The Cooling of Mars



This is an image of Mars.
Click on image for full size version (40K GIF)
Image from: NASA

Many of the reasons the history of Mars is different from that of the Earth stem from the small size of Mars. Mars is about 1/3 the size of the Earth. This means that it was able to cool much more rapidly over time than did the Earth.

When Mars formed about 4 Billion Years ago, it may have been left relatively colder than the other terrestrial planets. Further cooling inward from the surface of Mars froze the water, preventing the formation of special hydrated-minerals which allow for movement of the lithosphere. Without the ability to subduct and remelt, the Martian lithosphere slowly thickened to the point of being immovable, like hardening candy.

Later there was a period of warming and volcanism, caused by a warm plume of material rising from the deep interior of Mars, which pushed out and raised the crust, and created the Tharsis Bulge, Olympus Mons, and the other volcanoes. This volcanism influenced the subsequent Martian climate.


What is the cooling history of the Earth?


The Cooling of Mars



This is an image of Mars.
Click on image for full size version (40K GIF)
Image from: NASA

Mars is small. Mars is about 1/3 the size of the Earth. This means that it cooled off very fast.

Mars probably started colder than the other earth-like planets. Then, Mars cooled rapidly from the outside, inward, like hardening candy. This caused the surface crust of Mars to rapidly thicken to the point of being immovable and prevented any further continental drift.

Much later, Mars finally warmed a little from inside. (Earth and Venus were already warm from inside!) Then a bubble of material rose from the deep interior of Mars, like the bubble in a tire, which pushed out and raised the crust, and created the Tharsis Bulge, Olympus Mons, and the other volcanoes.


What is the cooling history of the Earth?


The Cooling of Mars



This is an image of Mars.
Click on image for full size version (40K GIF)
Image from: NASA

Mars is small. Mars is about 1/3 the size of the Earth. This means that it cooled off very fast.

Mars probably started colder than the other earth-like planets. Then, Mars cooled rapidly from the outside, inward, like hardening candy. This caused the surface crust of Mars to rapidly thicken to the point of being immovable and prevented any further continental drift.

Much later, Mars finally warmed a little from inside. (Earth and Venus were already warm from inside!) Then a bubble of material rose from the deep interior of Mars, like the bubble in a tire, which pushed out and elevated the crust, and created the Tharsis Bulge, Olympus Mons, and the other volcanoes.


What is the cooling history of the Earth?



Last modified April 2, 1997 by the Windows Team

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