PIA16477: Pressure Cycles on Mars
Target Name: Mars
Is a satellite of: Sol (our sun)
Mission: Mars Science Laboratory (MSL)
Spacecraft: Curiosity
Instrument: REMS
Product Size: 2999 x 2249 pixels (width x height)
Produced By: JPL
Full-Res TIFF: PIA16477.tif (20.24 MB)
Full-Res JPEG: PIA16477.jpg (262.7 kB)


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This graph shows the atmospheric pressure at the surface of Mars, as measured by the Rover Environmental Monitoring Station on NASA's Curiosity rover. The blue curve shows data from Sol 31 (Sept. 6, 2012) and the green curve shows data from Sol 93 (Nov. 7, 2012). Pressure is a measure of the amount of air in the whole column of atmosphere sitting above the rover.

The overall increase in pressure between Sol 31 and Sol 93 is the signature of the entire Martian atmosphere growing in mass as we move into springtime in the southern hemisphere. This happens because the south pole receives more and more sunlight, and carbon dioxide vaporizes off of the winter south polar cap. Each year the atmosphere grows and shrinks by about 30 percent due to this effect. The curves also show a strong daily variation in pressure of around 10 percent, with a peak near 7 a.m. on Mars and a minimum near 4 p.m. This daily cycle in pressure is caused by a "thermal tide," a global-scale pressure wave in Mars' atmosphere driven by sunlight heating the ground and air.



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