Morphology of Pit Craters on Mercury from Stereo-Derived Topography and Implications for Pit Crater Formation

Details Morphology of Pit Craters on Mercury from Stereo-Derived Topography and Implications for Pit Crater Formation Morphology of Pit Craters on Mercury from Stereo-Derived Topography and Implications for Pit Crater Formation

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1991g&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1991

Physics

Scientific paper

Pit craters on Mercury occur both inside impact craters and on
intercrater terrain. Morphology derived from MESSENGER stereo images
from orbit suggests formation by collapse above the crustal magma
reservoir, a likely contribution of explosive eruptions.

Affiliated with

Also associated with

No associations

Rating

Morphology of Pit Craters on Mercury from Stereo-Derived Topography and Implications for Pit Crater Formation 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 Morphology of Pit Craters on Mercury from Stereo-Derived Topography and Implications for Pit Crater Formation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Morphology of Pit Craters on Mercury from Stereo-Derived Topography and Implications for Pit Crater Formation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1040118