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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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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