Chondrule Destruction via Dust Collisions in Shock Waves
Y Matsumoto, K Kurosawa… - The Astrophysical …, 2024 - iopscience.iop.org
A leading candidate for the heating source of chondrules and igneous rims is shock waves.
This mechanism generates high relative velocities between chondrules and dust particles …
This mechanism generates high relative velocities between chondrules and dust particles …
Fine-grained rim formation via kinetic dust aggregation in shock waves around evaporating icy planetesimals
S Arakawa, H Kaneko, T Nakamoto - The Astrophysical Journal, 2022 - iopscience.iop.org
Fine-grained rims (FGRs) are frequently found around chondrules in primitive chondrites.
The remarkable feature of FGRs is their submicron-sized and nonporous nature. The typical …
The remarkable feature of FGRs is their submicron-sized and nonporous nature. The typical …
The Aguas Zarcas carbonaceous chondrite meteorite: Brecciation and aqueous alteration on the parent body
I Kouvatsis, JA Cartwright… - Meteoritics & Planetary …, 2024 - Wiley Online Library
CM chondrites are samples from primitive water‐rich asteroids that formed early in the solar
system; many record evidence for silicate rock–liquid water interaction. Many CM chondrites …
system; many record evidence for silicate rock–liquid water interaction. Many CM chondrites …
Modeling Chondrule Dust Rim Growth with Ellipsoidal Monomers
C Xiang, A Carballido, LS Matthews… - The Astrophysical …, 2023 - iopscience.iop.org
Fine-grained dust rims (FGRs) surrounding chondrules in carbonaceous chondrites encode
important information about early processes in the solar nebula. Here, we investigate the …
important information about early processes in the solar nebula. Here, we investigate the …