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...

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Bibliographic Details
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
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Online Access:https://doi.org/10.3847/PSJ/adbe71
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