CLASS/FSI Seminar Series 2020
Jan 14 - Apr 7, 2020
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SwRI’S Martian Moons Model Indicates Formation Following Large Impact
SSERVI researchers used state-of-the-art models to show that a Vesta-to-Ceres-sized impactor could produce Mars’ small moons.
Water ice and other frozen volatiles are to be found in many shadowed craters near the lunar poles.