GSTDTAP  > 气候变化
DOI10.1029/2018GL079759
High Ice Purity of Martian Lobate Debris Aprons at the Regional Scale: Evidence From an Orbital Radar Sounding Survey in Deuteronilus and Protonilus Mensae
Petersen, Eric Ivan1,2; Holt, John W.2,3; Levy, Joseph S.4
2018-11-16
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2018
卷号45期号:21页码:11595-11604
文章类型Article
语种英语
国家USA
英文摘要

Lobate Debris Aprons (LDA) are martian landforms with a strong morphologic resemblance to rock glaciers and debris-covered glaciers. While the Shallow Radar (SHARAD) sounder has confirmed that a handful of LDA are composed of >80% water ice, viscous flow morphology can also be produced by as little as 30% ice. To distinguish between these endmembers, we conducted a comprehensive regional SHARAD survey of LDA, in Deuteronilus Mensae. We found that the majority of LDA are penetrated by SHARAD and determined that they are composed of a material with epsilon' = 3 and tan delta approximate to 0.002 < 0.005. These LDA are thus consistently composed of >80% water ice, which constrains the regional sequestered ice budget to a minimum of 0.9 - 1.0 x 10(5) km(3) or a 62-69-cm Global Equivalent Layer.


Plain Language Summary Lobate debris aprons (LDA) are dust and rock-covered Martian landforms thought to contain buried water ice due to their resemblance to creeping permafrost and debris-covered glaciers. Their ice content has been the subject of debate; it may be as low as 30% or nearly pure ice. Understanding LDA composition and its variability across Mars is important for exploring climate history and investigating the feasibility of these features as water reservoirs for potential manned missions. The Shallow Radar (SHARAD) instrument on Mars Reconnaissance Orbiter can probe the interior of LDA, constraining their ice content. This has been demonstrated for individual LDA, which were shown to be composed of >80% water ice; however, no regional survey has been made to determine if these LDA are outliers or the norm. We present a survey of LDA composition constrained by SHARAD for the region of Deuteronilus Mensae-a region with abundant, widespread LDA. We found that 87% of LDA were penetrated by SHARAD and that these all had radar properties broadly consistent with high purity (80-90%) water ice. Combining these results with previous LDA volume mapping constrains their water ice content to 4 times the combined volume of the Great Lakes.


领域气候变化
收录类别SCI-E
WOS记录号WOS:000451832600011
WOS关键词GROUND ICE ; SHARAD DATA ; MARS ; DEPOSITS ; STABILITY ; GLACIERS ; PLANITIA
WOS类目Geosciences, Multidisciplinary
WOS研究方向Geology
引用统计
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/28606
专题气候变化
作者单位1.Univ Texas Austin, Univ Texas Inst Geophys, Austin, TX 78712 USA;
2.Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA;
3.Univ Arizona, Dept Geosci, Tucson, AZ 85721 USA;
4.Colgate Univ, Dept Geol, Hamilton, NY 13346 USA
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GB/T 7714
Petersen, Eric Ivan,Holt, John W.,Levy, Joseph S.. High Ice Purity of Martian Lobate Debris Aprons at the Regional Scale: Evidence From an Orbital Radar Sounding Survey in Deuteronilus and Protonilus Mensae[J]. GEOPHYSICAL RESEARCH LETTERS,2018,45(21):11595-11604.
APA Petersen, Eric Ivan,Holt, John W.,&Levy, Joseph S..(2018).High Ice Purity of Martian Lobate Debris Aprons at the Regional Scale: Evidence From an Orbital Radar Sounding Survey in Deuteronilus and Protonilus Mensae.GEOPHYSICAL RESEARCH LETTERS,45(21),11595-11604.
MLA Petersen, Eric Ivan,et al."High Ice Purity of Martian Lobate Debris Aprons at the Regional Scale: Evidence From an Orbital Radar Sounding Survey in Deuteronilus and Protonilus Mensae".GEOPHYSICAL RESEARCH LETTERS 45.21(2018):11595-11604.
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