Decoupling of high-pressure H2 production from serpentinization and magnetite in subduction zones
Siron G+4 more
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Lithological discrimination based on Landsat-9 OLI sensor and field observation data: The bana an-orogenic volcano-plutonic ring complex, West Cameroon line. [PDF]
Mohamed R+4 more
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Laboratory spectra of amorphous and crystalline olivine: An application to comet Halley IR spectrum
A Blanco+5 more
openalex
Does the direct effect of friction increase continuously with absolute temperature? [PDF]
Barbot S.
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Slab melting boosts the mantle wedge contribution to Li-rich magmas. [PDF]
Schettino E+9 more
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Olivine alteration and the loss of Mars' early atmospheric carbon. [PDF]
Murray J, Jagoutz O.
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A closer look into the structure and magnetism of the recently fallen meteorite Ribbeck. [PDF]
Kołodziej M+5 more
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Fundamental constraints and questions from the study of martian meteorites and the need for returned samples. [PDF]
Udry A, Ostwald AM, Day JMD, Hallis LJ.
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Dense hydrated Mg-silicates in diamond: Implications for transport of H2O into the mantle. [PDF]
Carvalho LDV+10 more
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AbstractOlivine‐phyric shergottites represent primitive Martian magmas, but they commonly contain excess olivine and rarely represent primary mantle melts. Olivine chemistry, however, tracks magma evolution and preserves information on the original parent magma composition.
Sierra Ramsey+7 more
openaire +2 more sources