The Origins of Phobos Grooves from Ejecta Launched from Impact Craters on Mars: Tests of the Hypothesis

Details The Origins of Phobos Grooves from Ejecta Launched from Impact Craters on Mars: Tests of the Hypothesis The Origins of Phobos Grooves from Ejecta Launched from Impact Craters on Mars: Tests of the Hypothesis

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1054r&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1054

Physics

Scientific paper

With modeling techniques, we test six major predictions of the J. Murray
hypothesis (that the main groove-forming process on Phobos is the
intersection of Phobos with ejecta from primary impact events on Mars to
produce chains of secondary craters).

Affiliated with

Also associated with

No associations

Rating

The Origins of Phobos Grooves from Ejecta Launched from Impact Craters on Mars: Tests of the Hypothesis does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Origins of Phobos Grooves from Ejecta Launched from Impact Craters on Mars: Tests of the Hypothesis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Origins of Phobos Grooves from Ejecta Launched from Impact Craters on Mars: Tests of the Hypothesis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1563499