different temperature is agent of what what are the difference between them
Answers
Surface temperatures, pressures, and atmospheric gas compositions bolster the feasibility of gas hydrate formation on Mars. Carbon dioxide, the dominant atmospheric gas, is a hydrate former. Selective areas of the planet have pressure/temperature combinations near the surface, or directly below, conducive to hydrate formation.
The global mean temperature at the surface of Mars is 200 K (Duxbury et al., 2004; Max and Clifford, 2000; Fairen et al., 2009; Krasnopolsky et al., 2004). However, local Martian surface temperatures vary widely. These temperatures range from 148 to 276 K, depending on locations, seasons, and altitudes.
Representative Martian surface temperatures are presented in Table 10.4, where the large variations are observed because the listing covers seasonal changes, various altitudes, equatorial regions, and polar regions. Temperatures may also be affected by suspended dust (Leovy, 2001).