High Channels on Mars Indicate Hesperian Recharge at Low Latitudes

Details High Channels on Mars Indicate Hesperian Recharge at Low Latitudes High Channels on Mars Indicate Hesperian Recharge at Low Latitudes

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003mars.conf.3071c&link_type=abstract

Sixth International Conference on Mars, July 20-25 2003, Pasadena, California, abstract no.3071

Physics

6

Scientific paper

We identify two Hesperian outflow channels that issued from a
750-km-long fault zone west of Ganges Chasma. One channel stands at
~2600 m, too high to be explained by discharge from a global aquifer.
Recharge from Tharsis was required.

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