Primitive meteorite groups such as the Vigarano, Mighei, and Karoonda carbonaceous chondrites have enigmatic patterns of elemental abundances, with moderately volatile elements—those that transition from vapor to condensate between ∼400 and ∼900 K ...
Jeremy W. Boyce +3 more
doaj +1 more source
Fumarolic-like activity on carbonaceous chondrite parent body. [PDF]
Ganino C, Libourel G.
europepmc +1 more source
Rare Earth Abundances in Meteoritic Chondrules [PDF]
Rare earth elements abundance in meteoritic chondrites determined by radiochemical neutron activation ...
Olehy, D. A. +2 more
core +1 more source
Insight into the evolution of the Tagish Lake carbonaceous chondrite by analysis of the oxygen isotopic composition of extracted water and Mössbauer spectroscopy [PDF]
Analysis of oxygen isotopes in water from Tagish Lake together with Mössbauer Spectroscopy suggest some similarities to the CI group of meteorites but also suggest differences in the extent of parent body hydrothermal ...
Baker, Lee +4 more
core +1 more source
The Polonnaruwa meteorite: oxygen isotope, crystalline and biological composition
Results of X-Ray Diffraction (XRD) analysis, Triple Oxygen Isotope analysis and Scanning Electron Microscopic (SEM) studies are presented for stone fragments recovered from the North Central Province of Sri Lanka following a witnessed fireball event on ...
Gibson, Carl H. +9 more
core
The evolution of organic material on Asteroid 162173 Ryugu and its delivery to Earth
The recent return of samples from asteroid 162173 Ryugu provides a first insight into early Solar System prebiotic evolution from known planetary bodies. Ryugu’s samples are CI chondrite-like, rich in water and organic material, and primarily composed of
H. G. Changela +20 more
doaj +1 more source
A primordial 15N-depleted organic component detected within the carbonaceous chondrite Maribo. [PDF]
Vollmer C +8 more
europepmc +1 more source
Al-Mg systematics of hibonite-bearing Ca,Al-rich inclusions from Ningqiang [PDF]
Hibonite-bearing Ca,Al-rich inclusions (CAIs) usually occur in CM and CH chondrites and possess petrographic and isotopic characteristics distinctive from other typical CAIs.
Guan, Yunbin, Hsu, Weibiao, Wang, Ying
core
Did the carbonaceous chondrites evolve in the crustal regions of partially differentiated asteroids? [PDF]
S. Sahijpal, Garima Gupta
openalex +1 more source
Meteoritic Evidence for a Ceres-sized Water-rich Carbonaceous Chondrite Parent Asteroid. [PDF]
Hamilton VE +5 more
europepmc +1 more source

