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• W2783138443 abstract "We show that a model in which Mars grows near Earth and Venus but is then scattered out of the terrestrial region yields a natural pathway to explain the low masses of the Martian moons Phobos and Deimos. In this scenario, the last giant impact experienced by Mars is followed by an extended period (tens to hundreds of Myr) of close passages by other planetary embryos. These close passages perturb and dynamically heat any system of forming satellites left over by the giant impact and can substantially reduce the mass in the satellite system (sometimes to zero). The close passage of massive perturbing bodies also offers the opportunity to capture small objects by three-body scattering. Both mechanisms lead to low-mass moon systems with a substantially collisional history." @default.
• W2783138443 created "2018-01-26" @default.
• W2783138443 creator A5022867222 @default.
• W2783138443 date "2018-01-08" @default.
• W2783138443 modified "2023-09-26" @default.
• W2783138443 title "A dynamical context for the origin of Phobos and Deimos" @default.
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• W2783138443 doi "https://doi.org/10.1093/mnras/stx3361" @default.
• W2783138443 hasPublicationYear "2018" @default.
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