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
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Deep fractures on Mars
Monday, 09 May 2011 08:50
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| Solar system - Mars |
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ESA's Mars Express satellite orbiting Mars has documented deep fractures in the surface of Mars. The huge canyons were robably caused by surface-tensions, when a very large impact crater flooded with lava cooled of
Newly released images from ESA’s Mars Express show Nili Fossae, a system of deep fractures around the giant Isidis impact basin. Some of these incisions into the martian crust are up to 500 m deep and probably formed at the same time as the basin. Nili Fossae is a ‘graben’ system on Mars, northeast of the Syrtis Major volcanic province, on the northwestern edge of the giant Isidis impact basin. Graben refers to the lowered terrain between two parallel faults or fractures in the rocks that collapses when tectonic forces pull the area apart. The Nili Fossae system contains numerous graben concentrically oriented around the edges of the basin. It is thought that flooding of the basin with basaltic lava after the impact that created it resulted in subsidence of the basin floor, adding stress to the planet’s crust, which was released by the formation of the fractures.
A small 3,5km crater whitout any ejecta blanket material, can be seen in the bottom left of the imag . The ejecta is either eroded or may have been buried. The surface material to the top left of the image is much darker than the rest of the area. It is most likely formed of basaltic rock or volcanic ash originating from the Syrtis Major region. Such lava blankets form when large amounts of low-viscosity basaltic magma flow across long distances before cooling and solidifying. On Earth, the same phenomenon can be seen in the Deccan Traps in India. ili Fossae interests planetary scientists because observations taken with telescopes on the Earth and published in 2009 have shown that there is a significant enhancement in Mars’ atmospheric methane over this area, suggesting that methane may be being produced there. Its origin remains mysterious, however, and could be geological or perhaps even biological. As a result, understanding the origin of methane on Mars is high on the priority list and in 2016, ESA and NASA plan to launch the ExoMars Trace Gas Orbiter to investigate further. Nili Fossae will be observed with great interest. Source: Mars Express homepage at ESA |




