|
SCIENCE FRIDAY ON MARS
MARS AT A GLANCE
|
|
|
|
|
|
general
moons
atmosphere/weather
surface
life?
General Planetary Information
- Mars is the fourth planet from the Sun, between Earth and
Jupiter.
- Minimum distance from the Sun: 128.6 million miles.
- Maximum distance from the Sun: 154.8 million miles.
- Minimum distance from Earth: 35 million miles.
- Diameter (avg): 4,200 miles. Earth's diameter is 7,913 miles.
- Volume: approximately 15 percent of Earth's volume.
- Mass: approximately 11 percent of Earth's mass.
- Density (water=1): 3.94. Earth's density=5.52.
- Surface gravity: 38 percent of Earth gravity.
- Length of day: 24 Earth hours, 37 Earth minutes.
- Length of year: 687 Earth days.
- Temperature (mean avg on surface): -45 degrees Fahrenheit.
Earth temperature is 60 degrees.
- Temperature range: -225 degrees F to 63 degrees F.
(calculated)
- Atmosphere (major components): carbon dioxide, with small
amounts of nitrogen, water vapor. Earth's atmosphere is made up of
nitrogen and oxygen, with smaller amounts of water vapor, carbon
dioxide, and argon.
- Albedo (percentage of light reflected back into space): 16
percent. Earth's albedo is 36 percent.
- Tilt of Axis: 25 deg, 12 min.
- Satellites: two, Phobos and Deimos.
general
moons
atmosphere/weather
surface
life?
Satellites
Phobos
Deimos
- Discovered by Asaph Hall, American astronomer, 1877.
- Named Phobos (fear) and Deimos (terror)
- Both irregularly shaped, heavily cratered.
- Phobos is about 5830 miles from the center of Mars. Deimos is
about 14,580 miles from Mars' center.
- Phobos' diameter: about 14 miles. Deimos' diameter: about 7
miles.
- Phobos orbits Mars about once every 7 and a half hours. Deimos
orbits Mars once every 30 hours, 19 minutes.
- both thought to be either pieces ejected from Mars during
early formation, or captured asteroids.
general
moons
atmosphere/weather
surface
life?
Atmosphere and Weather

A dust storm on Mars (look for red covering the ice cap in early
image!)
- Much thinner atmosphere than on Earth.
- Atmospheric pressure is 0.1 pound/square inch, less than 1
percent of Earth's atmospheric pressure.
- Atmosphere mainly carbon dioxide.
- The wind is important on Mars: dunes and drifts of sand and
dust have been observed, as have dust storms.
- Three types of clouds have been observed.
- Pink clounds of dust covering large areas
- Thin bluish clouds, thought to be made of ice crystals.
- Thicker white clouds, possibly water vapor. (only
occasionally seen)
general
moons
atmosphere/weather
surface
life?
Surface Features


Olympus Mons Valles Marineris
South Pole Ice Caps
- Two-thirds of the surface is covered with red-brown material.
Some seems to be limonite, material found in Earth deserts.
- Dark bluish-gray or greenish-gray patches called maria (seas)
cover about one third of the surface.
- The size and shape of the maria change, possibly due to
blowing sand and dust.
- About half the planet, mainly the Southern hemisphere, is
heavily cratered.
- The Northern hemisphere is more smooth, thought to be the
result both of wind-blown sediments and volcanic activity.
- No evidence of plate tectonic activity beyond early stages.
Possibly due to thick crust and mantle.
- Surface has canyons and gorges and features resembling dried
riverbeds, supporting those who think that once Mars had lots of
liquid water on its surface.
- What appear to be white polar ice caps, which shrink and grow
with the seasons, add further support to the liquid water theory.
- The Tharsis region near the equator has many large extinct
volcanoes.
- This includes the largest known volcano in the Solar System,
Olympus Mons, which is about 27 km tall, and 550 km across.
- Nearby is a deep gorge called the Vallis Marineris, possibly
an ancient fault line.
- The Vallis Marineris is over 4000 km long. Parts are over 150
km wide. It is between 2 and 7 km deep.
general
moons
atmosphere/weather
surface
life?
Possible Life?
The Martian Meteorite
Though the Viking mission settled the idea of "canals" on Mars
once and for all, the possibility that liquid water once flowed on
Mars around 4 billion years ago still has people wondering: could
there be some form of life on Mars? Was there life at one time?
Speculation was driven into a frenzy last year with the analysis of
the famous martian meteorite, found in Antarctica in 1984. Scientists
found four types of evidence inside the meteorite:
- masses of carbonates, similar to those produced by
microorganisms on Earth
- iron sulfides and magnetite, also produced by Earth
microorganisms
- traces of polycyclic aromatic hydrocarbons (PAH) produced by
the decay of Earth microorganisms
- tiny tube and egg-shaped objects, only 20 to 100 nanometers
across, resembling fossilized Earth microorganisms (but smaller.)
Not everyone is so sure, though - many people have presented ways
that the four clues could have been made without the help of
microscopic life. Unfortunatly, the Pathfinder/Sojourner mission is
not designed to analyze for traces of life. We'll have to wait for
future missions to do that!
Show related-mail
to:scifri@npr.org. Site-related
mail
to:producer@sciencefriday.c
om.
Science Friday Home |
Science Friday Kids
Connection
©1997, all
rights reserved.