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AffiliationUniv Arizona, Lunar & Planetary Lab, 1629 E Univ Blvd, Tucson, AZ 85721 USA
MetadataShow full item record
PublisherOXFORD UNIV PRESS
CitationDo L chondrites come from the Gefion family? Allison M McGraw Vishnu Reddy Juan A Sanchez Monthly Notices of the Royal Astronomical Society, Volume 476, Issue 1, 1 May 2018, Pages 630–634, https://doi.org/10.1093/mnras/sty250
Rights© 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
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AbstractOrdinary chondrites (H, L, and LL chondrites) are the most common type of meteorites comprising 80 per cent of the meteorites that fall on Earth. The source region of these meteorites in the main asteroid belt has been a basis of considerable debate in the small bodies community. L chondrites have been proposed to come from the Gefion asteroid family, based on dynamical models. We present results from our observational campaign to verify a link between the Gefion asteroid family and L chondrite meteorites. Near-infrared spectra of Gefion family asteroids (1839) Ragazza, (2373) Immo, (2386) Nikonov, (2521) Heidi, and (3860) Plovdiv were obtained at the NASA Infrared Telescope Facility (IRTF). Spectral band parameters including band centres and the band area ratio were measured from each spectrum and used to constrain the composition of these asteroids. Based on our results, we found that some members of the Gefion family have surface composition similar to that of H chondrites, primitive achondrites, and basaltic achondrites. No evidence was found for L chondrites among the Gefion family members in our small sample study. The diversity of compositional types observed in the Gefion asteroid family suggests that the original parent body might be partially differentiated or that the three asteroids with non-ordinary chondrite compositions might be interlopers.
VersionFinal published version
SponsorsIRTF TAC; National Aeronautics and Space Administration [NNH14CK55B]; NASA Planetary Geology and Geophysics Grants [NNX14AN05G, NNX14AM94G]; NASA Planetary Astronomy Grant [NNX14AJ37G]; NASA Undergraduate Space Grant Consortium