Central Pit Craters on Mars: Characteristics, Distributions, and Implications for Formation
نویسنده
چکیده
1242. [8] Kagy H. M. and N. G. Barlow (2008), LPS XXXIX, Abstract #1166. [9] Woronow A. (1981), Icarus, 45, 320-30. [10] Stewart S. T. et al. (2001), LPS XXXII, Abstract #2092. [11] Bray V. J. et al. (2005), LPS XXXVI, Abstract #1889. [12] Dohm J. M. et al. (2007), Icarus, 190, 74-92. [13] Barlow N. G. and T. L. Bradley (1990), Icarus, 87, 156-179. [14] Barlow N. G. and C. B. Perez (2003), JGR, 108, doi: 10.1029/2002JE002036. [15] Pierazzo E. et al. (2005), Large Meteorite Impacts III, 443-457. [16] Stewart S. T. and L. E. Senft (2008), Large Meteorite Impactsand Planetary Evolution Conference IV, Abstract # 1423. Figure 2: Distribution of summit (red) and floor (green) pit craters on Mars, superposed on the GRS water distribution map Figure 3: Ratio of pit diameter to crater diameter (Dp/Dc). Floor pits tend to be larger relative to their crater than summit pits.
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Distributions and Characteristics of Martian Central Pit Craters
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