Results 261 to 270 of about 76,410 (310)

Author Correction: Lunar primitive mantle olivine returned by Chang'e-6. [PDF]

open access: yesNat Commun
Sheng SZ   +10 more
europepmc   +1 more source

Water abundance in the lunar farside mantle. [PDF]

open access: yesNature
He H   +12 more
europepmc   +1 more source

Microbial Community Structure in Contrasting Hawaiian Coastal Sediments. [PDF]

open access: yesMicrob Ecol
Van Heurck B   +8 more
europepmc   +1 more source

Erratic behavior of platinum-group elements along an olivine-Cr-spinel cotectic in sulfide-undersaturated basaltic magma: roles of Cr-spinel and alloys. [PDF]

open access: yesSci Rep
Chayka IF   +14 more
europepmc   +1 more source

A potential mantle origin for precursor rocks of high-Mg impact glass beads in Chang'e-5 soil. [PDF]

open access: yesSci Adv
Ding CL   +10 more
europepmc   +1 more source
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Olivines and olivine coronas in mesosiderites

Geochimica et Cosmochimica Acta, 1980
The paper presents a study of olivines and their surrounding coronas in mesosiderites texturally and compositionally using optical and microprobe methods. Olivine composition ranges from Fo(58-92) and shows no consistent pattern of distribution within and between mesosiderites; olivine occurs as large single crystals or as partially recrystallized ...
C.E. Nehru   +3 more
openaire   +1 more source

Sintering of olivine and olivine-basalt aggregates

Physics and Chemistry of Minerals, 1984
The sintering behavior of olivine and olivine-basalt aggregates has been examined at temperatures near 1,300° C. Experimental factors contributing to rapid sintering kinetics and high-density, fine-grained specimens include: (i) the uniform dispersion of basalt throughout the specimen, (ii) a very fine, uniform particle size for the olivine powder ...
R. F. Cooper, D. L. Kohlstedt
openaire   +1 more source

Nickel–manganese variability in olivine and Al‐in‐olivine thermometry for olivine‐phyric shergottites

Meteoritics & Planetary Science, 2021
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 R. Ramsey   +3 more
openaire   +1 more source

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