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 The Planet Mars - Facts, Information, & Pictures


Mars is the fourth planet from the Sun and is known as the Red Planet due to the color of it's surface.  Mars is thought to have once had  an Earth-like atmosphere and surface, complete with lakes, rivers, and oceans, and as many speculate, life.  There is ample evidence on the surface of Mars that water once freely flowed throughout the planet.  Even today, we find Mars' polar ice caps that grow and shrink with the Martian seasons.  There is also an underground store of frozen water that has been found that holds enough water to fill Lake Michigan two times. 

Like Earth, Mars has tectonic activity, albeit a much different type of activity.  On Earth, tectonic activity occurs by the continental plates moves against each other.  On Mars, tectonic activity is driven by lave flow underneath the surface that pushes the plates vertically.  The planet has some rather impressive surface features. Mars boasts the largest volcanic mountain in the entire solar system, the Olympus Mons.  It is 27km (17 miles) high and 600km (373 miles) wide.  The Valles Marineris is a rift in Mars' surface that would stretch from New York to Los Angeles.  Carbon dioxide comprises 95% of the Martian Atmosphere followed by 3% nitrogen, 1.6% argon, with traces of H2O and oxygen.  There is a fair amount of particulate matter (i.e. dust) in the atmosphere and dust storms are quite common on Mars.

Mars has been the target of many missions, some of which ended in disaster when the spacecraft were never heard of again, such as Mars Climate Orbiter and Mars Polar Lander.  Fortunately, there have been some great recent successes, such as the two Mars rovers, Opportunity and Pathfinder.  Originally slated for 90 days missions each, but 4 years later, they are still going strong and are exploring Mars.  They are analyzing rocks and geologic features.

Martian meteorite ALH 84001 created a stir in the 1990's.  Dr. David McKay and his colleagues theorized that there is evidence that bacterial life existed in Mars 3.5 billion years ago.  In that meteorite are shapes that appear to be fossilized bacterial..  There are also mineral deposits that Dr. McKay theorizes were left behind by the bacteria.  The verdict is still out on this with no real consensus amongst scietntists. 

Mars has 2 very small moons, Phobos and Deimos.  Mariner 9 got up close and personal with Phobos and Deimon.  It spotted a large crater on the surface of Phobos that is 10km (6 miles) wide and is clearly the dominant surface feature.  Both Phobos and Deimon keep the same side to Mars, just like Earth's moon.

Mars Panoramic

Panoramic Photo Mars taken by Pathfinder Rover


Mass (kg) 6.42 x 1023
Diameter (km) 6787
Mean density (kg/m3) 3940
Escape velocity (m/s) 5000
Average distance from Sun 1.524 AU (227,936,640 km)
Rotation period (length of day in Earth days) 1.026
Revolution period (length of year in Earth days)     686.98
Obliquity (tilt of axis degrees) 25
Orbit inclination (degrees) 1.85
Orbit eccentricity (deviation from circular) 0.093
Maximum surface temperature (K) 310
Minimum surface temperature (K) 150
Visual geometric albedo (reflectivity) 0.15
Highest point on surface Olympus Mons
(about 24 km above surrounding lava plains)
Atmospheric components 95% carbon dioxide,
3% nitrogen,
1.6% argon
Surface materials basaltic rock and altered materials
Planet Mars
Picture of
Planet Mars



Martian Moon Phobos
Photograph of
Martian Moon Phobos



Martian Moon Deimon
Image of
Martian Moon Deimos


Olympus Mons
Picture of Olympus
Mons is thelargest
volcanic mountain
in our solar system


Endurance Crater
Endurance Crater as seen
by Mars rover
Opportunity

 



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