Figure 8 from High-fidelity Modeling of Rotationally Fissioned Asteroids

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High-fidelity Modeling of Rotationally Fissioned Asteroids

Authors: Alex B. Davis and Daniel J. Scheeres

2020 The Planetary Science Journal 1 25.

Provider: AAS Journals

Caption: Figure 8.

Magnitude of relative velocity as the secondary crosses the primary’s sphere of influence (SOI) for Moshup simulations. The sphere of influence for the Moshup primary is 10,370 m in radius.

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