Input interpretation
![lime | freezing point](../image_source/41314dcc9e0735323e162a30f3aa6823.png)
lime | freezing point
Result
![2580 °C (degrees Celsius)](../image_source/75066b621ab37b2243ef85effc651307.png)
2580 °C (degrees Celsius)
Unit conversions
![2853 K (kelvins)](../image_source/b706df888eb6bf530f0bff92cfcb1502.png)
2853 K (kelvins)
![4676 °F (degrees Fahrenheit)](../image_source/dff4c349580e07e763ccb8843d6f1fe6.png)
4676 °F (degrees Fahrenheit)
![5136 °R (degrees Rankine)](../image_source/cd8d9f401cc2002221a50141975b97df.png)
5136 °R (degrees Rankine)
![2064 °Ré (degrees Réaumur)](../image_source/8809efee7741a6e76c64284794bb7ace.png)
2064 °Ré (degrees Réaumur)
![1362 °Rø (degrees Rømer)](../image_source/28123d848844b2d71c3f6985c92f174e.png)
1362 °Rø (degrees Rømer)
Blackbody information
![perceived color | peak wavelength | 1.016 µm (micrometers) peak frequency | 167.7 THz (terahertz)](../image_source/25b65ffb4b8a3b8d3ff45b35aa2f8238.png)
perceived color | peak wavelength | 1.016 µm (micrometers) peak frequency | 167.7 THz (terahertz)
Corresponding main-sequence star properties
![temperature class | M5.5 absolute magnitude | +12 (bolometric) mass | 0.11 M_☉ radius | 0.13 R_☉ luminosity | 9.7×10^-4 L_☉ B-V color index | 2.0 lifetime | 2.5 trillion yr end state | helium white dwarf](../image_source/e908c49544ab398736c8048203a07fe1.png)
temperature class | M5.5 absolute magnitude | +12 (bolometric) mass | 0.11 M_☉ radius | 0.13 R_☉ luminosity | 9.7×10^-4 L_☉ B-V color index | 2.0 lifetime | 2.5 trillion yr end state | helium white dwarf
Examples of M5.5 main-sequence stars
![GJ 3700 | GJ 1061](../image_source/4e61d91d2d497ede79832ff1b18d5535.png)
GJ 3700 | GJ 1061
Corresponding quantities
![Thermodynamic energy E from E = kT: | 25 ceV (centielectronvolts)](../image_source/c7e4b2a93c3f54e1f5db995aabf5331b.png)
Thermodynamic energy E from E = kT: | 25 ceV (centielectronvolts)
![Blackbody energy flux Φ from Φ = σT^4: | 3.758×10^6 W/m^2 (watts per square meter)](../image_source/0ddf692d347942ee52d29b826e413481.png)
Blackbody energy flux Φ from Φ = σT^4: | 3.758×10^6 W/m^2 (watts per square meter)
![Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 6.151×10^7 lx (lux)](../image_source/958031e0ffcd3e724df4bbe96a96a274.png)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 6.151×10^7 lx (lux)