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Flow rates and duration within Kasei Valles, Mars: Implications for the formation of a Martian Ocean
Author(s) -
Williams Rebecca M.,
Phillips Roger J.,
Malin Michael C.
Publication year - 2000
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/1999gl010957
Subject(s) - mars exploration program , orbiter , outflow , martian , geology , altimeter , channel (broadcasting) , astrobiology , oceanography , remote sensing , astronomy , physics , engineering , electrical engineering
Calculated maximum discharges for the largest outflow channel system on Mars, Kasei Valles, based on elevation data from the Mars Orbiter Laser Altimeter (MOLA), are 2 to 4 orders of magnitude lower (8 × 10 4 – 2 × 10 7 m³ s −1 ) than estimated previously. Mars Orbiter Camera (MOC) images show morphological evidence consistent with these relatively modest flow rates. Topographic profiles of the outflow channels reveal previously unrecognized narrow, inner channels. Development of a sapping channel network between flow events suggests the system was active over a significant period of time and likely involved several separate flood events. The longer formation history and lower discharge rates may require a long fill time (>25 years) and a warmer climate to form a martian ocean.