Presidential Address: Presented 2000 August 28, Chicago, Illinois, USA The eucrite/Vesta story

Abstract— Many lines of evidence indicate that meteorites are derived from the asteroid belt but, in general, identifying any meteorite class with a particular asteroid has been problematical. One exception is asteroid 4 Vesta, where a strong case can be made that it is the ultimate source of the ho...

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Published in:Meteoritics & Planetary Science
Main Author: DRAKE, Michael J.
Format: Article in Journal/Newspaper
Language:English
Published: Wiley 2001
Subjects:
Online Access:http://dx.doi.org/10.1111/j.1945-5100.2001.tb01892.x
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spelling crwiley:10.1111/j.1945-5100.2001.tb01892.x 2024-09-15T18:36:48+00:00 Presidential Address: Presented 2000 August 28, Chicago, Illinois, USA The eucrite/Vesta story DRAKE, Michael J. 2001 http://dx.doi.org/10.1111/j.1945-5100.2001.tb01892.x https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fj.1945-5100.2001.tb01892.x https://onlinelibrary.wiley.com/doi/pdf/10.1111/j.1945-5100.2001.tb01892.x en eng Wiley http://onlinelibrary.wiley.com/termsAndConditions#vor Meteoritics & Planetary Science volume 36, issue 4, page 501-513 ISSN 1086-9379 1945-5100 journal-article 2001 crwiley https://doi.org/10.1111/j.1945-5100.2001.tb01892.x 2024-07-25T04:21:37Z Abstract— Many lines of evidence indicate that meteorites are derived from the asteroid belt but, in general, identifying any meteorite class with a particular asteroid has been problematical. One exception is asteroid 4 Vesta, where a strong case can be made that it is the ultimate source of the howardite‐eucrite‐diogenite (HED) family of basaltic achondrites. Visible and near‐infrared reflectance spectra first suggested a connection between Vesta and the basaltic achondrites. Experimental petrology demonstrated that the eucrites (the relatively unaltered and unmixed basaltic achondrites) were the product of approximately a 10% melt. Studies of siderophile element partitioning suggested that this melt was the residue of an asteroidal‐scale magma ocean. Mass balance considerations point to a parent body that had its surface excavated, but remains intact. Modern telescopic spectroscopy has identified kilometer‐scale “Vestoids” between Vesta and the 3:1 orbit‐orbit resonance with Jupiter. Dynamical simulations of impact into Vesta demonstrate the plausibility of ejecting relatively unshocked material at velocities consistent with these astronomical observations. Hubble Space Telescope images show a 460 km diameter impact basin at the south pole of Vesta. It seems that nature has provided multiple free sample return missions to a unique asteroid. Major challenges are to establish the geologic context of the HED meteorites on the surface of Vesta and to connect the remaining meteorites to specific asteroids. Article in Journal/Newspaper South pole Wiley Online Library Meteoritics & Planetary Science 36 4 501 513
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language English
description Abstract— Many lines of evidence indicate that meteorites are derived from the asteroid belt but, in general, identifying any meteorite class with a particular asteroid has been problematical. One exception is asteroid 4 Vesta, where a strong case can be made that it is the ultimate source of the howardite‐eucrite‐diogenite (HED) family of basaltic achondrites. Visible and near‐infrared reflectance spectra first suggested a connection between Vesta and the basaltic achondrites. Experimental petrology demonstrated that the eucrites (the relatively unaltered and unmixed basaltic achondrites) were the product of approximately a 10% melt. Studies of siderophile element partitioning suggested that this melt was the residue of an asteroidal‐scale magma ocean. Mass balance considerations point to a parent body that had its surface excavated, but remains intact. Modern telescopic spectroscopy has identified kilometer‐scale “Vestoids” between Vesta and the 3:1 orbit‐orbit resonance with Jupiter. Dynamical simulations of impact into Vesta demonstrate the plausibility of ejecting relatively unshocked material at velocities consistent with these astronomical observations. Hubble Space Telescope images show a 460 km diameter impact basin at the south pole of Vesta. It seems that nature has provided multiple free sample return missions to a unique asteroid. Major challenges are to establish the geologic context of the HED meteorites on the surface of Vesta and to connect the remaining meteorites to specific asteroids.
format Article in Journal/Newspaper
author DRAKE, Michael J.
spellingShingle DRAKE, Michael J.
Presidential Address: Presented 2000 August 28, Chicago, Illinois, USA The eucrite/Vesta story
author_facet DRAKE, Michael J.
author_sort DRAKE, Michael J.
title Presidential Address: Presented 2000 August 28, Chicago, Illinois, USA The eucrite/Vesta story
title_short Presidential Address: Presented 2000 August 28, Chicago, Illinois, USA The eucrite/Vesta story
title_full Presidential Address: Presented 2000 August 28, Chicago, Illinois, USA The eucrite/Vesta story
title_fullStr Presidential Address: Presented 2000 August 28, Chicago, Illinois, USA The eucrite/Vesta story
title_full_unstemmed Presidential Address: Presented 2000 August 28, Chicago, Illinois, USA The eucrite/Vesta story
title_sort presidential address: presented 2000 august 28, chicago, illinois, usa the eucrite/vesta story
publisher Wiley
publishDate 2001
url http://dx.doi.org/10.1111/j.1945-5100.2001.tb01892.x
https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fj.1945-5100.2001.tb01892.x
https://onlinelibrary.wiley.com/doi/pdf/10.1111/j.1945-5100.2001.tb01892.x
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op_source Meteoritics & Planetary Science
volume 36, issue 4, page 501-513
ISSN 1086-9379 1945-5100
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op_doi https://doi.org/10.1111/j.1945-5100.2001.tb01892.x
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