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Climate of Mars. Mars' cloudy sky as seen by Perseverance rover in 2023, sol 738. The climate of Mars has been a topic of scientific curiosity for centuries, in part because it is the only terrestrial planet whose surface can be easily directly observed in detail from the Earth with help from a telescope. Although Mars is smaller than the Earth ...
[3] [5] [2] The atmosphere of Mars is much thinner and colder than Earth's having a max density 20g/m 3 (about 2% of Earth’s value) with a temperature generally below zero down to -60 Celsius. The average surface pressure is about 610 pascals (0.088 psi) which is 0.6% of the Earth's value.
Mars is the fourth planet from the Sun. ... During a year, there are large surface temperature swings on the surface between −78.5 °C (−109.3 °F) ...
The median Martian surface temperature is about minus-85 degrees Fahrenheit (minus-65 degrees Celsius). With its tenuous atmosphere, solar heat on the Martian surface readily escapes into space.
There are large variations in surface temperature over space and time on airless or near-airless bodies like Mars, which has daily surface temperature variations of 50–60 K. [18] [19] Because of a relative lack of air to transport or retain heat, significant variations in temperature develop. Assuming the planet radiates as a blackbody (i.e ...
192 K, Debye temperature of ice. 273.15 K (0 °C), melting point of bound water. 273.16 K (0.01 °C), temperature of triple point of water. c. 293 K, room temperature. 373.15 K (100 °C), boiling point of bound water at sea level. 647 K, critical point of superheated water. 737.5 K, mean on Venus.
[9] [26] There can be large temperature swings on Mars, for example at the equator it may reach 70 degrees F (20 degrees C) in the daytime but then go down to minus 100 degrees F (−73 C) at night. [27] Examples of Mars surface temperatures: [27] Average −80 degrees Fahrenheit (−60 degrees Celsius).
1995 photo of Mars showing approximate size of the polar caps. The planet Mars has two permanent polar ice caps of water ice and some dry ice (frozen carbon dioxide, CO 2).Above kilometer thick layers of water ice permafrost slabs of dry ice are deposited during a pole's winter, [1] [2] lying in continuous darkness, causing 25–30% of the atmosphere being deposited annually at either of the ...