Bright carbonate veins on asteroid (101955) Bennu: Implications for aqueous alteration history
INTRODUCTION Carbonaceous asteroids formed early in Solar System history and
experienced varying degrees of aqueous (water-rock) and thermal alteration. Most models …
experienced varying degrees of aqueous (water-rock) and thermal alteration. Most models …
Evolution of organic matter in Orgueil, Murchison and Renazzo during parent body aqueous alteration: In situ investigations
C Le Guillou, S Bernard, AJ Brearley… - … et Cosmochimica Acta, 2014 - Elsevier
Chondrites accreted the oldest solid materials in the solar system including dust processed
in the protoplanetary disk and diverse organic compounds. After accretion, asteroidal …
in the protoplanetary disk and diverse organic compounds. After accretion, asteroidal …
The abundance and stability of “water” in type 1 and 2 carbonaceous chondrites (CI, CM and CR)
A Garenne, P Beck, G Montes-Hernandez… - … et Cosmochimica Acta, 2014 - Elsevier
Carbonaceous chondrites record processes of aqueous alteration in the presence of
hydrated and hydroxylated minerals, which could have provided a source of water in the …
hydrated and hydroxylated minerals, which could have provided a source of water in the …
Origin of hydrogen isotopic variations in chondritic water and organics
Chondrites are rocky fragments of asteroids that formed at different times and heliocentric
distances in the early solar system. Most chondrite groups contain water-bearing minerals …
distances in the early solar system. Most chondrite groups contain water-bearing minerals …
[HTML][HTML] Aragonite, breunnerite, calcite and dolomite in the CM carbonaceous chondrites: High fidelity recorders of progressive parent body aqueous alteration
Carbonate minerals in CM carbonaceous chondrite meteorites, along with the silicates and
sulphides with which they are intergrown, provide a detailed record of the nature and …
sulphides with which they are intergrown, provide a detailed record of the nature and …
[HTML][HTML] Clumped isotope and Δ17O measurements of carbonates in CM carbonaceous chondrites: New insights into parent body thermal and fluid evolution
The CM carbonaceous chondrites are key archives for understanding the earliest history of
the solar system. Their C-complex asteroid parent body (ies) underwent aqueous alteration …
the solar system. Their C-complex asteroid parent body (ies) underwent aqueous alteration …
Twinned calcite as an indicator of high differential stresses and low shock pressure conditions during impact cratering
L Seybold, CA Trepmann, S Hölzl… - … & Planetary Science, 2023 - Wiley Online Library
Shock‐related calcite twins are characterized in calcite‐bearing metagranite cataclasites
within crystalline megablocks of the Ries impact structure, Germany, as well as in cores from …
within crystalline megablocks of the Ries impact structure, Germany, as well as in cores from …
Collisional facilitation of aqueous alteration of CM and CV carbonaceous chondrites
AE Rubin - Geochimica et Cosmochimica Acta, 2012 - Elsevier
CM chondrites exhibit a strong correlation between the degree of alteration and the extent of
particle alignment (ie, the strength of the petrofabric). It seems likely that the S1 shock stage …
particle alignment (ie, the strength of the petrofabric). It seems likely that the S1 shock stage …
A Spectral Investigation of Aqueously and Thermally Altered CM, CM‐An, and CY Chondrites Under Simulated Asteroid Conditions for Comparison With OSIRIS‐REx …
HC Bates, KL Donaldson Hanna… - Journal of …, 2021 - Wiley Online Library
Volatile‐rich asteroids are crucial to understanding the transport of water and organics to the
terrestrial planet forming region in the early Solar System. Observations of two such …
terrestrial planet forming region in the early Solar System. Observations of two such …
[HTML][HTML] The paradox between low shock-stage and evidence for compaction in CM carbonaceous chondrites explained by multiple low-intensity impacts
Petrographic analysis of eight CM carbonaceous chondrites (EET 96029, LAP 031166, LON
94101, MET 01072, Murchison, Murray, SCO 06043, QUE 93005) by electron imaging and …
94101, MET 01072, Murchison, Murray, SCO 06043, QUE 93005) by electron imaging and …