Velocity determination for ejecta from craters in coarse-grained sand

Details Velocity determination for ejecta from craters in coarse-grained sand Velocity determination for ejecta from craters in coarse-grained sand

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..103b&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 103.

Physics

Solar System, Planetary Craters, Ejecta, Sands, Hypervelocity Impact, Velocity Measurement, Mars Craters, Grain Size, Fragmentation, Particle Trajectories

Scientific paper

The present study of impact ejecta raises questions concerning the fragmentation mechanism, ejection angles, and velocity of the ejecta in solar system solid bodies. The results obtained confirm findings that the more vertical trajectories contain material ejected at early stages in the cratering at higher velocities, and the near-horizontal trajectories contain material ejected at lower velocities and at a later stage.

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