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Retrospections Methane from Deep Cracks on Mars
 
Methane from Deep Cracks on Mars
Source: ESA press release
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Mars
Posted:   05/12/11

Summary: New images of the Nili Fossae region are helping scientists understand unique geological features in the area. Methane in Mars' atmosphere is enhanced over Nili Fossae, leading some scientists to believe that the gas is produced there. The origins of the Mars methane could be geological or perhaps even biological.


A wider contextual image showing the region around Nili Fossae. Credit: NASA MGS MOLA Science Team
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 strongly eroded impact crater is visible to the bottom right of the image. It measures about 12 km across and exhibits an ejecta blanket, usually formed by material thrown out during the impact. Two landslides have taken place to the west of the crater. Whether they were a direct result of the impact or occurred later is unknown.

A smaller crater, measuring only 3.5 km across, can be seen to the left of centre in the image and this one does not exhibit any ejecta blanket material. It has either been eroded or may have been buried.

Nili Fossae is a system of deep fractures around the giant Isidis impact basin. The deepest are 500 m incisions into the martian crust (1). A strongly eroded large impact crater is visible on the northeastern edge of the area (2) measuring about 12 km across. A smaller impact crater southwest of the fractures measuring just 3.5 km in diameter (3). The surface material on the southwestern image border is much darker than the rest of the area (4). It is probably basaltic rock or volcanic ash originating from Syrtis Major. Credit: ESA/DLR/FU Berlin (G. Neukum)
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.

Nili 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.


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