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The Diversity of Igneous Processes in Planetesimals and Implications for the Distribution of Alkali Elements in the Early Solar System

Collinet, Max (2022) The Diversity of Igneous Processes in Planetesimals and Implications for the Distribution of Alkali Elements in the Early Solar System. LPI Seminar Series, 2022-05-12, Online.

Full text not available from this repository.

Abstract

chondrite meteorites are highly variable in composition: some are ultramafic (primitive achondrites), basaltic (e.g., eucrites and angrites), or (trachy-) andesitic (e.g., GRA 06128, NWA 11119 and Erg Chech 002). These different groups correspond to the mantle and crust of planetary building blocks, respectively. They represent a unique opportunity to constrain the early melting processes that affected planetesimals and could have influenced the final composition of planets.

Item URL in elib:https://elib.dlr.de/186759/
Document Type:Conference or Workshop Item (Speech)
Title:The Diversity of Igneous Processes in Planetesimals and Implications for the Distribution of Alkali Elements in the Early Solar System
Authors:
AuthorsInstitution or Email of AuthorsAuthor's ORCID iDORCID Put Code
Collinet, Maxmax.collinet (at) dlr.dehttps://orcid.org/0000-0002-8791-9751UNSPECIFIED
Date:12 May 2022
Refereed publication:No
Open Access:No
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:No
Status:Published
Keywords:Planetary differentiation, accretion, solar nebula
Event Title:LPI Seminar Series
Event Location:Online
Event Type:Other
Event Date:12 May 2022
Organizer:Lunar and Planetary Institute
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space Exploration
DLR - Research area:Raumfahrt
DLR - Program:R EW - Space Exploration
DLR - Research theme (Project):R - Exploration of the Solar System
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Physics
Deposited By: Collinet, Max
Deposited On:20 Jun 2022 14:10
Last Modified:24 Apr 2024 20:48

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