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Fayalite from
Luna 24 landing site, Mare Crisium, The Moon


Locality type:Landing Site
Classification
Species:Fayalite
Formula:Fe22+SiO4
Confirmation
Validity:Confirmed
Confirmation Methods:SEM-EDS
Associated Minerals Based on Photo Data:
Ulvöspinel2 photos of Fayalite associated with Ulvöspinel at this locality.
Augite2 photos of Fayalite associated with Augite at this locality.
Anorthite2 photos of Fayalite associated with Anorthite at this locality.
Zirconolite1 photo of Fayalite associated with Zirconolite at this locality.
Ilmenite1 photo of Fayalite associated with Ilmenite at this locality.
Aluminian Chromite1 photo of Fayalite associated with Aluminian Chromite at this locality.
Troilite1 photo of Fayalite associated with Troilite at this locality.
Data
Mineral Data:Click here to view Fayalite data
Locality Data:Click here to view Luna 24 landing site, Mare Crisium, The Moon
Data Identifiers
Mindat Occurrence Record ID:845051
Long-form Identifier:1:3:845051:7
GUID (UUID V4):62ed04e7-1697-4d94-bece-81e644ea1eab
References
Reference Search (possible matching items)
Journal (article/letter/editorial)
Pleiades Publishing, Ltd., 2019. Russian Text © The Author(s), 2019, published in Geokhimiya, 2019, No...Olivines of Lunar Rocks: Sources and Localization in the Lunar Crust S. I. Demidovaa, *, M. O. Anosovaa, *...highland, mare, and mingled meteorites and in “Apollo-14”, “Luna-16, -20, -24” lunar samples. The olivines...possible sources of P-bearing olivine were found in the lunar material: 1) highland anorthositic–noritic–troctolitic...to high-Mg suite rocks: 2) late-stage products of mare basalts crystallization; and 3) unusual olivine–orthopyroxene
Journal (article/letter/editorial)
chronology and petrogenesis along the eastern limb of the Moon from Luna 16,20 and 24 samples B. A. COHENI, G....Abstract-Eighteen new lithic fragments from the Soviet Luna missions have been analyzed with electron microprobe...microprobe and 4OAr-39Ar methods. Luna 16 basalt fragments have aluminous compositions consistent with...wellconstrained ages (3347 & 24 Ma, 342 1 f 30 Ma). These data, combined with other Luna 16basalt ages, imply...there were multiple volcanic events filling Mare Fecunditatis. The returned basalt fragments have relatively
Journal (article/letter/editorial)
accepted in revised form .-Iugusr 2. 199 1 ) Abstract-The new lunar meteorite MAC88 105 has been studied by...mineral-chemical techniques and was compared with the Yamato lunar meteorites. Clast types and pyroxene...are not as common as in other lunar meteorites. The large and common granulitelike me&igneous clasts...crystals with fine-grained olivine and pyroxenes in the interstices. Pyroxenes with mg number = Mg X lOO/(...zoning trends more Mg-rich than the above mg range and than those of the VLT basalts common in lunar meteorites
Journal (article/letter/editorial)
–3518, 2003 Copyright © 2003 Elsevier Ltd Printed in the USA. All rights reserved 0016-7037/03 $30.00 ⫹ .00...Environmental Research, Ocean Research Institute, The University of Tokyo, Nakanoku, Tokyo, 164-8639, Japan...clasts. The matrix consists mainly of smaller mineral fragments (⬍0.5 mm), bound by glassy cement, the majority...majority of which are pyroxene and plagioclase. The pyroxene possesses extensive exsolution lamellae. These...are atypical for mare-basalts. One of the distinguishing textures of EET 96008 is the presence of small
Journal (article/letter/editorial)
2012; revision accepted 05 November 2012) Abstract–The Northwest Africa (NWA) 2996 meteorite is a lunar...clasts contain clusters of apatite, suggesting that the anorthosites either assimilated evolved rocks or...around the South Pole Aitken (SPA) basin, peripheral regions of eastern mare, Nectaris, Crisium, and southern...of Mare Humorum. However, the mineralogy of NWA 2996 is distinctive compared with Apollo and Luna mission...samples, and is likely consistent with an origin near the SPA basin: anorthosite clasts could represent local
Journal (article/letter/editorial)
1111/maps.12597 High crustal diversity preserved in the lunar meteorite Mount DeWitt 12007 (Victoria Land...2015; revision accepted 10 November 2015) Abstract–The meteorite Mount DeWitt (DEW) 12007 is a polymict...interspersed). The presence of tranquillityite, coupled with the petrophysical data, the O-isotope data...data (D17O = 0.075), and the FeOtot/MnO ratios in olivine (91), pyroxene (65), and bulk rock (77) indicate...plagioclase-rich meta-melt clasts. The volcanic products belong to the very low titanium (VLT) or low titanium
Journal (article/letter/editorial)
breccia Northwest Africa 7948 and implication for the lithologic components of lunar crust Xiaojia ZENG...14 December 2017) Abstract–This study presents the petrography, mineralogy, and bulk composition of...Apollo regolith breccias. Comparing the bulk composition of the meteorite with remotely sensed geochemical...suggests that the sample was derived from a region of the lunar surface distal from the nearside Th-rich...ejected from a nearside highlands-mare boundary (e.g., around Mare Crisium or Orientale) or a cryptomare
Journal (article/letter/editorial)
Meteoritical Society, 1996. Printed in USA. Four lunar mare meteorites: Crystallization trends of pyroxenes...Antarctic meteorites known to be derived from mare regions of the Moon: Y-793 169 and A-881757 (YA meteorites)...All have relatively low bulkrock Ti02 content, and the YA meteorites are uncommonly ancient. Our electron...microanalysis (EPMA) data indicate that the Y A meteorites and the dominant mare components of Y-793274 and EET...general trend for Ti-poor (low-Ti and very low-Ti) mare basalts. Their pyroxenes show a strong correlation
Journal (article/letter/editorial)
Abstract–Here we report the petrography, mineralogy, and trace element geochemistry of the Dhofar 1180 lunar...lithic clasts are moderately to extremely Fe-rich. The Ti/[Ti+Cr]-Fe/[Fe+Mg] compositional trend of pyroxenes...lithic clasts is consistent with that of low-Ti mare basalts. Glasses display a wide chemical variation...probably a last-stage differentiation product of mare basalt. Molar Fe/Mn ratios of both olivine and pyroxene...derived from an area on the lunar nearside but far away from the center of the Imbrium Basin. INTRODUCTION
Journal (article/letter/editorial)
mingled impact melt breccia from the highlands—A complete cross section of the lunar crust S. E. ROBERTS 1...Mg-suite, and gabbronorite lithologies as defined by the Apollo sample collection. Clasts representing magnesian...mineralogy although pyroxferroite grains are present. The juxtaposition of evolved, basaltic clasts without...these basaltic clasts may represent cryptomare. The lithologies found in NWA 10986 offer a unique and...section view of the Moon sourced outside of the Procellarum KREEP Terrane. rich terrain, the Procellarum
Journal (article/letter/editorial)
breccias preserve the records of geologic processes on the Moon. In this study, we report the occurrence, petrography...petrography, mineralogy, and geologic significance of the observed secondary olivine veinlets in lunar feldspathic...dominated by interconnecting olivine mineral grains. The host clasts are mainly composed of mafic minerals...lithology. The studied olivine veinlets (~5 to 30 lm in width) are distributed within the mafic mineral...mineral host, but do not extend into the adjacent plagioclase. Chemically, these olivine veinlets are Fe-richer
Journal (article/letter/editorial)
homepage: http://www.tandfonline.com/loi/tigr20 Moon rock mineralogy V. L. Barsukov , M. A. Nazarav &...& L. S. Tarasov (1982) Moon rock mineralogy, International Geology Review, 24:2, 238-248, DOI: 10.10...13:40 Moon rock mineralogy V.L. Borsukov, M.A. Nozorov, ond L.S. Torosov is restricted to the range...parts of the hloon (Vinogradov, 1975; Schmitt, 1975; Florenskiy et al., 1977). Nevertheless, the material...various laboratories throughout the world is reasonably representative, and the data can be combined with orbital
Journal (article/letter/editorial)
(2019) doi: 10.1111/maps.13295 The early geological history of the Moon inferred from ancient lunar meteorite...breccia that provides insights into the early magmatic history of the Moon. MIL 13317 is formed from a mixture...for ~835  84 Myr, at an average depth of ~30 cm. The fusion crust has an intermediate composition (Al2O3...ppm) chemical component. Taking the fusion crust to be indicative of the bulk sample composition, this...originated from a regolith that is associated with a mare-highland boundary that is KREEP-rich (i.e., K, rare
Journal (article/letter/editorial)
diversity at the Apollo 12 landing site: Inferences from petrologic examinations of the soil sample 12003...Sciences, Open University, Milton Keynes MK7 6AA, UK The Centre for Planetary Sciences at UCL-Birkbeck, Gower...10 mm) from the 12003 soil sample as part of an ongoing study of basaltic diversity at the Apollo 12 landing...landing site. An attempt has been made to classify these samples according to the well-established grouping...identified within the 12003 soil. One sample is identified as a possible new addition to the feldspathic suite
Journal (article/letter/editorial)
version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting...note that during the production process errors may be discovered which could affect the content, and all...all legal disclaimers that apply to the journal pertain. Oldest high-Ti basalt and magnesian crustal...this meteorite for the first time, and in situ U-Pb dating of apatite in one of the high-Ti basalts shows...one of the earliest high-Ti basalts on the Moon. 3. The magnesian cores of pyroxene from the dated high-Ti
Report (volume)
MINERALOGY & GEOCHEMISTRY Volume 60 NEW VIEWS of the MOON EDITORS: Bradley L. Jolliff, Mark A. Wieczorek...This book is dedicated to the memory of the late Graham Ryder, who was one of the original four members of...of CAPTEM when the New Views of the Moon scientific initiative was first conceived. Graham, who was a...owing to his broad knowledge of the lunar samples and his residence at the Lunar and Planetary Institute...where CAPTEM met, was a logical choice to be one of the co-leaders of this lunarscience initiative. Not only
Report (issue)
GEOCHIMICA ETT COSMOCHIMICA ACTA + Journal ey The Geochemical ce and. The ercenitter] Society Albright College...miles). North is at the upper right edge of the disc. Seen above the planet are the satellites Dione (right)...spot at the south edge of a yellow band; in true color, the spot would appear brown and the band white...spot slightly above and to the left in this image moves eastward relative to the green spot at a rate that...it to pass the green feature in about 50 days. The convective clouds that appear between the two spots
 
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