Normal fault growth in analog models and on Mars

被引:17
|
作者
Wyrick, Danielle Y. [1 ]
Morris, Alan P. [1 ]
Ferrill, David A. [1 ]
机构
[1] So Res Inst, Dept Earth Mat & Planetary Sci, San Antonio, TX 78238 USA
关键词
Geological processes; Mars; Tectonics; Terrestrial planets; SCALING RELATIONS; SEGMENT LINKAGE; ALBA-PATERA; DISPLACEMENT; LENGTH; EXPLANATION; POPULATION; DIMENSIONS; SLIP;
D O I
10.1016/j.icarus.2011.01.011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Normal faults observed in extensional clay models evolve by displacement (throw) accumulation and concomitant trace length increase, and by segment linkage. The first of these processes leads to an increase in the maximum throw to trace length (D-max/L) ratio, whereas the second leads to a decrease in this ratio. With increasing extension individual faults evolve along stepwise tracks in D-max/L. parameter space, although at any given time a summary plot of D-max versus L for the entire fault population will typically span one order of magnitude in D-max/L ratio and two orders of magnitude in trace length, obscuring the stepwise nature of fault evolution and giving the impression of self-similar fault growth along a locus of constant D-max/L ratio. In addition, the number of simple faults (faults with a single throw maximum) incorporated into a compound fault (a fault with multiple throw maxima) is strongly correlated with the fault's trace length, indicating that trace length increase is dominated by linkage not throw accumulation. When analyzed for evidence of relict simple faults (expressed as throw maxima), normal faults observed on Mars exhibit similar characteristics to those developed in analog clay models. By analogy, we infer that Mars normal faults evolve in a similar fashion to faults in clay models. (C) 2011 Elsevier Inc. All rights reserved.
引用
收藏
页码:559 / 567
页数:9
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