Oral histories in meteoritics and planetary science —XVI: Donald D. Bogard

Abstract– Donald D. Bogard (Don, Fig. 1 ) became interested in meteorites after seeing the Fayetteville meteorite in an undergraduate astronomy class at the University of Arkansas. During his graduate studies with Paul Kuroda at Arkansas, Don helped discover the Xe decay products of 244 Pu. After a...

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Published in:Meteoritics & Planetary Science
Main Author: SEARS, Derek W. G.
Format: Article in Journal/Newspaper
Language:English
Published: Wiley 2012
Subjects:
Online Access:http://dx.doi.org/10.1111/j.1945-5100.2012.01333.x
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spelling crwiley:10.1111/j.1945-5100.2012.01333.x 2023-12-03T10:14:03+01:00 Oral histories in meteoritics and planetary science —XVI: Donald D. Bogard SEARS, Derek W. G. 2012 http://dx.doi.org/10.1111/j.1945-5100.2012.01333.x https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fj.1945-5100.2012.01333.x https://onlinelibrary.wiley.com/doi/pdf/10.1111/j.1945-5100.2012.01333.x en eng Wiley http://onlinelibrary.wiley.com/termsAndConditions#vor Meteoritics & Planetary Science volume 47, issue 3, page 416-433 ISSN 1086-9379 1945-5100 Space and Planetary Science Geophysics journal-article 2012 crwiley https://doi.org/10.1111/j.1945-5100.2012.01333.x 2023-11-09T14:16:53Z Abstract– Donald D. Bogard (Don, Fig. 1 ) became interested in meteorites after seeing the Fayetteville meteorite in an undergraduate astronomy class at the University of Arkansas. During his graduate studies with Paul Kuroda at Arkansas, Don helped discover the Xe decay products of 244 Pu. After a postdoctoral period at Caltech, where he learned much from Jerry Wasserburg, Peter Eberhardt, Don Burnett, and Sam Epstein, Don became one of a number of young Ph.D. scientists hired by NASA’s Manned Spacecraft Center to set up the Lunar Receiving Laboratory (LRL) and to perform a preliminary examination of Apollo samples. In collaboration with Oliver Schaeffer (SUNY), Joseph Zähringer (Max Planck, Heidelberg), and Raymond Davis (Brookhaven National Laboratory), he built a gas analysis laboratory at JSC, and the noble gas portion of this laboratory remained operational until he retired in 2010. At NASA, Don worked on the lunar regolith, performed pioneering work on cosmic ray produced noble gas isotopes and Ar‐Ar dating, the latter for important insights into the thermal and shock history of meteorites and lunar samples. During this work, he discovered that the trapped gases in SNC meteorites were very similar to those of the Martian atmosphere and thus established their Martian origin. Among Don’s many administrative accomplishments are helping to establish the Antarctic meteorite and cosmic dust processing programs at JSC and serving as a NASA‐HQ discipline scientist, where he advanced peer review and helped create new programs. Don is a recipient of NASA’s Scientific Achievement and Exceptional Service Medals and the Meteoritical Society’s Leonard Medal. Donald Bogard. image Article in Journal/Newspaper Antarc* Antarctic Wiley Online Library (via Crossref) Antarctic The Antarctic Meteoritics & Planetary Science 47 3 416 433
institution Open Polar
collection Wiley Online Library (via Crossref)
op_collection_id crwiley
language English
topic Space and Planetary Science
Geophysics
spellingShingle Space and Planetary Science
Geophysics
SEARS, Derek W. G.
Oral histories in meteoritics and planetary science —XVI: Donald D. Bogard
topic_facet Space and Planetary Science
Geophysics
description Abstract– Donald D. Bogard (Don, Fig. 1 ) became interested in meteorites after seeing the Fayetteville meteorite in an undergraduate astronomy class at the University of Arkansas. During his graduate studies with Paul Kuroda at Arkansas, Don helped discover the Xe decay products of 244 Pu. After a postdoctoral period at Caltech, where he learned much from Jerry Wasserburg, Peter Eberhardt, Don Burnett, and Sam Epstein, Don became one of a number of young Ph.D. scientists hired by NASA’s Manned Spacecraft Center to set up the Lunar Receiving Laboratory (LRL) and to perform a preliminary examination of Apollo samples. In collaboration with Oliver Schaeffer (SUNY), Joseph Zähringer (Max Planck, Heidelberg), and Raymond Davis (Brookhaven National Laboratory), he built a gas analysis laboratory at JSC, and the noble gas portion of this laboratory remained operational until he retired in 2010. At NASA, Don worked on the lunar regolith, performed pioneering work on cosmic ray produced noble gas isotopes and Ar‐Ar dating, the latter for important insights into the thermal and shock history of meteorites and lunar samples. During this work, he discovered that the trapped gases in SNC meteorites were very similar to those of the Martian atmosphere and thus established their Martian origin. Among Don’s many administrative accomplishments are helping to establish the Antarctic meteorite and cosmic dust processing programs at JSC and serving as a NASA‐HQ discipline scientist, where he advanced peer review and helped create new programs. Don is a recipient of NASA’s Scientific Achievement and Exceptional Service Medals and the Meteoritical Society’s Leonard Medal. Donald Bogard. image
format Article in Journal/Newspaper
author SEARS, Derek W. G.
author_facet SEARS, Derek W. G.
author_sort SEARS, Derek W. G.
title Oral histories in meteoritics and planetary science —XVI: Donald D. Bogard
title_short Oral histories in meteoritics and planetary science —XVI: Donald D. Bogard
title_full Oral histories in meteoritics and planetary science —XVI: Donald D. Bogard
title_fullStr Oral histories in meteoritics and planetary science —XVI: Donald D. Bogard
title_full_unstemmed Oral histories in meteoritics and planetary science —XVI: Donald D. Bogard
title_sort oral histories in meteoritics and planetary science —xvi: donald d. bogard
publisher Wiley
publishDate 2012
url http://dx.doi.org/10.1111/j.1945-5100.2012.01333.x
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https://onlinelibrary.wiley.com/doi/pdf/10.1111/j.1945-5100.2012.01333.x
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op_source Meteoritics & Planetary Science
volume 47, issue 3, page 416-433
ISSN 1086-9379 1945-5100
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op_doi https://doi.org/10.1111/j.1945-5100.2012.01333.x
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