Physics
Scientific paper
Mar 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1093f&link_type=abstract
34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1093
Physics
3
Scientific paper
Three main stages for water evolution are recorded on Mars: a Noachian
/Early Hesperian ocean, portrayed by an almost equipotential line we
name Contact 0; a Late Hesperian sea (Contact 2); and minor lakes
representing Late Hesperian ponded waters.
Anderson Robert C.
Baker Victor R.
de Pablo Miguel A.
Dohm James M.
Fairén Alberto G.
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