Input interpretation
![uranium carbide (1:1) | freezing point](../image_source/a03b2f76d3062b8cfcf5ab21039f0363.png)
uranium carbide (1:1) | freezing point
Result
![2790 °C (degrees Celsius)](../image_source/64010b871fae7829d7939a5a2c6386bc.png)
2790 °C (degrees Celsius)
Unit conversions
![3063 K (kelvins)](../image_source/8903e87433f9f649cd9963bbb2b9b92c.png)
3063 K (kelvins)
![5054 °F (degrees Fahrenheit)](../image_source/760cbc9009703c733c62370d0f772eae.png)
5054 °F (degrees Fahrenheit)
![5514 °R (degrees Rankine)](../image_source/f0e4490f6c90e26bfd3cddf7223e39b2.png)
5514 °R (degrees Rankine)
![2232 °Ré (degrees Réaumur)](../image_source/6287c2231b6d7d65114b206dff3a0e20.png)
2232 °Ré (degrees Réaumur)
![1472 °Rø (degrees Rømer)](../image_source/9f176dd1f46910b3bcd082a775c1c6dc.png)
1472 °Rø (degrees Rømer)
Blackbody information
![perceived color | peak wavelength | 946 nm (nanometers) peak frequency | 180.1 THz (terahertz)](../image_source/c784cf4dd88c8bf5e751dbc7cc2667c1.png)
perceived color | peak wavelength | 946 nm (nanometers) peak frequency | 180.1 THz (terahertz)
Corresponding main-sequence star properties
![temperature class | M4.5 absolute magnitude | +11 (bolometric) mass | 0.16 M_☉ radius | 0.22 R_☉ luminosity | 0.0039 L_☉ B-V color index | 1.8 lifetime | 920 billion yr end state | helium white dwarf](../image_source/28e3ff1901ca49470eacec72a7a933b6.png)
temperature class | M4.5 absolute magnitude | +11 (bolometric) mass | 0.16 M_☉ radius | 0.22 R_☉ luminosity | 0.0039 L_☉ B-V color index | 1.8 lifetime | 920 billion yr end state | helium white dwarf
Examples of M4.5 main-sequence stars
![Ross 128 | Gl 83.1 | GJ 1151](../image_source/31d1cd02f2ed9c7ae3f6a6e7d763fdfb.png)
Ross 128 | Gl 83.1 | GJ 1151
Corresponding quantities
![Thermodynamic energy E from E = kT: | 26 ceV (centielectronvolts)](../image_source/3c480f0b3118178af27adde138445acc.png)
Thermodynamic energy E from E = kT: | 26 ceV (centielectronvolts)
![Blackbody energy flux Φ from Φ = σT^4: | 4.992×10^6 W/m^2 (watts per square meter)](../image_source/3f651545b0332ee111ea02373e94d90d.png)
Blackbody energy flux Φ from Φ = σT^4: | 4.992×10^6 W/m^2 (watts per square meter)
![Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 1.13×10^8 lx (lux)](../image_source/30f24614e9c4c711fafd5417c4f68390.png)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 1.13×10^8 lx (lux)