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note
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This research was supported by the NASA Cosmochemistry Program (D.D.C.), the Origins of Solar Systems Program (D.D.C.), and the Astrophysics Theory Program (W.L); by the U.S. Department of Energy under contract DE-AC05-96OR22464 with Lockheed Martin Energy Research Corporation (W.L.), and by NSF Division of Astronomical Sciences (A.D.).
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