215.png)
1937 °Rø (degrees Rømer)
Blackbody information
![perceived color | peak wavelength | 734 nm (nanometers) peak frequency | 232.1 THz (terahertz)](../image_source/a174d6d94dfa8d77c70459df432d51ef.png)
perceived color | peak wavelength | 734 nm (nanometers) peak frequency | 232.1 THz (terahertz)
Corresponding main-sequence star properties
![temperature class | K8 absolute magnitude | +7.6 (bolometric) mass | 0.61 M_☉ radius | 0.56 R_☉ luminosity | 0.068 L_☉ B-V color index | 1.4 lifetime | 34 billion yr end state | carbon-oxygen white dwarf](../image_source/e07f540fdfac7dcc89626e1e997f43dd.png)
temperature class | K8 absolute magnitude | +7.6 (bolometric) mass | 0.61 M_☉ radius | 0.56 R_☉ luminosity | 0.068 L_☉ B-V color index | 1.4 lifetime | 34 billion yr end state | carbon-oxygen white dwarf
Examples of K8 main-sequence stars
![Groombridge 1618 | HIP 98746 | HIP 54646 | HIP 21553 | Gl 795 B](../image_source/b9a5a1ae74a4b6bbe9685896e37785ad.png)
Groombridge 1618 | HIP 98746 | HIP 54646 | HIP 21553 | Gl 795 B
Corresponding quantities
![Thermodynamic energy E from E = kT: | 34 ceV (centielectronvolts)](../image_source/c4dc17b9b096e82ae2e6e0e033e39736.png)
Thermodynamic energy E from E = kT: | 34 ceV (centielectronvolts)
![Blackbody energy flux Φ from Φ = σT^4: | 1.377×10^7 W/m^2 (watts per square meter)](../image_source/9a6b5b15447bd95423fddc48a0e01d1b.png)
Blackbody energy flux Φ from Φ = σT^4: | 1.377×10^7 W/m^2 (watts per square meter)
![Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 7.295×10^8 lx (lux)](../image_source/fdacb02dbe53e72632ec9d4f20ec0e45.png)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 7.295×10^8 lx (lux)