PMID- 33819749 OWN - NLM STAT- PubMed-not-MEDLINE LR - 20210419 IS - 1873-3557 (Electronic) IS - 1386-1425 (Linking) VI - 255 DP - 2021 Jul 5 TI - Compositional and spectrochemical analyses of Cr-spinels in the Sittampundi Anorthosite Complex, Southern India: Implications for remote observation of spinels on the Moon. PG - 119677 LID - S1386-1425(21)00253-5 [pii] LID - 10.1016/j.saa.2021.119677 [doi] AB - The spectroscopic techniques such as Laser Raman, Fourier Transform Infrared (FTIR), and hyperspectral have been used widely to understand the mineral chemistry and crystal structure and identify the functional phases and organic molecules in geological materials on Earth and other planetary bodies. The present study used these spectroscopic techniques combined with X-ray Diffraction (XRD) and Electron Probe Micro Analysis (EPMA) to understand the spectral-compositional relationships of the Cr-spinel (Chromian spinel) present in chromitite bodies associated with Sittampundi Anorthosite Complex (SAC), southern India. The bands/lenses of Cr-spinel are found as layers (few centimeters to 6 m thick) intercalated with anorthosites and clinopyroxenites of the SAC. The cumulate Cr-spinels of the study area exhibit compositions ranging between Al-chromite and Cr-spinel. Fe-, Al-rich Cr-spinel is a characteristic of the SAC with Cr(2)O(3) content ranging from ~32-37 wt% and Cr# (Cr/[Cr + Al]) in the 0.44 to 0.53 range. The XRD spectra of these Cr-spinels have shown characteristic peaks corresponding to its constituent phases, with the highest peak at 36.11 degrees . The observed longward shift in the Raman A(1g) peak (~705-714 cm(-1)) is likely to be caused by the substitution of Al(3+) in the spinel structure. The Raman A(1g) peak position near 705 cm(-1) in the spectra is attributed to the coexistence of (Mg, Fe) in the tetrahedral site and (Al, Cr) in the octahedral site. The broader and stronger 2 microm band position in the hyperspectral data is at relatively shorter wavelengths than typical Cr-spinels due to enhanced Al content (Al(2)O(3) ~ 25 wt%) in the SAC samples. The 2 microm band position is observed to have a longward shift with increasing Cr(2)O(3) and Cr# abundances and a corresponding shortward shift with enhanced Al(2)O(3) content in Cr-spinels. The linear relationship between the 2 microm band position and Cr/Al abundances indicates that this absorption band is significant in distinguishing Cr-spinels from Al-spinels. Based on spectral and compositional resemblance, Fe- and Al-rich Cr-spinels in SAC are considered as probable terrestrial (functional) analogues for similar lunar spinel compositions given that evidence-based correlation of intricate processes involved in their formation under the lunar and terrestrial conditions. The present study demonstrates the approach of applying spectrochemical characteristics of terrestrial analogue spinels for remote identification of lunar spinels and retrieving their compositional ranges from the spectral reflectance parameters. CI - Copyright (c) 2021 Elsevier B.V. All rights reserved. FAU - Thesniya, P M AU - Thesniya PM AD - Department of Earth and Space Sciences, Indian Institute of Space Science and Technology (IIST), Thiruvananthapuram 695 547, India. FAU - Saranya, R AU - Saranya R AD - Department of Geology, University of Kerala, Thiruvananthapuram 695 581, India. FAU - Rajesh, V J AU - Rajesh VJ AD - Department of Earth and Space Sciences, Indian Institute of Space Science and Technology (IIST), Thiruvananthapuram 695 547, India. Electronic address: rajeshvj@iist.ac.in. LA - eng PT - Journal Article DEP - 20210309 PL - England TA - Spectrochim Acta A Mol Biomol Spectrosc JT - Spectrochimica acta. Part A, Molecular and biomolecular spectroscopy JID - 9602533 SB - IM OTO - NOTNLM OT - Chemical and spectral analyses OT - Cr-spinel OT - Lunar spinels OT - Sittampundi Anorthosite Complex OT - Southern India OT - Terrestrial analogue COIS- Declaration of Competing Interest The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper. EDAT- 2021/04/06 06:00 MHDA- 2021/04/06 06:01 CRDT- 2021/04/05 20:15 PHST- 2020/07/13 00:00 [received] PHST- 2021/02/25 00:00 [revised] PHST- 2021/03/01 00:00 [accepted] PHST- 2021/04/06 06:00 [pubmed] PHST- 2021/04/06 06:01 [medline] PHST- 2021/04/05 20:15 [entrez] AID - S1386-1425(21)00253-5 [pii] AID - 10.1016/j.saa.2021.119677 [doi] PST - ppublish SO - Spectrochim Acta A Mol Biomol Spectrosc. 2021 Jul 5;255:119677. doi: 10.1016/j.saa.2021.119677. Epub 2021 Mar 9.