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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Martian soil oxidation-reduction potential not too extreme for life
Friday, 19 August 2011 01:53
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| Solar system - Mars |
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Measurements from the Vikings in the '70's, suggested taht the environment on Mars would be too ixidating to support any life. But new analysis af samples from the Phoenix lander, shows that the oxidation-reduction potential of the soil is only moderate.
Martian soils. Some Viking measurements indirectly suggested that the soils contained highly oxidizing compounds, which could present extremely harsh conditions for life. But recent observations from the Phoenix Mars Mission pointed to evidence of perchlorate, a potentially highly oxidizing compound, in the Martian soils. However, some studies have noted that because perchlorate is highly stable, its presence in Martian soils cannot explain the Viking measurements. Quinn et al. (2011) present a new analysis of Mars soil samples using the Wet Chemistry Laboratory, a component of the Microscopy, Electrochemistry, and Conductivity Analyzer on the NASA Mars Phoenix Lander. They found that although low levels of oxidizing compounds may be present, the oxidation-reduction potential of the soil is moderate and well within the range expected for habitable soils. Source: Geophysical Research Letters |




