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.

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
|
|

Picture of
Planet Mars

Photograph of
Martian Moon Phobos

Image of
Martian Moon Deimos

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

Endurance Crater as seen
by Mars rover
Opportunity
|