Constraining Source Crater Regions for Boulder Tracks and Elongated Secondary Craters on Eros

Details Constraining Source Crater Regions for Boulder Tracks and Elongated Secondary Craters on Eros Constraining Source Crater Regions for Boulder Tracks and Elongated Secondary Craters on Eros

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.2173d&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

1

Scientific paper

Dynamical models of reaccretion of impact ejecta on asteroids are used
to 'back track' the derived landing trajectories of selected boulders on
Eros, placing constraints on the source regions for the primary impact
craters.

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