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astro-ph2006★ 34 cited
Meteoritical and dynamical constraints on the growth mechanisms and formation times of asteroids and Jupiter
Edward R. D. Scott
Peak temperatures inside meteorite parent bodies are closely linked to accretion times. Most iron meteorites come from bodies that accreted <0.5 Myr after CAIs formed and were melt…
astro-ph2005
Evolution of oxygen isotopic composition in the inner solar nebula
Alexander N. Krot, Ian D. Hutcheon, Hisayoshi Yurimoto +7
Changes in the chemical and isotopic composition of the solar nebula with time are reflected in the properties of different constituents that are preserved in chondritic meteorites…
astro-ph2005
Thermal Processing of Silicate Dust in the Solar Nebula: Clues from Primitive Chondrite Matrices
Edward R. D. Scott, Alexander N. Krot
The most abundant matrix minerals in chondritic meteorites, hydrated phyllosilicates and ferrous olivine crystals, formed predominantly in asteroids during fluid-assisted metamorph…