A&A, 572, A72 (2014). 31 pages, 29 figures. (Final version)International audienceContext. Circumstellar disks are known to contain a significant mass in dust ranging from micron to centimeter size.
Guillot, Tristan +2 more
core
Protracted core formation and impact disruptions shaped the earliest outer Solar System planetesimals. [PDF]
Grewal DS +5 more
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Chalcogen isotopes reveal limited volatile contribution from late veneer to Earth. [PDF]
Wang W +4 more
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Chondrule formation by collisions of planetesimals containing volatiles triggered by Jupiter's formation. [PDF]
Sirono SI, Turrini D.
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Hydrogen Isotopic Fractionation in the Solar Nebula and Implications for Water in Earth and Inner Solar System Bodies. [PDF]
Asaduzzaman A.
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The Origins & Reservoirs of Exocomets. [PDF]
Bannister M +13 more
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Aqueous breakdown of aspartate and glutamate to n-ω-amino acids on the parent bodies of carbonaceous chondrites and asteroid Ryugu. [PDF]
Li Y +12 more
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Origin and Evolution of the Galilean Satellites Within the Jovian System. [PDF]
Nimmo F +10 more
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I/Pu reveals Earth mainly accreted from volatile-poor differentiated planetesimals. [PDF]
Liu W +5 more
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Silicon isotope constraints on terrestrial planet accretion. [PDF]
Onyett IJ +5 more
europepmc +1 more source

