Martian Upland History: Inconsistencies and Constraints

Details Martian Upland History: Inconsistencies and Constraints Martian Upland History: Inconsistencies and Constraints

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1794h&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1794

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Scientific paper

ALH 84001 & age distribution of Mars meteorites constrain geological
character of Martian uplands as loosely consolidated sediments. A
reservoir of 4.5 Gy crust exists with near-surface exposures in some
regions. A synthesis of Neukum/Hartmann age data is given.

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