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Basic Facts About The Planet Mars...


 
 


Mars is the fourth planet from the Sun and has some of the most breathtaking scenery in the solar system. There are canyons three times as deep and five times as long as the Grand Canyon, enormous volcanoes over twice as tall as Mount Everest, polar ice caps, huge fields of sand dunes, butterscotch-colored daytime skies, clouds, and thousands of kilometers of valleys reminiscent of dry river beds on Earth.

 
 
Composition of the atmosphere (by volume) 
95.3% carbon dioxide 
2.7%   nitrogen 
1.6%   argon 
0.13% oxygen 
remainder: traces of water vapor, neon, krypton, xenon
Average air pressure at the surface 6 millibars 
(compared to 1013 millibars on Earth)
Average diameter
of Mars
6 779 km (about half that of the Earth)*
Average distance from the Sun: 227 940 000 km (or 1.52 Astronomical Units, i.e. 1.52 times as far as Earth)
Martian sidereal day 
(i.e., rotation time): 
24 hours, 37 minutes and 22 seconds
Martian solar day 
(i.e., time between two successive noons)
24 hours, 39 minutes and 35 seconds
Martian year 
(i.e., time to orbit the Sun):
669.6 Martian solar days or 687 Earth days (i.e., about 1.9 Earth years)
Global average temperature:  218 K (-55 °C)
Minimum surface temperature: 140 K (-133 °C) (temperature of frozen carbon dioxide on high elevations at the winter pole)
Maximum surface temperature: 300 K (27 °C) (dark tropical regions in summer)
Surface area: about the same as the land area on Earth
Highest mountain: Olympus Mons - the largest mountain in the Solar System rising 24 km above the surrounding plain (21.2 km above the reference level**). Its base is more than 500 km in diameter and is rimmed by a cliff 6 km high
Largest canyon: Valles Marineris - a canyon 4 000 km long, up to 5.3 km deep**, and up to 20 km wide. 
Largest impact crater and deepest point on Mars: Hellas Planitia - an impact crater in the southern hemisphere up to 7.8 km deep** and 2 000 km in diameter 
 
Surface bulge: Tharsis - a huge bulge on the Martian surface that is about 4 000 km across and 10 km high 
 
 
   
* Geodetic data is taken from the results of the MOLA (Mars Orbiter Laser Altimeter) instrument on the NASA's Mars Global Surveyor spacecraft and differs from older data that you may see.

** In this table, zero elevation is defined as the gravitational equipotential surface whose average value at the equator is equal to the average radius as determined by the MOLA (Mars Orbiter Laser Altimeter) instrument on the NASA's Mars Global Surveyor spacecraft. See the MOLA geodetic data page for more details.

Key Reference:
H.H. Kieffer, B. M. Jakosky, C. W. Snyder and M. S. Matthews (Editors), Mars, University of Arizona Press, Tucson, Arizona, 1992.

   
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Responsible NASA Official: Robert Haberle
Last Updated: 08/29/04
Designed by: James Schilling