On the origins of band topography, Europa

被引:80
作者
Nimmo, F
Pappalardo, RT
Giese, B
机构
[1] UCL, Dept Earth Sci, London WC1E 6BT, England
[2] Univ Colorado, Atmospher & Space Phys Lab, Boulder, CO 80309 USA
[3] DLR, D-12489 Berlin, Germany
关键词
satellites of Jupiter; tectonics; ices; geological processes;
D O I
10.1016/j.icarus.2003.08.002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We use stereo-derived topography of extensional bands on Europa to show that these features can be elevated by 100-150 m with respect to the surroundings, and that the positive topography sometimes extends beyond the band margins. Lateral variations in shell thickness cannot maintain the observed topography for timescales greater than similar to 0.1 Myr. Lateral density variations can maintain the observed topography indefinitely; mean density contrasts of 5 and 50 kg m(-3) are required for shell thicknesses of 20 and 2 km, respectively. Density variations caused by temperature contrasts require either present-day heating or that bands are young features (< 1 Myr old). Stratigraphic analyses suggest that these mechanisms are unlikely. The observation that bands form from ridges may be explained by an episode of shear-heating on ridges weakening the ridge area, and leading to strain localization during extension. Fracture porosity is likely to persist over Myr timescales in the top one-third to one-quarter of the conductive part of the ice shell. Lateral variations in this porosity (of order 20%) are the most likely mechanism for producing band topography if the ice shell is thin (approximate to 2 km); porosity variations of 2% or less are required if the shell is thicker (approximate to 20 km). If the ice shell is thick, lateral variations in salt content are a more likely mechanism. Warm ice will tend to lose dense, low-melting temperature phases and be buoyant relative to colder, salt-rich ice. Thus, lateral density variations will arise naturally if bands have been the sites of either localized heating or upwelling of warm ice during extension. (C) 2003 Elsevier Inc. All rights reserved.
引用
收藏
页码:21 / 32
页数:12
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