Planetesimal Impact Vapor Plumes and Nebular Shocks Form Chondritic Mixtures
The origin of chondrules and the chondritic sedimentary rocks that dominate the meteoritic record is a long-standing problem in planetary science. Here, we develop a physical model for the formation of chondritic mixtures as an outcome of vaporizing collisions between planetesimals that were dynamic...
Saved in:
| Main Authors: | Sarah T. Stewart, Simon J. Lock, Philip J. Carter, Erik J. Davies, Michail I. Petaev, Stein B. Jacobsen |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Planetary Science Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/PSJ/adbe71 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Hydrous Chondrites under Shock
by: Adrien Saurety, et al.
Published: (2025-01-01) -
A Long‐Lived Planetesimal Dynamo Powered by Core Crystallization
by: Clara Maurel, et al.
Published: (2021-03-01) -
Micromagnetic and microstructural analyses in chondrules of the Allende meteorite
by: Daniel Flores-Gutiérrez, et al.
Published: (2018-02-01) -
Development of a technique to identify μm-sized organic matter in asteroidal material: An approach using machine learning
by: Rahul Kumar, et al.
Published: (2025-09-01) -
Deep Mantle–Atmosphere Coupling and Carbonaceous Bombardment: Options for Biomolecule Formation on an Oxidized Early Earth
by: Klaus Paschek, et al.
Published: (2025-01-01)