The compositional and physical properties of localized lunar pyroclastic deposits

被引:20
作者
Trang, David [1 ]
Gillis-Davis, Jeffrey J. [1 ]
Lemelin, Myriam [1 ]
Cahill, Joshua T. S. [2 ]
Hawke, B. Ray [1 ]
Giguere, Thomas A. [1 ]
机构
[1] Univ Hawaii Manoa, Hawaii Inst Geophys & Planetol, 1680 East West Rd, Honolulu, HI 96822 USA
[2] Johns Hopkins Univ, Appl Phys Lab, 11100 Johns Hopkins Rd, Laurel, MD 20723 USA
关键词
Moon; surface; Radiative transfer; Geological processes; Radar observations; Volcanism; NEAR-INFRARED SPECTRA; REFLECTANCE; ERUPTION; MANTLE; IMPACT; CRATER; EARTH; SPECTROSCOPY; OLIVINE; REGION;
D O I
10.1016/j.icarus.2016.09.025
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Lunar localized pyroclastic deposits are low albedo deposits with areas < 2500 km(2). These deposits were difficult to study before the turn of the millennium because of the lack of available high spatial-resolution data. With the launch of the Lunar Reconnaissance Orbiter, Kaguya, and Chaandrayan-1, new sets of diverse high spatial-resolution data are now available. Using several of these data sets, we conducted a study of 34 localized pyroclastic deposits globally. For each localized pyroclastic deposit, we examined topography to estimate pyroclastic volume and juvenile proportions, S-band radar backscatter, thermal infrared-derived measures of surficial rock abundance and regolith density, and mineral abundances. Our goals are to (1) quantitatively characterize the physical and mineralogical properties of each localized pyroclastic deposit, (2) investigate the physical and mineralogical variations among localized pyroclastic deposits, (3) compare these properties of localized (< 2500 km(2)) to regional pyroclastic deposits (> 2500 km(2)), and (4) provide useful parameters for future volcanological modeling. From this study, we find that: (1) localized pyroclastic deposits exhibit low relief structures, (2) the surface rock abundance and circular polarization ratio of localized pyroclastic deposits display a wide range of values (0.2-0.5% and 0.3-0.6, respectively), (3) the glass abundance of localized pyroclastic deposits vary between 0 and similar to 80 wt.%, (4) there are four types of localized pyroclastic deposits based upon the surface rock abundance and glass abundance parameters, (5) pyroclastic deposits within the same floor-fractured crater tend to have similar properties, and (6) localized pyroclastic deposits are diverse with respect to regional pyroclastic deposits, but a subset of localized pyroclastic deposits have similar physical and mineralogical properties to regional pyroclastic deposits. (C) 2016 Elsevier Inc. All rights reserved.
引用
收藏
页码:232 / 253
页数:22
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