Formation of ferroan dacite by lunar silicic volcanism recorded in a meteorite from the Moon

Abstract An igneous clast from the Northwest Africa 773 (NWA 773) clan of lunar meteorites formed by silicic volcanism on the Moon. The clast was identified in Northwest Africa 2727 (NWA 2727), which is included in the NWA 773 clan. Over 80 mode% of the clast consists of silica + plagioclase + K-Ba-...

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Main Authors: Hiroshi Nagaoka, Timothy J. Fagan, Masahiro Kayama, Yuzuru Karouji, Nobuyuki Hasebe, Mitsuru Ebihara
Format: Article
Language:English
Published: SpringerOpen 2020-03-01
Series:Progress in Earth and Planetary Science
Subjects:
Online Access:http://link.springer.com/article/10.1186/s40645-020-0324-8
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spelling doaj-d726f5556b1b4d7fb09bc7b0a4b7a2422020-11-25T00:07:14ZengSpringerOpenProgress in Earth and Planetary Science2197-42842020-03-017111810.1186/s40645-020-0324-8Formation of ferroan dacite by lunar silicic volcanism recorded in a meteorite from the MoonHiroshi Nagaoka0Timothy J. Fagan1Masahiro Kayama2Yuzuru Karouji3Nobuyuki Hasebe4Mitsuru Ebihara5Research Institute for Science and Engineering, Waseda UniversityDepartment of Earth Science, School of Education, Waseda UniversityDepartment of Earth and Planetary Materials Science, Graduate School of Science, Tohoku UniversityJAXA Space Exploration Center, Japan Aerospace Exploration AgencyResearch Institute for Science and Engineering, Waseda UniversityDepartment of Earth Science, School of Education, Waseda UniversityAbstract An igneous clast from the Northwest Africa 773 (NWA 773) clan of lunar meteorites formed by silicic volcanism on the Moon. The clast was identified in Northwest Africa 2727 (NWA 2727), which is included in the NWA 773 clan. Over 80 mode% of the clast consists of silica + plagioclase + K-Ba-feldspar. The silica phases cristobalite, tridymite, and quartz are all present in the clast, indicating rapid cooling at low pressure in agreement with a volcanic setting. This clast is characterized as a dacite on the basis of mineral modes and whole-rock chemical composition. Olivine and pyroxene in the clast have high Fe/Mg ratios (olivine Fe# > 99, pyroxene Fe# > 99; with Fe# = molar Fe/(Fe + Mg) × 100), suggesting crystallization from a residual liquid after fractionation of more magnesian silicates. The clast is similar in some respects to ferroan gabbro alkaline-phase-ferroan (FG/ARFe) clasts that are inferred to be co-magmatic with olivine gabbro (OG) and other mafic lithologies of the NWA 773 clan. However, the high silica concentration and dominance of apatite as the main Ca-phosphate (no merrillite was identified) are distinct from the FG/ARFe clasts. Thus, the dacite clast probably crystallized in a magmatic setting that was independent of the OG and FG/ARFe lithologies. The mafic major element composition, young age, and high KREEP-content of the NWA 773 clan have been used previously to infer an origin from the Procellarum-KREEP terrane (PKT) on the nearside of the Moon. Several candidates for silicic volcanism/plutonism have been identified in the PKT (e.g., Gruithuisen Domes, Hansteen alpha, Lassell Massif). The presence of the dacite lithology provides additional support for an origin in or around PKT for meteorites of the NWA 773 clan, and for complex igneous activity in PKT region.http://link.springer.com/article/10.1186/s40645-020-0324-8MoonMineralogyPetrologyVolcanologySilicic volcanism
collection DOAJ
language English
format Article
sources DOAJ
author Hiroshi Nagaoka
Timothy J. Fagan
Masahiro Kayama
Yuzuru Karouji
Nobuyuki Hasebe
Mitsuru Ebihara
spellingShingle Hiroshi Nagaoka
Timothy J. Fagan
Masahiro Kayama
Yuzuru Karouji
Nobuyuki Hasebe
Mitsuru Ebihara
Formation of ferroan dacite by lunar silicic volcanism recorded in a meteorite from the Moon
Progress in Earth and Planetary Science
Moon
Mineralogy
Petrology
Volcanology
Silicic volcanism
author_facet Hiroshi Nagaoka
Timothy J. Fagan
Masahiro Kayama
Yuzuru Karouji
Nobuyuki Hasebe
Mitsuru Ebihara
author_sort Hiroshi Nagaoka
title Formation of ferroan dacite by lunar silicic volcanism recorded in a meteorite from the Moon
title_short Formation of ferroan dacite by lunar silicic volcanism recorded in a meteorite from the Moon
title_full Formation of ferroan dacite by lunar silicic volcanism recorded in a meteorite from the Moon
title_fullStr Formation of ferroan dacite by lunar silicic volcanism recorded in a meteorite from the Moon
title_full_unstemmed Formation of ferroan dacite by lunar silicic volcanism recorded in a meteorite from the Moon
title_sort formation of ferroan dacite by lunar silicic volcanism recorded in a meteorite from the moon
publisher SpringerOpen
series Progress in Earth and Planetary Science
issn 2197-4284
publishDate 2020-03-01
description Abstract An igneous clast from the Northwest Africa 773 (NWA 773) clan of lunar meteorites formed by silicic volcanism on the Moon. The clast was identified in Northwest Africa 2727 (NWA 2727), which is included in the NWA 773 clan. Over 80 mode% of the clast consists of silica + plagioclase + K-Ba-feldspar. The silica phases cristobalite, tridymite, and quartz are all present in the clast, indicating rapid cooling at low pressure in agreement with a volcanic setting. This clast is characterized as a dacite on the basis of mineral modes and whole-rock chemical composition. Olivine and pyroxene in the clast have high Fe/Mg ratios (olivine Fe# > 99, pyroxene Fe# > 99; with Fe# = molar Fe/(Fe + Mg) × 100), suggesting crystallization from a residual liquid after fractionation of more magnesian silicates. The clast is similar in some respects to ferroan gabbro alkaline-phase-ferroan (FG/ARFe) clasts that are inferred to be co-magmatic with olivine gabbro (OG) and other mafic lithologies of the NWA 773 clan. However, the high silica concentration and dominance of apatite as the main Ca-phosphate (no merrillite was identified) are distinct from the FG/ARFe clasts. Thus, the dacite clast probably crystallized in a magmatic setting that was independent of the OG and FG/ARFe lithologies. The mafic major element composition, young age, and high KREEP-content of the NWA 773 clan have been used previously to infer an origin from the Procellarum-KREEP terrane (PKT) on the nearside of the Moon. Several candidates for silicic volcanism/plutonism have been identified in the PKT (e.g., Gruithuisen Domes, Hansteen alpha, Lassell Massif). The presence of the dacite lithology provides additional support for an origin in or around PKT for meteorites of the NWA 773 clan, and for complex igneous activity in PKT region.
topic Moon
Mineralogy
Petrology
Volcanology
Silicic volcanism
url http://link.springer.com/article/10.1186/s40645-020-0324-8
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