Accumulation of Distal Impact Ejecta on Mars Since the Hesperian

Details Accumulation of Distal Impact Ejecta on Mars Since the Hesperian Accumulation of Distal Impact Ejecta on Mars Since the Hesperian

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003mars.conf.3242w&link_type=abstract

Sixth International Conference on Mars, July 20-25 2003, Pasadena, California, abstract no.3242

Physics

1

Scientific paper

Cumulative deposits of glass-rich distal ejecta from a series of
Hesperian-aged (and younger) craters could supply a plausible source for
an ejecta-based origin of the enigmatic dark materials found on Mars.

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