Exposure history of the Sutter's Mill carbonaceous chondrite |
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| Authors: | K Nishiizumi M W Caffee Y Hamajima R C Reedy K C Welten |
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| Institution: | 1. Space Sciences Laboratory, University of California, , Berkeley, California, 94720–7450 USA;2. Department of Physics, Purdue University, , West Lafayette, Indiana, 47907–2036 USA;3. Low Level Radioactivity Laboratory, Kanazawa University, , Nomi, Ishikawa, 923‐1224 Japan;4. Planetary Science Institute, , Los Alamos, New Mexico, 87544–3826 USA |
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| Abstract: | The Sutter's Mill (SM) carbonaceous chondrite fell in California on April 22, 2012. The cosmogenic radionuclide data indicate that Sutter's Mill was exposed to cosmic rays for 0.082 ± 0.008 Myr, which is one of the shortest ages for C chondrites, but overlaps with a small cluster at approximately 0.1 Myr. The age is significantly longer than proposed ages that were obtained from cosmogenic noble gas concentrations, which have large uncertainties due to trapped noble gas corrections. The presence of neutron‐capture 60Co and 36Cl in SM indicates a minimum preatmospheric radius of approximately 50 cm, and is consistent with a radius of 1–2 m, as derived from the fireball observations. Although a large preatmospheric size was proposed, one fragment (SM18) contains solar cosmic ray–produced short‐lived radionuclides, such as 56Co and 51Cr. This implies that this specimen was less than 2 cm from the preatmospheric surface of Sutter's Mill. Although this conclusion seems surprising, it is consistent with the observation that the meteoroid fragmented high in the atmosphere. The presence of SCR‐produced nuclides is consistent with the high SCR fluxes observed during the last few months before the meteorite's fall, when its orbit was less than 1 AU from the Sun. |
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