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Widespread production of silica- and alkali-rich melts at the onset of planetesimal melting

Collinet, Max and Grove, Timothy (2020) Widespread production of silica- and alkali-rich melts at the onset of planetesimal melting. Geochimica et Cosmochimica Acta, 277 (15), pp. 334-357. Elsevier. doi: 10.1016/j.gca.2020.03.005. ISSN 0016-7037.

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Official URL: https://www.sciencedirect.com/science/article/abs/pii/S0016703720301666

Abstract

We present the results of melting experiments on a suite of carbonaceous and ordinary chondritic compositions (CV, CM, CI, H and LL) performed at low pressure (0.1–13.1 MPa) and over a range of oxygen fugacity (log fO2 − (log fO2)IW = −2.5 to −1 and +0.8, IW being the iron-wustite buffer). These experiments constrain the composition of partial melts (F = 5–25 wt.%) of chondritic planetesimals. Most experiments (IW −2.5 to −1) were conducted in Molybdenum-Hafnium Carbide pressure vessels, which prevented the loss of alkali elements from the melt. The results show that all planetesimals not significantly depleted in moderately volatile elements relative to the sun’s photosphere (e.g. CI, H and LL compositions) produced low-degree melts (<15 wt.%) rich in SiO2, Al2O3 and alkali elements, regardless of the fO2. Despite their high apparent viscosities (104-5 Pa.s), such low-density partial melts (2400–2500 kg/m3) were mobilized and, upon crystallizing, formed rocks containing up to 80 vol.% of plagioclase An10-30 (i.e. oligoclase) such as the trachyandesite achondrites Graves Nunataks 06128/9, Northwest Africa 6698 and 11575, the Almahata Sitta clast ALM-A, as well as smaller “albitic clasts” in polymict ureilites and “alkali-silica-rich” inclusions in non-magmatic iron meteorites. We suggest that silica- and alkali- rich melts were widespread in small bodies of the early solar system but that much evidence was erased by subsequent stages of melting and planetary accretion and differentiation.

Item URL in elib:https://elib.dlr.de/137522/
Document Type:Article
Title:Widespread production of silica- and alkali-rich melts at the onset of planetesimal melting
Authors:
AuthorsInstitution or Email of AuthorsAuthor's ORCID iD
Collinet, Maxmax.collinet (at) dlr.dehttps://orcid.org/0000-0002-8791-9751
Grove, TimothyDept. of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambrige, USAUNSPECIFIED
Date:2020
Journal or Publication Title:Geochimica et Cosmochimica Acta
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In SCOPUS:Yes
In ISI Web of Science:Yes
Volume:277
DOI :10.1016/j.gca.2020.03.005
Page Range:pp. 334-357
Publisher:Elsevier
ISSN:0016-7037
Status:Published
Keywords:primitive melts, melt migration, asteroids, planetary accretion, planetary differentiation, differentiated meteorites, primordial crust, primary crust
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, R - Vorhaben Planetary Evolution and Life (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Physics
Deposited By: Plesa, Dr. Ana-Catalina
Deposited On:17 Nov 2020 09:57
Last Modified:17 Nov 2020 09:57

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