The origins and concentrations of water, carbon, nitrogen and noble gases on Earth
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Low N/C in today's mid-ocean ridge source basalts suggests considerable N2 degassing once the upper mantle became oxidized.
“However, low N/C in today’s mid-ocean ridge source basalts (144) suggests considerable N2 degassing once the upper mantle became oxidized because then nitrogen became insoluble in magmas and upper mantle fluids (145).”
From The Archean atmosphere (2020) · cites this paper as [144]
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Background67P/Churyumov-Gerasimenko, a Jupiter family comet with a high D/H ratio
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Cometary Isotopic Measurements
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Self-citationAtmospheric Escape Processes and Planetary Atmospheric Evolution
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Early accretion of water in the inner solar system from a carbonaceous chondrite–like source
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Noble gas constraints on the origin and evolution of Earth’s volatiles
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A hydrogen-based oxidation mechanism relevant to planetary formation
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Nitrogen solubility in molten metal and silicate at high pressure and temperature
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Evolution of atmospheric xenon and other noble gases inferred from Archean to Paleoproterozoic rocks
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Terrestrial planet formation from lost inner solar system material
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Lunar and terrestrial planet formation in the Grand Tack scenario
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Delivery of carbon, nitrogen, and sulfur to the silicate Earth by a giant impact
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Volcanic, Magmatic and Hydrothermal Gases
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The aqueous alteration of CM chondrites, a review
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Ruthenium isotope vestige of Earth’s pre-late-veneer mantle preserved in Archaean rocks
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The redox geodynamics linking basalts and their mantle sources through space and time
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Asteroidal impacts and the origin of terrestrial and lunar volatiles
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The partitioning of the inner and outer Solar System by a structured protoplanetary disk
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Nitrogen solubility in upper mantle minerals
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Carbon in the Core: Its Influence on the Properties of Core and Mantle
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Habitability of Exoplanet Waterworlds
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Super-Earth masses sculpted by pebble isolation around stars of different masses
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The Delivery of Water During Terrestrial Planet Formation
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VOLATILE DELIVERY TO PLANETS FROM WATER-RICH PLANETESIMALS AROUND LOW-MASS STARS
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TWO BEYOND-PRIMITIVE EXTRASOLAR PLANETESIMALS
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The elemental abundances (with uncertainties) of the most Earth-like planet
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Hydration and Dehydration in Earth's Interior
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An asteroidal origin for water in the Moon
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- Authors
- Marty, B.
- Affiliations
- Centre National de la Recherche Scientifique (FR)
- Corresponding author
- Marty, Bernard
- ORCID
- Marty, Bernard
- Venue
- Earth and Planetary Science Letters
- Publisher
- Elsevier BV
- Published
- 2012-01
- Volume
- 313-314
- Pages
- 56-66
- ISSN
- 0012-821X (ISSN-L)
- OpenAlex
- W2095245998
- Cited by
- 1,012
- References
- 158
- Citations by year
- 2026: 50 · 2025: 71 · 2024: 87 · 2023: 70 · 2022: 81 · 2021: 79 · 2020: 90 · 2019: 70 · 2018: 93 · 2017: 75 · 2016: 62 · 2015: 69 · 2014: 48 · 2013: 39 · 2012: 23
- FWCI
- 19.04
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Earth and Planetary Science Letters (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- HAL (submittedVersion, other-oa)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Physical Sciences › Earth and Planetary Sciences › Geophysics › Geological and Geochemical Analysis
- Physical Sciences › Earth and Planetary Sciences › Paleontology › Paleontology and Stratigraphy of Fossils
- Keywords
- water, carbon, nitrogen, noble gases, hydrogen isotopes, nitrogen isotopes, noble gas isotopes, primitive meteorites, cometary volatiles, radiogenic argon, carbonaceous chondrites, Earth accretion
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