The Geologically Recent Giant Impact Basins at Vesta’s South Pole

Dawn’s global mapping of Vesta reveals that its observed south polar depression is composed of two overlapping giant impact features. These large basins provide exceptional windows into impact processes at planetary scales. The youngest, Rheasilvia, is 500 kilometers wide and 19 kilometers deep and...

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Published in:Science
Main Authors: Schenk, P., O'Brien, D.P., Marchi, S., Gaskell, R.W., Preusker, Frank, Roatsch, T., Jaumann, R., Buczkowski, D.L., McCord, T. B., McSween, H.Y., Williams, D.A., Yingst, R. A., Raymond, C.A., Russell, C.T.
Format: Article in Journal/Newspaper
Language:unknown
Published: American Association for the Advancement of Science (AAAS) 2012
Subjects:
Online Access:https://elib.dlr.de/80372/
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author Schenk, P.
O'Brien, D.P.
Marchi, S.
Gaskell, R.W.
Preusker, Frank
Roatsch, T.
Jaumann, R.
Buczkowski, D.L.
McCord, T. B.
McSween, H.Y.
Williams, D.A.
Yingst, R. A.
Raymond, C.A.
Russell, C.T.
author_facet Schenk, P.
O'Brien, D.P.
Marchi, S.
Gaskell, R.W.
Preusker, Frank
Roatsch, T.
Jaumann, R.
Buczkowski, D.L.
McCord, T. B.
McSween, H.Y.
Williams, D.A.
Yingst, R. A.
Raymond, C.A.
Russell, C.T.
author_sort Schenk, P.
collection Unknown
container_issue 6082
container_start_page 694
container_title Science
container_volume 336
description Dawn’s global mapping of Vesta reveals that its observed south polar depression is composed of two overlapping giant impact features. These large basins provide exceptional windows into impact processes at planetary scales. The youngest, Rheasilvia, is 500 kilometers wide and 19 kilometers deep and finds its nearest morphologic analog among large basins on low-gravity icy satellites. Extensive ejecta deposits occur, but impact melt volume is low, exposing an unusual spiral fracture pattern that is likely related to faulting during uplift and convergence of the basin floor. Rheasilvia obliterated half of another 400-kilometer-wide impact basin, Veneneia. Both basins are unexpectedly young, roughly 1 to 2 billion years, and their formation substantially reset Vestan geology and excavated sufficient volumes of older compositionally heterogeneous crustal material to have created the Vestoids and howardite-eucrite-diogenite meteorites.
format Article in Journal/Newspaper
genre South pole
genre_facet South pole
geographic South Pole
geographic_facet South Pole
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institution Open Polar
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op_container_end_page 697
op_doi https://doi.org/10.1126/science.1223272
op_relation Schenk, P. und O'Brien, D.P. und Marchi, S. und Gaskell, R.W. und Preusker, Frank und Roatsch, T. und Jaumann, R. und Buczkowski, D.L. und McCord, T. B. und McSween, H.Y. und Williams, D.A. und Yingst, R. A. und Raymond, C.A. und Russell, C.T. (2012) The Geologically Recent Giant Impact Basins at Vesta’s South Pole. Science, 336, Seiten 694-697. American Association for the Advancement of Science (AAAS). doi:10.1126/science.1223272 <https://doi.org/10.1126/science.1223272>. ISSN 0036-8075.
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publisher American Association for the Advancement of Science (AAAS)
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spelling ftdlr:oai:elib.dlr.de:80372 2025-06-15T14:49:31+00:00 The Geologically Recent Giant Impact Basins at Vesta’s South Pole Schenk, P. O'Brien, D.P. Marchi, S. Gaskell, R.W. Preusker, Frank Roatsch, T. Jaumann, R. Buczkowski, D.L. McCord, T. B. McSween, H.Y. Williams, D.A. Yingst, R. A. Raymond, C.A. Russell, C.T. 2012-05 https://elib.dlr.de/80372/ unknown American Association for the Advancement of Science (AAAS) Schenk, P. und O'Brien, D.P. und Marchi, S. und Gaskell, R.W. und Preusker, Frank und Roatsch, T. und Jaumann, R. und Buczkowski, D.L. und McCord, T. B. und McSween, H.Y. und Williams, D.A. und Yingst, R. A. und Raymond, C.A. und Russell, C.T. (2012) The Geologically Recent Giant Impact Basins at Vesta’s South Pole. Science, 336, Seiten 694-697. American Association for the Advancement of Science (AAAS). doi:10.1126/science.1223272 <https://doi.org/10.1126/science.1223272>. ISSN 0036-8075. Planetengeologie Zeitschriftenbeitrag PeerReviewed 2012 ftdlr https://doi.org/10.1126/science.1223272 2025-06-04T04:58:10Z Dawn’s global mapping of Vesta reveals that its observed south polar depression is composed of two overlapping giant impact features. These large basins provide exceptional windows into impact processes at planetary scales. The youngest, Rheasilvia, is 500 kilometers wide and 19 kilometers deep and finds its nearest morphologic analog among large basins on low-gravity icy satellites. Extensive ejecta deposits occur, but impact melt volume is low, exposing an unusual spiral fracture pattern that is likely related to faulting during uplift and convergence of the basin floor. Rheasilvia obliterated half of another 400-kilometer-wide impact basin, Veneneia. Both basins are unexpectedly young, roughly 1 to 2 billion years, and their formation substantially reset Vestan geology and excavated sufficient volumes of older compositionally heterogeneous crustal material to have created the Vestoids and howardite-eucrite-diogenite meteorites. Article in Journal/Newspaper South pole Unknown South Pole Science 336 6082 694 697
spellingShingle Planetengeologie
Schenk, P.
O'Brien, D.P.
Marchi, S.
Gaskell, R.W.
Preusker, Frank
Roatsch, T.
Jaumann, R.
Buczkowski, D.L.
McCord, T. B.
McSween, H.Y.
Williams, D.A.
Yingst, R. A.
Raymond, C.A.
Russell, C.T.
The Geologically Recent Giant Impact Basins at Vesta’s South Pole
title The Geologically Recent Giant Impact Basins at Vesta’s South Pole
title_full The Geologically Recent Giant Impact Basins at Vesta’s South Pole
title_fullStr The Geologically Recent Giant Impact Basins at Vesta’s South Pole
title_full_unstemmed The Geologically Recent Giant Impact Basins at Vesta’s South Pole
title_short The Geologically Recent Giant Impact Basins at Vesta’s South Pole
title_sort geologically recent giant impact basins at vesta’s south pole
topic Planetengeologie
topic_facet Planetengeologie
url https://elib.dlr.de/80372/