Topographic Controls on Martian Valley Networks: Implications for Climate Change During the Noachian Period

Details Topographic Controls on Martian Valley Networks: Implications for Climate Change During the Noachian Period Topographic Controls on Martian Valley Networks: Implications for Climate Change During the Noachian Period

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2436i&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2436

Physics

1

Scientific paper

Topographic controls on martian valley networks are mostly large, early
Noachian features that underwent slow aqueous weathering and erosion in
an arid to hyperarid Noachian paleoclimate, followed by valley
entrenchment around the Noachian/Hesperian transition.

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