News on Mars
- Discovery of significant changes in Martian sand-dunes
- Signs of ancient flowing water on Mars
- ESAs Mars Express gravity results plot volcanic history
- Impact sites hint at life on Mars
- Pit chains may hold caverns ideal for life
- New explanation for layered deposits in Mars Grand-Canyon
- A mounting - INSIDE a crater on Mars
- Wake-up on to a dusty season on Mars
- Discovery of new kind of surface on mars
- Lakes and shorelines on mars
- Tornado on Mars
- Recent geological activity on Mars
- ESA's Mars-express find evidence of past ocean
- Surface on Mars unlikely place for life
- Mars: A thin but windy atmosphere
- Observing campain of Mars's north pole
- Landslides on Mars occur spontaniously
- Martian avalanches caused by meteor impacts
- Water on Mars: maybe martian microbes
- Mars rover finds mineral vein deposited by water
- Martian polar gullies created by CO2 fluidation
- Sand-dunes move on Mars
- Most Martian-clay is subsurface originated
- Direct measurement of Mars's past temperature
- Clusters of newly formed craters on Mars
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Mars facts

Mars: 4th planet from the Sun
Distance from Sun: 228mio km.
Diameter: 6.794km.
Surface-pressure: 0,001atm.
Atm composition: 99% CO
Temp: -100ºC to +20ºC
Moons: Phobos & Deimos
Newsletter
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A workhorse in orbit
Monday, 21 March 2011 13:12
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| Solar system - Mars |
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The 2001 Mars Odyssey orbiter is still cirkling Mars after 10years, making in the hardest working Mars-spacecraft in history. This image shows the Chasme Borealis valley that cuts through Mars's North pole
Chasma Boreale is a long, flat-floored valley that cuts deep into Mars' north polar icecap. Its walls rise about 1,4km above the floor. Where the edge of the ice cap has retreated, sheets of sand are emerging that accumulated during earlier ice-free climatic cycles. Winds blowing off the ice have pushed loose sand into dunes and driven them down-canyon in a westward direction, toward our viewpoint. Click image for full-resolution 2000 x 4000pixels image NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Science Mission Directorate, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University Source: NASA |




