Wilson, Lionel and Mouginis-Mark, Peter J. (2003) Phreatomagmatic explosive activity at Hrad Vallis, Mars. Journal of Geophysical Research: Planets, 108 (E8). p. 5082. ISSN 2169-9100Full text not available from this repository.
Hrad Vallis is a ∼370 m deep, ∼800 km long depression located at 34°N, 218°W, in Elysium Planitia, Mars. A distinctive deposit, present on both sides of the source area of Hrad Vallis, has a maximum width of ∼70 km along the strike of the depression, a lower unit extends for nearly 100 km away from the depression on either side, and an upper unit extends for ∼50 km. Viking and Mars Orbiter Camera (MOC) images show lobate deposit boundaries, rheomorphic deformation, and numerous craters 270–580 m in diameter within the deposit. The deposit coincides with a broad topographic rise ∼30 km wide and ∼100–150 m high extending along the sides of the valley for at least 100 km along strike. We propose that these features formed when a dike underlying the axis of the valley generated a shallow sill, which in turn is partly responsible for the rise topography. The remainder of the rise consists of a mud-like deposit of ejecta from a large-scale phreatomagmatic explosion due to violent mechanical and thermal mixing between the central part of the sill and ice-rich rock layers in the upper few hundred meters of the crust in a fuel-coolant-type interaction. The observed range and thickness of ejecta and the depth of the Hrad depression imply explosion steam pressures up to 360 MPa, ejecta speeds of ∼400 m s−1, and a sill at least 150 m thick intruded at a depth of ∼350–400 m below the original surface.
|Journal or Publication Title:||Journal of Geophysical Research: Planets|
|Subjects:||G Geography. Anthropology. Recreation > GE Environmental Sciences|
|Departments:||Faculty of Science and Technology > Lancaster Environment Centre|
|Deposited On:||14 Jan 2009 11:46|
|Last Modified:||19 Apr 2016 00:06|
Actions (login required)