Input interpretation
![cerium(III) sulfide | freezing point](../image_source/640131b660df93c9a3f85ed30feb7a24.png)
cerium(III) sulfide | freezing point
Result
![2450 °C (degrees Celsius)](../image_source/37d12489931dd958c8eca9c7c3025edf.png)
2450 °C (degrees Celsius)
Unit conversions
![2723 K (kelvins)](../image_source/4dd2290a4a3ae5c38012ffd4693e3ed6.png)
2723 K (kelvins)
![4442 °F (degrees Fahrenheit)](../image_source/892434682b0b3d34231291b43ff63c5c.png)
4442 °F (degrees Fahrenheit)
![4902 °R (degrees Rankine)](../image_source/bfd78c73619ad74d9ba2ad0f30a3de0d.png)
4902 °R (degrees Rankine)
![1960 °Ré (degrees Réaumur)](../image_source/3ead3dc9771e2631b7044581e41c3e1f.png)
1960 °Ré (degrees Réaumur)
![1294 °Rø (degrees Rømer)](../image_source/7e51a6d5559839bc926810038bf4d584.png)
1294 °Rø (degrees Rømer)
Blackbody information
![perceived color | peak wavelength | 1.064 µm (micrometers) peak frequency | 160.1 THz (terahertz)](../image_source/eff7c1e98bd3358ecbaa4224c3d2865f.png)
perceived color | peak wavelength | 1.064 µm (micrometers) peak frequency | 160.1 THz (terahertz)
Corresponding main-sequence star properties
![temperature class | M6 absolute magnitude | +12 (bolometric) mass | 0.1 M_☉ radius | 0.13 R_☉ luminosity | 8.3×10^-4 L_☉ B-V color index | 2.1 lifetime | 3.1 trillion yr end state | helium white dwarf](../image_source/aeb1f0321d70fb7173cde5519a450c18.png)
temperature class | M6 absolute magnitude | +12 (bolometric) mass | 0.1 M_☉ radius | 0.13 R_☉ luminosity | 8.3×10^-4 L_☉ B-V color index | 2.1 lifetime | 3.1 trillion yr end state | helium white dwarf
Examples of M6 main-sequence stars
![V1365 Orionis | Gl 860 B](../image_source/cc5514b036876463fd6058fb1cd8cfa2.png)
V1365 Orionis | Gl 860 B
Corresponding quantities
![Thermodynamic energy E from E = kT: | 23 ceV (centielectronvolts)](../image_source/62542a42b278126cc0e2d3749411f8b0.png)
Thermodynamic energy E from E = kT: | 23 ceV (centielectronvolts)
![Blackbody energy flux Φ from Φ = σT^4: | 3.118×10^6 W/m^2 (watts per square meter)](../image_source/29265ca0c7769009367b1226223f4814.png)
Blackbody energy flux Φ from Φ = σT^4: | 3.118×10^6 W/m^2 (watts per square meter)
![Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 4.031×10^7 lx (lux)](../image_source/0dbc77c979cbb236a625e4969b28bef3.png)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 4.031×10^7 lx (lux)