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It looks like it will be another six months before the Mars
Reconnaissance Orbiter (MRO) completes its aerobraking maneuvers. But pictures of Phobos and Deimos on the MRO website - http://marsprogram.jpl.nasa.gov/facts/phobos.html http://marsprogram.jpl.nasa.gov/facts/deimos.html - and some recent reading on Roche limits - http://en.wikipedia.org/wiki/Roche_l...ected_examples - reminded me of the striations seen on Phobos but not Deimos. See http://marsprogram.jpl.nasa.gov/facts/phobos.html According to the Wikipedia entry on Roche limits, Phobos orbits within its fluid Roche limit for Mars: Body | Rigid Roche Limit | Fluid Roche Limit Phobos 172% 89% Deimos 451% 233% Maybe this explains the horizontal striations seen on Phobos? Or is there a consensus explanation of the Phobos striations from the professional astronomers? - Canopus56 |
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