Using HED meteorites to interpret neutron and gamma‐ray data from asteroid 4 Vesta |
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| Authors: | Andrew W Beck David J Lawrence Patrick N Peplowski Thomas H Prettyman Timothy J McCoy Harry Y McSween Jr Michael J Toplis Naoyuki Yamashita |
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| Affiliation: | 1. The Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, USA;2. Planetary Science Institute, Tucson, Arizona, USA;3. Department of Mineral Sciences, Smithsonian Institution, Washington, District of Columbia, USA;4. Department of Earth and Planetary Sciences, The University of Tennessee, Knoxville, Tennessee, USA;5. Université de Toulouse, UPS‐OMP, Institut de Recherche en Astrophysiqe et Planétologie, Toulouse, France;6. CNRS, IRAP, Toulouse, France |
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| Abstract: | Here, we construct a comprehensive howardite, eucrite, and diogenite (HED) bulk chemistry data set to compare with Dawn data. Using the bulk chemistry data set, we determine four gamma‐ray/neutron parameters in the HEDs (1) relative fast neutron counts (fast counts), (2) macroscopic thermal neutron absorption cross section (absorption), (3) a high‐energy gamma‐ray compositional parameter (Cp), and (4) Fe abundance. These correspond to the four measurements of Vesta made by Dawn's Gamma Ray and Neutron Detector (GRaND) that can be used to discern HED lithologic variability on the Vestan surface. We investigate covariance between fast counts and average atomic mass (<A>) in the meteorite data set, where a strong correlation (r2 = 0.99) is observed, and we demonstrate that systematic offsets from the fast count/<A> trend are linked to changes in Fe and Ni concentrations. To compare the meteorite and GRaND data, we investigate and report covariance among fast counts, absorption, Cp, and Fe abundance in the HED meteorite data set. We identify several GRaND measurement spaces where the Yamato type B diogenites are distinct from all other HED lithologies, including polymict mixtures. The type B's are diogenites that are enriched in Fe + pigeonite + diopside ± plagioclase, relative to typical, orthopyroxenitic diogenites. We then compare these results to GRaND data and demonstrate that regions north of ~70°N latitude on Vesta (including the north pole) are consistent with type B diogenites. We propose two models to explain type B diogenite compositions in the north (1) deposition as Rheasilvia ejecta, or (2) type B plutons that were emplaced at shallow depths in the north polar region and sampled by local impacts. Lastly, using principal component (PC) analysis, we identify unique PC spaces for all HED lithologies, indicating that the corresponding GRaND measurables may be used to produce comprehensive lithologic maps for Vesta. |
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