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Mars

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Seven times smaller than Earth and 10 times less massive, Mars is a comparatively small planet. Encircled by 2 small satellites, Phobos and Deimos, it is a solid sphere with a desert landscape tinged red by iron oxide.

With a gravitational force just one-third of that on Earth, Mars has only been able to retain a very thin, tenuous atmosphere consisting of 95% carbon dioxide. Atmospheric pressure is highly variable and 170 times weaker than on Earth.
With little heat from the Sun and no significant greenhouse effect, temperatures at the equator vary between –100°C and 0°C.

Most of the changes to Mars’ surface are caused by the winds that sweep across its dry landscape, raising clouds of ochre dust and turning the atmosphere a reddish brown. Violent storms periodically hurl these dust clouds 50 kilometres into the air, totally blocking out the sky.
Mars’ southern ice cap, seen by the Mars Global Surveyor probe. Taken in summer, this photograph shows the ice cap at its narrowest, spanning 430 kilometres.

Mars’ southern ice cap, seen by the Mars Global Surveyor probe. Taken in summer, this photograph shows the ice cap at its narrowest, spanning 430 kilometres.

At the poles, permanent ice caps of frozen water and carbon dioxide (dry ice) advance and recede with the changing seasons, while the rest of the planet is strewn with rocks and dust. Covered with countless meteor craters in its southern hemisphere and with volcanic plains in its northern hemisphere, the surface of Mars has been gouged out by giant canyons that extend from west to east. Its internal structure resembles that of other terrestrial planets, comprising a crust, mantle and core.



 

This gigantic scar on the surface of the red planet is a vast canyon system called the Valles Marineris. Some 50 to 100 kilometres wide and 4,000 kilometres long, it was probably created by a massive landslide following an earthquake.

Space photographs have also revealed the existence of winding valleys like dried-out riverbeds, showing that some liquid—perhaps water—once flowed here. This means that Mars was once warmer and wetter than it is today.

Mars
Etymology: Mars was named after the Greek and Roman gods of war, due to its blood-red colour.

Discovered: Before records began.

Distinctive feature: Mars’ history and current characteristics suggest the possibility—now or in the past—of some form of life.

Typical one-way journey time using current technologies: 6 to 11 months.


 

Last updated: May 2003

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