Comparison Between Elysium Fossae Ridges and Terrestrial Sub-ice Volcanoes
Ridges and mounds that resemble terrestrial sub-ice tindars occur at the east edge of the Utopia Planitia basin, just west of a long, linear scarp that trends northeast across the west flank of Elysium Mons from about 21° N to 30°N. (Chapman, 1994). Volcanic features and deposits that occur upslope and east of the scarp show no evidence of interaction with surface ice. West of the scarp, channels and other fluidized-appearing materials are prominent on Utopia Planitia. The ridges follow the same northeast trend as the Elysium Fossae troughs on the west flank of the Elysium Mons volcano.
Reference for Sub-ice Volcanic Origin of Elysium/Utopia Deposits
Allen, C. C., 1979a. Volcano-ice interactions on Mars, J. Geophys. Res. 84, 8048-8059.
Allen, C. C., 1979b. Volcano-ice interactions on the Earth and Mars, NASA TM 81979, 164-326.
Anderson, D. M., 1992. Glaciation in Elysium, MSATT Workshop Polar Regions of Mars, (abs.) Lunar Planet. Sci. Inst. Tech. Rept. 92-08(1).
Chapman, M. G., 1994. Evidence, age, and thickness of a frozen paleolake in Utopia Planitia, Mars, Icarus 109, 393-406
Chapman, M.G., 2003, Sub-ice volcanoes and ancient oceans/lakes: A Martian challenge, in Subglacial lakes' detection, outbursts mechanisms and consequences, Amir Moktari-Fard (Ed.), Special Paper on Subglacial Lake Detection, Global and Planetary Change 35, 185-198.
Hodges C. A., and H. J. Moore, 1978. Tablemountains of Mars, (abs.) Lunar Planet. Sci. Conf. 9th, 523-525.
|