The formation of Rima Parry V

Details The formation of Rima Parry V The formation of Rima Parry V

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..647j&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 647.

Computer Science

Volcanology, Magma, Lunar Surface, Clementine Spacecraft, Lunar Orbiter

Scientific paper

Rima Parry V is a graben in the moon's Fra Mauro Formation which has been captured by Clementine images. Analysis of the Clementine images has shown the presence of a linear feature to the north of Rima Parry V whose altered composition, in conjunction with the presence of a volcanic deposit, suggests that a dike extends under this feature; the linear feature could have been formed before or after the intrusion of the dike.

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