Cosmogenic helium and neon in 11 Myr old ultramafic xenoliths: Consequences for mantle signatures in old samples
International audience The helium and neon isotopic compositions of olivines coming from a 11 Myr old xenolith sampled at Mt. Hampton (West Antarctica) were analyzed by crushing. The helium isotopic ratio varies between 1340 and 6300 (R/Ra between 115 and 539) with 4 He content around 3-8 10 -10 ccS...
Published in: | Geochemistry, Geophysics, Geosystems |
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Online Access: | https://insu.hal.science/insu-03601115 https://insu.hal.science/insu-03601115/document https://insu.hal.science/insu-03601115/file/Geochem%20Geophys%20Geosyst%20-%202005%20-%20Moreira%20-%20Cosmogenic%20helium%20and%20neon%20in%2011%20Myr%20old%20ultramafic%20xenoliths%20Consequences%20for.pdf https://doi.org/10.1029/2005GC000939 |
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ftsorbonneuniv:oai:HAL:insu-03601115v1 2024-09-09T19:10:12+00:00 Cosmogenic helium and neon in 11 Myr old ultramafic xenoliths: Consequences for mantle signatures in old samples Moreira, Manuel Madureira, Pedro Institut de Physique du Globe de Paris (IPGP) Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS) 2005 https://insu.hal.science/insu-03601115 https://insu.hal.science/insu-03601115/document https://insu.hal.science/insu-03601115/file/Geochem%20Geophys%20Geosyst%20-%202005%20-%20Moreira%20-%20Cosmogenic%20helium%20and%20neon%20in%2011%20Myr%20old%20ultramafic%20xenoliths%20Consequences%20for.pdf https://doi.org/10.1029/2005GC000939 en eng HAL CCSD AGU and the Geochemical Society info:eu-repo/semantics/altIdentifier/doi/10.1029/2005GC000939 insu-03601115 https://insu.hal.science/insu-03601115 https://insu.hal.science/insu-03601115/document https://insu.hal.science/insu-03601115/file/Geochem%20Geophys%20Geosyst%20-%202005%20-%20Moreira%20-%20Cosmogenic%20helium%20and%20neon%20in%2011%20Myr%20old%20ultramafic%20xenoliths%20Consequences%20for.pdf BIBCODE: 2005GGG.6.8006M doi:10.1029/2005GC000939 http://hal.archives-ouvertes.fr/licences/copyright/ info:eu-repo/semantics/OpenAccess EISSN: 1525-2027 Geochemistry, Geophysics, Geosystems https://insu.hal.science/insu-03601115 Geochemistry, Geophysics, Geosystems, 2005, 6, pp. 337-338. ⟨10.1029/2005GC000939⟩ cosmogenic crushing helium mantle neon [SDU]Sciences of the Universe [physics] info:eu-repo/semantics/article Journal articles 2005 ftsorbonneuniv https://doi.org/10.1029/2005GC000939 2024-07-25T23:47:51Z International audience The helium and neon isotopic compositions of olivines coming from a 11 Myr old xenolith sampled at Mt. Hampton (West Antarctica) were analyzed by crushing. The helium isotopic ratio varies between 1340 and 6300 (R/Ra between 115 and 539) with 4 He content around 3-8 10 -10 ccSTP/g, confirming that cosmogenic helium can be extracted by crushing. The neon also shows a clear cosmogenic origin ( 20 Ne/ 22 Ne down to 7.7 and 21 Ne/ 22 Ne > 0.32), indicating that the cosmogenic neon can also be extracted by crushing out of the olivines. Melting of the powder left after the crushing experiment gives a 4 He/ 3 He ratio as low as 42 ± 8 (R/Ra = 17,300) and 21 Ne/ 22 Ne as high as 0.78, close to the cosmogenic production end-member. This study shows that up to ∼0.5% of cosmogenic helium and neon can be extracted by crushing. In this way, for samples that had been exposed to cosmic rays for a long time (e.g., a few Myr), a crushing procedure may not give the mantle ratios without ambiguity, and measurement of neon can help to discriminate between cosmogenic and mantle origin of the 3 He. Article in Journal/Newspaper Antarc* Antarctica West Antarctica HAL Sorbonne Université Hampton ENVELOPE(-70.100,-70.100,-69.333,-69.333) West Antarctica Geochemistry, Geophysics, Geosystems 6 8 n/a n/a |
institution |
Open Polar |
collection |
HAL Sorbonne Université |
op_collection_id |
ftsorbonneuniv |
language |
English |
topic |
cosmogenic crushing helium mantle neon [SDU]Sciences of the Universe [physics] |
spellingShingle |
cosmogenic crushing helium mantle neon [SDU]Sciences of the Universe [physics] Moreira, Manuel Madureira, Pedro Cosmogenic helium and neon in 11 Myr old ultramafic xenoliths: Consequences for mantle signatures in old samples |
topic_facet |
cosmogenic crushing helium mantle neon [SDU]Sciences of the Universe [physics] |
description |
International audience The helium and neon isotopic compositions of olivines coming from a 11 Myr old xenolith sampled at Mt. Hampton (West Antarctica) were analyzed by crushing. The helium isotopic ratio varies between 1340 and 6300 (R/Ra between 115 and 539) with 4 He content around 3-8 10 -10 ccSTP/g, confirming that cosmogenic helium can be extracted by crushing. The neon also shows a clear cosmogenic origin ( 20 Ne/ 22 Ne down to 7.7 and 21 Ne/ 22 Ne > 0.32), indicating that the cosmogenic neon can also be extracted by crushing out of the olivines. Melting of the powder left after the crushing experiment gives a 4 He/ 3 He ratio as low as 42 ± 8 (R/Ra = 17,300) and 21 Ne/ 22 Ne as high as 0.78, close to the cosmogenic production end-member. This study shows that up to ∼0.5% of cosmogenic helium and neon can be extracted by crushing. In this way, for samples that had been exposed to cosmic rays for a long time (e.g., a few Myr), a crushing procedure may not give the mantle ratios without ambiguity, and measurement of neon can help to discriminate between cosmogenic and mantle origin of the 3 He. |
author2 |
Institut de Physique du Globe de Paris (IPGP) Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS) |
format |
Article in Journal/Newspaper |
author |
Moreira, Manuel Madureira, Pedro |
author_facet |
Moreira, Manuel Madureira, Pedro |
author_sort |
Moreira, Manuel |
title |
Cosmogenic helium and neon in 11 Myr old ultramafic xenoliths: Consequences for mantle signatures in old samples |
title_short |
Cosmogenic helium and neon in 11 Myr old ultramafic xenoliths: Consequences for mantle signatures in old samples |
title_full |
Cosmogenic helium and neon in 11 Myr old ultramafic xenoliths: Consequences for mantle signatures in old samples |
title_fullStr |
Cosmogenic helium and neon in 11 Myr old ultramafic xenoliths: Consequences for mantle signatures in old samples |
title_full_unstemmed |
Cosmogenic helium and neon in 11 Myr old ultramafic xenoliths: Consequences for mantle signatures in old samples |
title_sort |
cosmogenic helium and neon in 11 myr old ultramafic xenoliths: consequences for mantle signatures in old samples |
publisher |
HAL CCSD |
publishDate |
2005 |
url |
https://insu.hal.science/insu-03601115 https://insu.hal.science/insu-03601115/document https://insu.hal.science/insu-03601115/file/Geochem%20Geophys%20Geosyst%20-%202005%20-%20Moreira%20-%20Cosmogenic%20helium%20and%20neon%20in%2011%20Myr%20old%20ultramafic%20xenoliths%20Consequences%20for.pdf https://doi.org/10.1029/2005GC000939 |
long_lat |
ENVELOPE(-70.100,-70.100,-69.333,-69.333) |
geographic |
Hampton West Antarctica |
geographic_facet |
Hampton West Antarctica |
genre |
Antarc* Antarctica West Antarctica |
genre_facet |
Antarc* Antarctica West Antarctica |
op_source |
EISSN: 1525-2027 Geochemistry, Geophysics, Geosystems https://insu.hal.science/insu-03601115 Geochemistry, Geophysics, Geosystems, 2005, 6, pp. 337-338. ⟨10.1029/2005GC000939⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1029/2005GC000939 insu-03601115 https://insu.hal.science/insu-03601115 https://insu.hal.science/insu-03601115/document https://insu.hal.science/insu-03601115/file/Geochem%20Geophys%20Geosyst%20-%202005%20-%20Moreira%20-%20Cosmogenic%20helium%20and%20neon%20in%2011%20Myr%20old%20ultramafic%20xenoliths%20Consequences%20for.pdf BIBCODE: 2005GGG.6.8006M doi:10.1029/2005GC000939 |
op_rights |
http://hal.archives-ouvertes.fr/licences/copyright/ info:eu-repo/semantics/OpenAccess |
op_doi |
https://doi.org/10.1029/2005GC000939 |
container_title |
Geochemistry, Geophysics, Geosystems |
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6 |
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8 |
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1809824808434663424 |