| Mars
Overview
With the exception of Earth, Mars is the most popular
planet for science-fiction writers. Today, it is now the most popular
planet on the Internet as well. The current NASA mission has turned
everyone eyes to the “Red Planet” in hopes that it can answer
some of our questions. Luckily, there is already a great deal that we
know about Mars through previous missions.
Mars is the fourth planet from the sun and the third smallest. It is
approximately half the size of Earth but has only one tenth the mass.
Because of this, the force of gravity on Mars is less than that on Earth.
Going to Mars would be a quick way to lose weight, as a 150-pound person
would only weigh 56.5 pounds standing on the surface of Mars. (Check
out www.exploratorium.edu/ronh/weight
to find out what you’d weigh on other planets!)
Here on Earth, plate tectonics cause the crust to slowly move on top
of the mantle. This is why we have earthquakes and island chains, like
Hawaii. On Mars, there is currently no evidence for tectonic motion.
Combined with the lower gravity, this is why Mars is home to the largest
mountains in the solar system. The Tharsis region on Mars is an area
almost 2500 miles across and reaches over 6 miles high. The title of
largest mountain in the solar system goes to Olympus Mons. This single
mountain is 310 miles across and almost 15 miles tall. As a point of
reference, Mt. Everest, the tallest peak on Earth, is only 5.5 miles
high.
Besides Olympus Mons, another striking feature is Valles Marineris.
Visible from Earth, this giant canyon stretches for 2500 miles and can
be as much as 5 miles deep. Originally Valles Marineris was viewed as
part of a gigantic system of manmade, or should I say Martian-made structures.
Giovanni Schiaparelli, an Italian astronomer first observed Mars in
1877 and observed “canali”- the Italian word for “channels.”
The word made some people think that they were canals used by a Martian
civilization. Percival Lowell did some of the most extensive observations
of Mars and discovered over 500 canals, which he wrote about in his
1903 book Mars and it’s Canals. Unfortunately, when our spacecraft
reached Mars, we discovered that there were no canals.
Canals actually would not have been very useful on Mars. It’s
located 142 million miles away from the sun, (one and a half times farther
than the Earth) and has a very thin atmosphere. The average temperature
on the surface of Mars is –81°F, far below the freezing point
of water. The atmosphere also cools very quickly as temperatures during
the day reach can often reach 60°F but then drop to –135°F
during the night. While Mars currently cannot support liquid water on
the surface, there are trace amounts of water vapor in the atmosphere
as well as ice in the Martian poles. There appears to be evidence that
there once was water on the surface and that there may still be liquid
water below. One of the Mars Exploration Rovers jobs will be to find
evidence of water on Mars.
Some Basic Facts about Mars Compared to the Earth...
| |
Earth |
Mars |
| Distance from Sun |
93,000,000 miles |
142,000,000 miles |
| Diameter |
7926 miles |
4220 miles |
| Day (in Earth hours) |
23 hours, 56 minutes |
24 horus, 37 minutes |
| Year (in Earth days) |
365.25 days |
687 days |
| Tilt of Axis |
23.5 degrees |
25 degrees |
| Orbital Eccentricity |
0.0167 degrees |
0.0934 degrees |
| Surface Gravity |
9.8 m/s2 |
9.8 m/s2 |
| Escape velocity |
11.18 km/s |
5.02 km/s |
| Moons |
1 |
2 - Phobos and Deimos |
| Atmospheric Pressure |
1013 millibars |
7 millibars |
| Atmospheric Composition |
77% nitrogen
21% oxygen
1% argon
0.037% carbon dioxide |
95% carbon dioxide
2.7% nitrogen
1.6% argon
13% oxygen |
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