Recognition of Sedimentary Rock Occurrences in Satellite and Aerial Images of Other Worlds—Insights from Mars

Sedimentary rocks provide records of past surface and subsurface processes and environments. The first step in the study of the sedimentary rock record of another world is to learn to recognize their occurrences in images from instruments aboard orbiting, flyby, or aerial platforms. For two decades,...

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Autores principales: Kenneth S. Edgett, Ranjan Sarkar
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Publicado: MDPI AG 2021
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Acceso en línea:https://doaj.org/article/afe18e15f9f64b2ab0dbbbe74c2052f9
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spelling oai:doaj.org-article:afe18e15f9f64b2ab0dbbbe74c2052f92021-11-11T18:53:22ZRecognition of Sedimentary Rock Occurrences in Satellite and Aerial Images of Other Worlds—Insights from Mars10.3390/rs132142962072-4292https://doaj.org/article/afe18e15f9f64b2ab0dbbbe74c2052f92021-10-01T00:00:00Zhttps://www.mdpi.com/2072-4292/13/21/4296https://doaj.org/toc/2072-4292Sedimentary rocks provide records of past surface and subsurface processes and environments. The first step in the study of the sedimentary rock record of another world is to learn to recognize their occurrences in images from instruments aboard orbiting, flyby, or aerial platforms. For two decades, Mars has been known to have sedimentary rocks; however, planet-wide identification is incomplete. Global coverage at 0.25–6 m/pixel, and observations from the Curiosity rover in Gale crater, expand the ability to recognize Martian sedimentary rocks. No longer limited to cases that are light-toned, lightly cratered, and stratified—or mimic original depositional setting (e.g., lithified deltas)—Martian sedimentary rocks include dark-toned examples, as well as rocks that are erosion-resistant enough to retain small craters as well as do lava flows. Breakdown of conglomerates, breccias, and even some mudstones, can produce a pebbly regolith that imparts a “smooth” appearance in satellite and aerial images. Context is important; sedimentary rocks remain challenging to distinguish from primary igneous rocks in some cases. Detection of ultramafic, mafic, or andesitic compositions do not dictate that a rock is igneous, and clast genesis should be considered separately from the depositional record. Mars likely has much more sedimentary rock than previously recognized.Kenneth S. EdgettRanjan SarkarMDPI AGarticleMARS sedimentary rockearly MarsMars volcanismextraterrestrial sedimentspacecraft image interpretationsatellite image interpretationScienceQENRemote Sensing, Vol 13, Iss 4296, p 4296 (2021)
institution DOAJ
collection DOAJ
language EN
topic MARS sedimentary rock
early Mars
Mars volcanism
extraterrestrial sediment
spacecraft image interpretation
satellite image interpretation
Science
Q
spellingShingle MARS sedimentary rock
early Mars
Mars volcanism
extraterrestrial sediment
spacecraft image interpretation
satellite image interpretation
Science
Q
Kenneth S. Edgett
Ranjan Sarkar
Recognition of Sedimentary Rock Occurrences in Satellite and Aerial Images of Other Worlds—Insights from Mars
description Sedimentary rocks provide records of past surface and subsurface processes and environments. The first step in the study of the sedimentary rock record of another world is to learn to recognize their occurrences in images from instruments aboard orbiting, flyby, or aerial platforms. For two decades, Mars has been known to have sedimentary rocks; however, planet-wide identification is incomplete. Global coverage at 0.25–6 m/pixel, and observations from the Curiosity rover in Gale crater, expand the ability to recognize Martian sedimentary rocks. No longer limited to cases that are light-toned, lightly cratered, and stratified—or mimic original depositional setting (e.g., lithified deltas)—Martian sedimentary rocks include dark-toned examples, as well as rocks that are erosion-resistant enough to retain small craters as well as do lava flows. Breakdown of conglomerates, breccias, and even some mudstones, can produce a pebbly regolith that imparts a “smooth” appearance in satellite and aerial images. Context is important; sedimentary rocks remain challenging to distinguish from primary igneous rocks in some cases. Detection of ultramafic, mafic, or andesitic compositions do not dictate that a rock is igneous, and clast genesis should be considered separately from the depositional record. Mars likely has much more sedimentary rock than previously recognized.
format article
author Kenneth S. Edgett
Ranjan Sarkar
author_facet Kenneth S. Edgett
Ranjan Sarkar
author_sort Kenneth S. Edgett
title Recognition of Sedimentary Rock Occurrences in Satellite and Aerial Images of Other Worlds—Insights from Mars
title_short Recognition of Sedimentary Rock Occurrences in Satellite and Aerial Images of Other Worlds—Insights from Mars
title_full Recognition of Sedimentary Rock Occurrences in Satellite and Aerial Images of Other Worlds—Insights from Mars
title_fullStr Recognition of Sedimentary Rock Occurrences in Satellite and Aerial Images of Other Worlds—Insights from Mars
title_full_unstemmed Recognition of Sedimentary Rock Occurrences in Satellite and Aerial Images of Other Worlds—Insights from Mars
title_sort recognition of sedimentary rock occurrences in satellite and aerial images of other worlds—insights from mars
publisher MDPI AG
publishDate 2021
url https://doaj.org/article/afe18e15f9f64b2ab0dbbbe74c2052f9
work_keys_str_mv AT kennethsedgett recognitionofsedimentaryrockoccurrencesinsatelliteandaerialimagesofotherworldsinsightsfrommars
AT ranjansarkar recognitionofsedimentaryrockoccurrencesinsatelliteandaerialimagesofotherworldsinsightsfrommars
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