2013Proceedings of XII International Symposium on Nuclei in the Cosmos — PoS(NIC XII)Open access

Ni isotope systematics in chondrules from unequilibrated chondrites to constraint 60Fe in the early Solar system.

R. K. Mishra, Marc Chaussidon, K. K. Marhas

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Abstract

Presence of 60 Fe in early Solar System was established more than two decades ago, but the Solar System initial ratio of 60 Fe/ 56 Fe is, still, not well constrained.Isotopic studies of bulk meteorites samples from differentiated meteorites, achondrites, and chondrules suggest a low Solar System initial 60 Fe/ 56 Fe value of ~2×10 -8 , while the in-situ studies using secondary ion mass spectrometer suggest a much higher Solar System initial value of ~7×10 -7 .

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Presence of 60 Fe in early Solar System was established more than two decades ago, but the Solar System initial ratio of 60 Fe/ 56 Fe is, still, not well constrained.Isotopic studies of bulk meteorites samples from differentiated meteorites, achondrites, and chondrules suggest a low Solar System initial 60 Fe/ 56 Fe value of ~2×10 -8 , while the in-situ studies using secondary ion mass spectrometer suggest a much higher Solar System initial value of ~7×10 -7 .

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Available abstract

Presence of 60 Fe in early Solar System was established more than two decades ago, but the Solar System initial ratio of 60 Fe/ 56 Fe is, still, not well constrained.Isotopic studies of bulk meteorites samples from differentiated meteorites, achondrites, and chondrules suggest a low Solar System initial 60 Fe/ 56 Fe value of ~2×10 -8 , while the in-situ studies using secondary ion mass spectrometer suggest a much higher Solar System initial value of ~7×10 -7 .

Key concepts: Chondrule, Achondrite, Meteorite, Chondrite, Formation and evolution of the Solar System, Solar System, Astrobiology, Isotope

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Ni isotope systematics in chondrules from unequilibrated chondrites to constraint 60Fe in the early Solar system. — Research Paper | ScholarLens