activity
20052026
most citedEvolution of oxygen isotopic composition in the inner solar nebula

80 citations · 193 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2026★ 3 cited

Non-equilibrium condensation of the first Solar System solids

Sebastien Charnoz, Jérome Aleon, Marc Chaussidon +3

Primitive meteorites (chondrites) consist of an out-of-equilibrium assemblage of minerals formed during the assembling of our Solar Nebula. The conditions under which their precurs…

astro-ph.EP2022★ 36 cited

Presolar stardust in asteroid Ryugu

Jens Barosch, Larry R. Nittler, Jianhua Wang +121

We have conducted a NanoSIMS-based search for presolar material in samples recently returned from C-type asteroid Ryugu as part of JAXA's Hayabusa2 mission. We report the detection…

astro-ph.EP2015★ 23 cited

Growth of calcium-aluminum-rich inclusions by coagulation and fragmentation in a turbulent protoplanetary disk: observations and modelisation

S. Charnoz, J. Aleon, N. Chaumard +2

Whereas it is generally accepted that calcium-aluminum-rich inclusions (CAIs) from chondritic meteorites formed in a hot environment in the solar protoplanetary disk, the condition…

astro-ph.EP2011★ 51 cited

3D Lagrangian turbulent diffusion of dust grains in a protoplanetary disk: method and first applications

Sebastien Charnoz, Laure Fouchet, Jérôme Aleon +1

In order to understand how the chemical and isotopic compositions of dust grains in a gaseous turbulent protoplanetary disk are altered during their journey in the disk, it is impo…

astro-ph2008

Meteorites and the physico-chemical conditions in the early solar nebula

Jerome Aleon

Chondritic meteorites constitute the most ancient rock record available in the laboratory to study the formation of the solar system and its planets. Detailed investigations of the…

astro-ph2005★ 80 cited

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…