What are some extremely high temperatures?
On the ground we are lucky to have experienced temperatures near the lower end of what is possible. Temperatures on the ground range from 184 hp (-89 ° C, -128.6 ° F) to 331 K (58 ° C, 136.4 ° F), with an average surface temperature of 287 h (14 ° C, 57 ° F). 287 K is compared to the solar surface temperature, which is 5780 h.
1170 K is the approximate temperature of the wood burning in the fire. Iron is melted at 1811 K. The temperature of the molten core of the ground is about 5650 K. At 7000 K, the most famous elements and compounds such as carbon, evaporates. Generally, at temperatures deep below 9000 k, gases become plasma, which is ionized gas, which means that electrons are torn from atomic cores and float freely in the mixture. Wolfram does not evaporate up to 15500 hp.
Permanent temperatures greater than about a few kk (kilocevin or 1000 hp) are found mainly in the cores of gas giants and in the interiors of stars and other exotic astronomical objects. The Jupiter core is estimated at 20-30 kk. The hottest flash when it was measured at zEmi, was 28 kk. The temperature on the surface of Sirius, the brightest star in the night sky, is about 33 kk.
temperatures above 100 kk are generated by atomic bombs, particle accelerators, experimental fusion reactors and stars. The temperature of about 17 meters from the detonation point of Little Boy, one of the first atomic bombs, would be about 300 kk. Local excitations caused by X -rays are temperature in this range. The corona of the Sun, which is significantly warmer than its surface, has a temperature in the range of 1-10 mk (megakelvin or a million Kelvins). The core of the sun is 13.6 mk and the temperature for the controlled nuclear fusion is 100 MK. The sun successfully connects the atomic cores due to its extremely high pressure along with the heat. Local excitation Caused by Gama rays are in this thermal range.
temperatures above 1 gk (Gigakelvin or billions of Kelvin) are reserved for special phenomena in space such as matter and antimater reactions, supernova, fusion of galactic clusters and (for extremely small fractions of seconds) in particle accelerators. The supernova explosion has temperatures of approximately 10 gk. In this intense heat, heavy elements such as uranium are formed.
The highest temperature ever existed is probably 10