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Cerberus Fossae

From Wikipedia, the free encyclopedia

A 3km section of the Cerberus Fossae fissure, taken by the Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC)
A 3km section of the Cerberus Fossae fissure, taken by the Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC)

The Cerberus Fossae are a series of semi-parallel fissures on Mars formed by faults which pulled the crust apart in the Cerberus region (9°N, 197°W). Ripples seen at the bottom of the fault are sand blown by the wind [1]. The underlying cause for the faulting was magma pressure related to the formation of the Elysium Volcanic field, located to the northwest. The faults pass through pre-existing features such as hills, indicating that is is a younger feature[2]. The formation of the fossae is suspected to have released pressurised underground water, previously confined by the cryosphere, with flow rates up to 2 × 106 m3s−1, leading to the creation of the Athabasca Valles. [1]

[edit] References

  1. ^ James W. Head; Lionel Wilson, Karl L. Mitchell (2003). "Generation of recent massive water floods at Cerberus Fossae, Mars by dike emplacement, cryospheric cracking, and confined aquifer groundwater release". Geophysical Research Letters 30 (11). DOI:10.1029/2003GL017135. 

[edit] See also


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