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Title: A Low Viscosity Lunar Magma Ocean Forms a Stratified Anorthitic Flotation Crust With Mafic Poor and Rich Units

Journal Article · · Geophysical Research Letters
DOI:https://doi.org/10.1002/2017GL075703· OSTI ID:1418040

Much of the lunar crust is monomineralic, comprising >98% plagioclase. The prevailing model argues the crust accumulated as plagioclase floated to the surface of a solidifying lunar magma ocean (LMO). Whether >98% pure anorthosites can form in a flotation scenario is debated. An important determinant of the efficiency of plagioclase fractionation is the viscosity of the LMO liquid, which was unconstrained. Here we present results from new experiments conducted on a late LMO-relevant ferrobasaltic melt. The liquid has an exceptionally low viscosity of 0.22 $$+0.11\atop{-0.19}$$to 1.45 $$+0.46\atop{-0.82}$$ Pa s at experimental conditions (1,300–1,600°C; 0.1–4.4 GPa) and can be modeled by an Arrhenius relation. Extrapolating to LMO-relevant temperatures, our analysis suggests a low viscosity LMO would form a stratified flotation crust, with the oldest units containing a mafic component and with very pure younger units. Old, impure crust may have been buried by lower crustal diapirs of pure anorthosite in a serial magmatism scenario.

Research Organization:
Argonne National Lab. (ANL), Argonne, IL (United States). Advanced Photon Source (APS)
Sponsoring Organization:
USDOE Office of Science (SC), Basic Energy Sciences (BES); National Aeronautics and Space Administration (NASA)
Grant/Contract Number:
AC02- 06CH11357
OSTI ID:
1418040
Journal Information:
Geophysical Research Letters, Vol. 44, Issue 22; ISSN 0094-8276
Publisher:
American Geophysical UnionCopyright Statement
Country of Publication:
United States
Language:
ENGLISH
Citation Metrics:
Cited by: 21 works
Citation information provided by
Web of Science

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  • Carlson, Richard W.; Borg, Lars E.; Gaffney, Amy M.
  • Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 372, Issue 2024 https://doi.org/10.1098/rsta.2013.0246
journal September 2014

Cited By (1)

Magma oceans as a critical stage in the tectonic development of rocky planets
  • Schaefer, Laura; Elkins-Tanton, Linda T.
  • Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 376, Issue 2132 https://doi.org/10.1098/rsta.2018.0109
journal October 2018

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