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Venus tesserae feature layered, folded, and eroded rocks
Tesserae on Venus are locally the stratigraphically oldest units preserved on the planet. These regions are characterized by pervasive tectonic deformation including normal faults, grabens, thrust faults, and folds. In multiple tesserae, sets of (often highly) curved, parallel linear features are al...
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Published in: | Geology (Boulder) 2021-01, Vol.49 (1), p.81-85 |
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description | Tesserae on Venus are locally the stratigraphically oldest units preserved on the planet. These regions are characterized by pervasive tectonic deformation including normal faults, grabens, thrust faults, and folds. In multiple tesserae, sets of (often highly) curved, parallel linear features are also present. These features strongly resemble terracing in layered volcanic or sedimentary sequences on Earth having arcuate or sinuous outcrop patterns that follow undulating topography. Should this analogy hold for Venus, then these outcrop patterns imply some erosion of the tessera units in which these strata occur; radar-dark materials filling proximal lows might be deposits of that eroded material. This outcrop pattern is seen in geographically dispersed tessera units, so the preservation of layering could be common for this terrain type. If so, then tesserae record the culmination of volcanic and/or sedimentary deposition, folding, and erosion-complex geological histories that should be considered in future studies of this enigmatic terrain. |
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M. Celal ; Klimczak, Christian ; Senske, David A ; Whitten, Jennifer L ; Khawja, Sara ; Ernst, Richard E ; Solomon, Sean C</creator><creatorcontrib>Byrne, Paul K ; Ghail, Richard C ; Gilmore, Martha S ; Sengor, A. M. Celal ; Klimczak, Christian ; Senske, David A ; Whitten, Jennifer L ; Khawja, Sara ; Ernst, Richard E ; Solomon, Sean C</creatorcontrib><description>Tesserae on Venus are locally the stratigraphically oldest units preserved on the planet. These regions are characterized by pervasive tectonic deformation including normal faults, grabens, thrust faults, and folds. In multiple tesserae, sets of (often highly) curved, parallel linear features are also present. These features strongly resemble terracing in layered volcanic or sedimentary sequences on Earth having arcuate or sinuous outcrop patterns that follow undulating topography. Should this analogy hold for Venus, then these outcrop patterns imply some erosion of the tessera units in which these strata occur; radar-dark materials filling proximal lows might be deposits of that eroded material. This outcrop pattern is seen in geographically dispersed tessera units, so the preservation of layering could be common for this terrain type. 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Should this analogy hold for Venus, then these outcrop patterns imply some erosion of the tessera units in which these strata occur; radar-dark materials filling proximal lows might be deposits of that eroded material. This outcrop pattern is seen in geographically dispersed tessera units, so the preservation of layering could be common for this terrain type. If so, then tesserae record the culmination of volcanic and/or sedimentary deposition, folding, and erosion-complex geological histories that should be considered in future studies of this enigmatic terrain.</description><subject>Alpha Regio</subject><subject>Aphrodite Terra</subject><subject>arcuate features</subject><subject>basalts</subject><subject>chemical weathering</subject><subject>Deformation</subject><subject>emissivity</subject><subject>erosion</subject><subject>exhumation</subject><subject>Extraterrestrial geology</subject><subject>Fault lines</subject><subject>faults</subject><subject>folds</subject><subject>Geological faults</subject><subject>Geology</subject><subject>grabens</subject><subject>igneous rocks</subject><subject>imagery</subject><subject>layered materials</subject><subject>linear features</subject><subject>Magellan Program</subject><subject>morphology</subject><subject>normal faults</subject><subject>Outcrops</subject><subject>Ovda Regio</subject><subject>paleoatmosphere</subject><subject>patterns</subject><subject>planets</subject><subject>Radar</subject><subject>radar methods</subject><subject>sedimentary rocks</subject><subject>surface features</subject><subject>Tectonics</subject><subject>Tellus Tessera</subject><subject>Terracing</subject><subject>Terrain</subject><subject>terrains</subject><subject>terrestrial comparison</subject><subject>terrestrial planets</subject><subject>tesserae</subject><subject>Thrust faults</subject><subject>Venus</subject><subject>Venus surface</subject><subject>volcanic rocks</subject><subject>weathering</subject><issn>0091-7613</issn><issn>1943-2682</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNpNkE1LxDAURYMoOI6CP6HgRtBqXj6aZinDOAoDbtRtSNMXmbE2Y9Ii8-_NUBfCg3sXh_PgEnIJ9A6A0_uVUFrkfkRmoAUvWVWzYzKjVEOpKuCn5CylLaUgpKpnpH7HfkzFgClhtFh4tMMYsejsHiO2t4UPXXtI27cFxpB7EYP7TOfkxNsu4cVfzsnb4_J18VSuX1bPi4d1aTmIoRTK-3zUoVcKGimRSQCrKtFiA9qDReWbbFXOaSGFVjrzvLGtY84Lz-fkavLuYvgeMQ1mG8bY55eGibqmupJMZep6olwMKUX0Zhc3XzbuDVBz2MVMuxjI6M2EfmBIboO9w58Qu_aflzJqqGJSA_8FYe5jWQ</recordid><startdate>20210101</startdate><enddate>20210101</enddate><creator>Byrne, Paul K</creator><creator>Ghail, Richard C</creator><creator>Gilmore, Martha S</creator><creator>Sengor, A. 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Celal</creatorcontrib><creatorcontrib>Klimczak, Christian</creatorcontrib><creatorcontrib>Senske, David A</creatorcontrib><creatorcontrib>Whitten, Jennifer L</creatorcontrib><creatorcontrib>Khawja, Sara</creatorcontrib><creatorcontrib>Ernst, Richard E</creatorcontrib><creatorcontrib>Solomon, Sean C</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Water Resources Abstracts</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><jtitle>Geology (Boulder)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Byrne, Paul K</au><au>Ghail, Richard C</au><au>Gilmore, Martha S</au><au>Sengor, A. 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These features strongly resemble terracing in layered volcanic or sedimentary sequences on Earth having arcuate or sinuous outcrop patterns that follow undulating topography. Should this analogy hold for Venus, then these outcrop patterns imply some erosion of the tessera units in which these strata occur; radar-dark materials filling proximal lows might be deposits of that eroded material. This outcrop pattern is seen in geographically dispersed tessera units, so the preservation of layering could be common for this terrain type. If so, then tesserae record the culmination of volcanic and/or sedimentary deposition, folding, and erosion-complex geological histories that should be considered in future studies of this enigmatic terrain.</abstract><cop>Boulder</cop><pub>Geological Society of America (GSA)</pub><doi>10.1130/G47940.1</doi><tpages>5</tpages></addata></record> |
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subjects | Alpha Regio Aphrodite Terra arcuate features basalts chemical weathering Deformation emissivity erosion exhumation Extraterrestrial geology Fault lines faults folds Geological faults Geology grabens igneous rocks imagery layered materials linear features Magellan Program morphology normal faults Outcrops Ovda Regio paleoatmosphere patterns planets Radar radar methods sedimentary rocks surface features Tectonics Tellus Tessera Terracing Terrain terrains terrestrial comparison terrestrial planets tesserae Thrust faults Venus Venus surface volcanic rocks weathering |
title | Venus tesserae feature layered, folded, and eroded rocks |
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