Episodic formation of refractory inclusions in the Solar System and their presolar heritage.

26Al Mg isotope Solar System formation episodic outburst presolar dust refractory inclusion

Journal

Earth and planetary science letters
ISSN: 0012-821X
Titre abrégé: Earth Planet Sci Lett
Pays: Netherlands
ID NLM: 100971345

Informations de publication

Date de publication:
01 Apr 2020
Historique:
entrez: 2 8 2021
pubmed: 28 1 2020
medline: 28 1 2020
Statut: epublish

Résumé

Refractory inclusions [Ca-Al-rich Inclusions (CAIs) and Amoeboid Olivine Aggregates (AOAs)] in primitive meteorites are the oldest Solar System solids. They formed in the hot inner protoplanetary disk and, as such, provide insights into the earliest disk dynamics and physicochemical processing of the dust and gas that accreted to form the Sun and its planetary system. Using the short-lived

Identifiants

pubmed: 34334802
doi: 10.1016/j.epsl.2020.116088
pmc: PMC7611424
mid: EMS96519
doi:

Types de publication

Journal Article

Langues

eng

Pagination

116088

Subventions

Organisme : European Research Council
ID : 833275
Pays : International

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Auteurs

K K Larsen (KK)

Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, Copenhagen DK-1350, Denmark.

D Wielandta (D)

Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, Copenhagen DK-1350, Denmark.

M Schillera (M)

Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, Copenhagen DK-1350, Denmark.

A N Krot (AN)

Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, Copenhagen DK-1350, Denmark.
Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Manoa, HI 96822, USA.

M Bizzarro (M)

Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, Copenhagen DK-1350, Denmark.

Classifications MeSH