Model calculations for neutron-induced reactions in meteorites and planetary surfaces. [PDF]
Leya I.
europepmc +1 more source
Recent progress and future prospects of the early solar system chronology. [PDF]
Amelin Y, Yin QZ.
europepmc +1 more source
<i>In situ</i> analysis of titanium isotope ratios in stardust using LA-CC-MC-ICPMS/MS. [PDF]
Shaw KMM +6 more
europepmc +1 more source
Physicochemical Controls on the Compositions of the Earth and Planets. [PDF]
Sossi PA +4 more
europepmc +1 more source
Integrated geological datasets for the Zandrivierspoort Formation banded iron formation, Rhenosterkoppies Greenstone Belt, South Africa. [PDF]
Tibane LV, Mamba D, Nkosi ZH.
europepmc +1 more source
Taphonomic bias of hydrothermal silicification in biodiversity patterns of Cambrian shelly pavements from the Iberian Chains, NE Spain. [PDF]
Martínez-Benítez B +2 more
europepmc +1 more source
The Yamato-type (CY) carbonaceous chondrite group: Analogues for the surface of asteroid Ryugu?
We report new mineralogical, petrographic and noble gas analyses of the carbonaceous chondrite meteorites Y-82162 (C1/2ung), Y-980115 (CI1), Y-86029 (CI1), Y-86720 (C2ung), Y-86789 (C2ung), and B-7904 (C2ung).
Ashley J KING +2 more
exaly +2 more sources
CV and CM chondrite impact melts
Nicole G Lunning +2 more
exaly +2 more sources
Pore size distribution in an uncompacted equilibrated ordinary chondrite
The extraordinarily uncompacted nature of the ordinary L chondrite fall Baszkowka gives a unique opportunity to investigate the potentially pre-compaction pore size distribution in an equilibrated ordinary chondrite.
Jon M Friedrich +2 more
exaly +3 more sources
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The Bencubbin chondrite breccia and its relationship to CR chondrites and the ALH85085 chondrite
Meteoritics, 1990Abstract— Bencubbin is an unclassified meteorite breccia which consists mainly of host silicate (∼40 vol.%) and host metal (∼60%) components. Rare (< 1%) ordinary chondrite clasts and a dark xenolith (formerly called a carbonaceous chondrite clast) are also found.
Michael K. Weisberg +2 more
openaire +1 more source

