History of the solar nebula from meteorite paleomagnetism. [PDF]
Weiss BP, Bai XN, Fu RR.
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Carbon and oxygen isotope evidence for a protoplanetary disk origin of organic solids in meteorites. [PDF]
Lawrence WM, Blake GA, Eiler J.
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Chondrule age distribution and rate of heating events for chondrule formation
Chondrules are considered to be formed by flash heating events in the protoplanetary disk. In order to evaluate some basic factors in the heating mechanism, we examined the rate of heating events that explains the abundance and the observed age distribution of chondrules in unequilibrated ordinary chondrites. First, we compiled the literature data of ^(
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Low-Temperature Aqueous Alteration of Chondrites. [PDF]
Lee MR +19 more
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The Ni isotopic composition of Ryugu reveals a common accretion region for carbonaceous chondrites. [PDF]
Spitzer F +90 more
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Cross-Scale Multimodal Imaging for Organic Matter in Extraterrestrial Samples. [PDF]
Dong M +8 more
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The initial solar system abundance of 60Fe and early core formation of the first asteroids. [PDF]
Fang L +5 more
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Impact-induced sublimation drives volatile depletion in carbonaceous meteorites. [PDF]
Long ZY +11 more
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Triple oxygen isotopes of lunar water unveil indigenous and cometary heritage. [PDF]
Thiemens MM, Martinez MHN, Thiemens MH.
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Instantaneous formation of interstellar minerals and mineral quantum dots. [PDF]
Roy A +13 more
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