Manuel Moreira
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Previous Organizations / Institutes
The organizations / institutes from the scholar's other articles in the past ten years
Research Subjects
Research Interests
Manuel Moreira has a total of 10 co-authors. Here are the top co-authors by number of shared publications:
Claude Allègre
Université Denis Diderot-Paris 7, Laboratoire de Géochimie et Cosmochimie, Institut de Physique du Globe de Paris, CNRS Unité de Recherche Associée Number 1758, 4 Place Jussieu, 75252 Paris Cedex 05, France
1 shared publicationClaude J. Allègre
1 shared publicationClaude-Jean Allègre
Laboratoire de Géochimie et Cosmochimie, Institut de Physique du Globe et Université Paris 7-Denis Diderot, CNRS, 4 place Jussieu, 75252 Paris Cedex 05, France
1 shared publication- Cécile Gautheron
Université Paris-Saclay, CNRS, GEOPS, Orsay, France
1 shared publication Hélène Ondréas
Ifremer Plouzané France
1 shared publicationJeff W. Harris
1 shared publication
Latest Publications
- 24 May 2008
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 35 (10)
Helium isotopes on the Pacific‐Antarctic ridge (52.5°–41.5°S)
The first isotopic data and concentrations of helium are reported for the Pacific‐Antarctic ridge between 52.5°S and 41.5°S. The 4He/3He ratio is extremely homogeneous over more than 1200 km, with a mean ratio of 99,275 (R/Ra = 7.29) and a standard deviation of 2719 (0.19), which is the lowest dispersion observed for the global mid oceanic ridge system. Moreover, the Menard T.F. is a frontier between two mantles with slightly different helium isotopic ratios (96,595 ± 1520 and 100,347 ± 2330). No difference in the helium concentration between the two ridge segments defined by the Menard T.F. can be observed, as well as no significant difference in the U and Th contents suggesting that the difference in helium isotopic ratio is old (>500 My) and may represent a slight difference in degassing or/and trace element depletion history.
- 24 May 2008
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 35 (10)
Helium isotopes on the Pacific‐Antarctic ridge (52.5°–41.5°S)
The first isotopic data and concentrations of helium are reported for the Pacific‐Antarctic ridge between 52.5°S and 41.5°S. The 4He/3He ratio is extremely homogeneous over more than 1200 km, with a mean ratio of 99,275 (R/Ra = 7.29) and a standard deviation of 2719 (0.19), which is the lowest dispersion observed for the global mid oceanic ridge system. Moreover, the Menard T.F. is a frontier between two mantles with slightly different helium isotopic ratios (96,595 ± 1520 and 100,347 ± 2330). No difference in the helium concentration between the two ridge segments defined by the Menard T.F. can be observed, as well as no significant difference in the U and Th contents suggesting that the difference in helium isotopic ratio is old (>500 My) and may represent a slight difference in degassing or/and trace element depletion history.
- 15 December 2007
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 264 (1-2) , 114-122
Constraints on the origin of the 129Xe on Earth using the tellurium double beta decay
- 15 December 2007
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 264 (1-2) , 114-122
Constraints on the origin of the 129Xe on Earth using the tellurium double beta decay
- 30 November 2006
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 252 (1-2) , 220-222
Reply to: “Recycled” volatiles in mantle derived diamonds—Evidence from nitrogen and noble gas isotopic data
- 30 November 2006
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 252 (1-2) , 220-222
Reply to: “Recycled” volatiles in mantle derived diamonds—Evidence from nitrogen and noble gas isotopic data
- 18 August 2005
- Published by American Geophysical Union (AGU) in Geochemistry, Geophysics, Geosystems
- Vol. 6 (8)
Cosmogenic helium and neon in 11 Myr old ultramafic xenoliths: Consequences for mantle signatures in old samples
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 4He 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 (20Ne/22Ne down to 7.7 and 21Ne/22Ne > 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 4He/3He ratio as low as 42 ± 8 (R/Ra = 17,300) and 21Ne/22Ne 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 3He.
- 18 August 2005
- Published by American Geophysical Union (AGU) in Geochemistry, Geophysics, Geosystems
- Vol. 6 (8)
Cosmogenic helium and neon in 11 Myr old ultramafic xenoliths: Consequences for mantle signatures in old samples
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 4He 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 (20Ne/22Ne down to 7.7 and 21Ne/22Ne > 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 4He/3He ratio as low as 42 ± 8 (R/Ra = 17,300) and 21Ne/22Ne 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 3He.
- 15 May 2002
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 198 (3-4) , 401-416
Rare gas systematics on Mid Atlantic Ridge (37–40°N)
- 15 May 2002
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 198 (3-4) , 401-416
Rare gas systematics on Mid Atlantic Ridge (37–40°N)
- 20 February 1998
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 279 (5354) , 1178-1181
Rare Gas Systematics in Popping Rock: Isotopic and Elemental Compositions in the Upper Mantle
New experimental data on the isotopic variations of neon, argon, and xenon in a popping rock imply that the 40 Ar/ 36 Ar ratio of the upper mantle is less than 44,000 and that the 129 Xe/ 130 Xe ratio is less than 8.2. The elemental abundance pattern of rare gases is chondritic-like and is quite distinct from the solar pattern. These data imply that Earth accreted from planetesimals that probably underwent a transformation of their rare gas budget from solar- to chondritic-like, leaving the isotopic composition unchanged from the solar pattern.
- 20 February 1998
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 279 (5354) , 1178-1181
Rare Gas Systematics in Popping Rock: Isotopic and Elemental Compositions in the Upper Mantle
New experimental data on the isotopic variations of neon, argon, and xenon in a popping rock imply that the 40 Ar/ 36 Ar ratio of the upper mantle is less than 44,000 and that the 129 Xe/ 130 Xe ratio is less than 8.2. The elemental abundance pattern of rare gases is chondritic-like and is quite distinct from the solar pattern. These data imply that Earth accreted from planetesimals that probably underwent a transformation of their rare gas budget from solar- to chondritic-like, leaving the isotopic composition unchanged from the solar pattern.