Young, Blocky Flows in East Ius/West Melas and West Candor Chasmata, Mars: Debris Avalanche Deposits Derived from Interior Layered Deposit (ILD) Mounds?

Details Young, Blocky Flows in East Ius/West Melas and West Candor Chasmata, Mars: Debris Avalanche Deposits Derived from Interior Layered Deposit (ILD) Mounds? Young, Blocky Flows in East Ius/West Melas and West Candor Chasmata, Mars: Debris Avalanche Deposits Derived from Interior Layered Deposit (ILD) Mounds?

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1361s&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1361

Physics

5

Scientific paper

Several blocky flow deposits occur on the flanks of ILD mounds and on
the floor of Valles Marineris in the East Ius/West Melas and Candor
Chasmata area of Mars. The deposits are interpreted as debris avalanche
deposits, and the blocks may represent wind-eroded debris avalanche
hummocks.

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