Input interpretation
![zirconium(IV) oxide | freezing point](../image_source/adffb094ed3f70d9472dfe2fbd28f4f6.png)
zirconium(IV) oxide | freezing point
Result
![2700 °C (degrees Celsius)](../image_source/1494057b323eac48ecca9636af236bd4.png)
2700 °C (degrees Celsius)
Unit conversions
![2973 K (kelvins)](../image_source/686ebb69ea688361411d66ae92add694.png)
2973 K (kelvins)
![4892 °F (degrees Fahrenheit)](../image_source/b72b3d9f68003be33fdb047f9ea84c4a.png)
4892 °F (degrees Fahrenheit)
![5352 °R (degrees Rankine)](../image_source/7b9d9b986bc57d160f85512535a61db6.png)
5352 °R (degrees Rankine)
![2160 °Ré (degrees Réaumur)](../image_source/ae478eca82b23fcd204c3eee92c417e7.png)
2160 °Ré (degrees Réaumur)
![1425 °Rø (degrees Rømer)](../image_source/7af2728d7b754a3f36b8bbedc311c0a6.png)
1425 °Rø (degrees Rømer)
Blackbody information
![perceived color | peak wavelength | 0.9746 µm (micrometers) peak frequency | 174.8 THz (terahertz)](../image_source/b4d6c10d53f0eb86d648e8c948e95578.png)
perceived color | peak wavelength | 0.9746 µm (micrometers) peak frequency | 174.8 THz (terahertz)
Corresponding main-sequence star properties
![temperature class | M5.5 absolute magnitude | +12 (bolometric) mass | 0.12 M_☉ radius | 0.15 R_☉ luminosity | 0.0015 L_☉ B-V color index | 1.9 lifetime | 2.1 trillion yr end state | helium white dwarf](../image_source/499652ad096c0fbe60a2bfdce9eda61b.png)
temperature class | M5.5 absolute magnitude | +12 (bolometric) mass | 0.12 M_☉ radius | 0.15 R_☉ luminosity | 0.0015 L_☉ B-V color index | 1.9 lifetime | 2.1 trillion yr end state | helium white dwarf
Examples of M5.5 main-sequence stars
![GJ 3700 | GJ 1061](../image_source/f9700bbea8acdf2df898acee752a0ae4.png)
GJ 3700 | GJ 1061
Corresponding quantities
![Thermodynamic energy E from E = kT: | 26 ceV (centielectronvolts)](../image_source/ecc13aa8268bf7e0c3201676bb9edac1.png)
Thermodynamic energy E from E = kT: | 26 ceV (centielectronvolts)
![Blackbody energy flux Φ from Φ = σT^4: | 4.431×10^6 W/m^2 (watts per square meter)](../image_source/b06b1659ace94f98f6df39805ee5ecd3.png)
Blackbody energy flux Φ from Φ = σT^4: | 4.431×10^6 W/m^2 (watts per square meter)
![Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 8.797×10^7 lx (lux)](../image_source/c7a7a975f5653885c049283b355a9bbf.png)
Approximate luminous exitance from a planar blackbody radiator perpendicular to its surface: | 8.797×10^7 lx (lux)