Igneous processes in the small bodies of the Solar System I. Asteroids and comets. [PDF]
Leone G, Tanaka HKM.
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Oxygen isotopes of anhydrous primary minerals show kinship between asteroid Ryugu and comet 81P/Wild2. [PDF]
Kawasaki N +93 more
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Forming the Noncarbonaceous Chondrite Parent Bodies in the Presence of the Jupiter Barrier
Meteorites can be divided into two groups—noncarbonaceous chondrite like (NC) and carbonaceous chondrite like (CC)—with distinct stable-isotope compositions. Parent bodies of NC and CC meteorites have overlapping formation ages. This suggests they formed
John Chambers
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Fast, collimated jets are ubiquitous features of young stellar objects. They are generally thought to be powered by disk accretion, but the details are debated.
Yisheng Tu +4 more
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Paleomagnetic evidence for a disk substructure in the early solar system. [PDF]
Borlina CS +6 more
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A novel method for extracting metals from asteroids using non-aqueous deep eutectic solvents. [PDF]
Rivera RM +3 more
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Imprint of chondrule formation on the K and Rb isotopic compositions of carbonaceous meteorites. [PDF]
Nie NX +7 more
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Igneous meteorites suggest Aluminium-26 heterogeneity in the early Solar Nebula. [PDF]
Krestianinov E +11 more
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Combining Micro-Raman Spectroscopy and Scanning Electron Microscopy Mapping: A Stony Meteorite Study. [PDF]
Musa M +5 more
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Initial Conditions of Planet Formation: Time Constraints from Small Bodies and the Lifetime of Reservoirs in the Solar Protoplanetary Disk. [PDF]
Schönbächler M +3 more
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