A hypothesis for the low inclination of the orbits of the Martian moons following capture is presented, in which the inclination is reduced by the cumulative effect of ejection and re-accretion of material from the surfaces.
Eccentricity and Inclination Reduction Following Capture of Martian Moons
52nd Lunar and Planetary Science Conference (LPSC 52) ; 2021 ; Virtual, US
Aufsatz (Konferenz)
Keine Angabe
Englisch
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