Comparing the Properties of Observed Main-Belt Asteroid Binaries and Modeled Escaping Ejecta Binaries (EEBs) from Numerical Simulations

Details Comparing the Properties of Observed Main-Belt Asteroid Binaries and Modeled Escaping Ejecta Binaries (EEBs) from Numerical Simulations Comparing the Properties of Observed Main-Belt Asteroid Binaries and Modeled Escaping Ejecta Binaries (EEBs) from Numerical Simulations

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2558d&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2558

Computer Science

2

Scientific paper

Parameters of modeled asteroid satellite systems are compared with
observed properties of main-belt asteroid pairs to provide clues to
better understand the origin and evolution of these systems.

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