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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The Viking Mars lander found organics on Mars
Wednesday, 12 January 2011 15:28
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| Solar system - Mars |
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When the Viking lander landed on Mars in 1975, NASA actually did find organic compound's; They just didn't belive it! The most comprehensive search for organics in the Martian soil was performed by the Viking Landers. Martian soil was subjected to a thermal volatilization process to vaporize and break organic molecules, and the resultant gases and volatiles were analyzed by gas chromatography-mass spectrometry. Only water at 0.1–1.0 wt% was detected, with traces of chloromethane at 15 ppb, at Viking landing site 1, and water at 0.05–1.0 wt% and carbon dioxide at 50–700 ppm, with traces of dichloromethane at 0.04–40 ppb, at Viking landing site 2. These chlorohydrocarbons were considered to be terrestrial contaminants, although they had not been detected at those levels in the blank runs. Recently, perchlorate was discovered in the Martian Arctic soil by the Phoenix Lander. A new re-analysis of the old data show that when Mars-like soils from the Atacama Desert containing 32 ± 6 ppm of organic carbon are mixed with 1 wt% magnesium perchlorate and heated, nearly all the organics present are decomposed to water and carbon dioxide, but a small amount is chlorinated, forming 1.6 ppm of chloromethane and 0.02 ppm of dichloromethane at 500°C. A chemical kinetics model was developed to predict the degree of oxidation and chlorination of organics in the Viking oven. Re-interpretation of the Viking results therefore suggests ≤0.1% perchlorate and 1.5–6.5 ppm organic carbon at landing site 1 and ≤0.1% perchlorate and 0.7–2.6 ppm organic carbon at landing site 2. The detection of organics on Mars is important to assess locations for future experiments to detect life itself. Source: American Geophysical Union |




