activity
20022023
most citedAbundance, distribution, and origin of 60Fe in the solar protoplanetary disk

210 citations · 1.7k across the 28 of their papers we have counts for

collaborators

28 papers

astro-ph.EP2023★ 4 cited

Methodologies for 176Lu-176Hf Analysis of Zircon Grains from the Moon and Beyond

Xi Chen, Nicolas Dauphas, Zhe J. Zhang +6

Zircons are found in extraterrestrial rocks from the Moon, Mars, and some differentiated meteorite parent-bodies. These zircons are rare, often of small size, and have been affecte…

astro-ph.IM2023

Science Priorities for the Extraction of the Solid MSR Samples from their Sample Tubes

N. Dauphas, S. S. Russell, D. Beaty +20

Preservation of the chemical and structural integrity of samples that will be brought back from Mars is paramount to achieving the scientific objectives of MSR. Given our knowledge…

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.SR2021

Oxygen and Aluminum-Magnesium Isotopic Systematics of Presolar Nanospinel Grains from CI Chondrite Orgueil

Nan Liu, Nicolas Dauphas, Sergio Cristallo +2

Presolar oxide grains have been previously divided into several groups (Group 1 to 4) based on their isotopic compositions, which can be tied to several stellar sources. Much of av…

astro-ph.EP2021

Earth's accretion inferred from iron isotopic anomalies of supernova nuclear statistical equilibrium origin

Timo Hopp, Nicolas Dauphas, Fridolin Spitzer +2

Nucleosynthetic Fe isotopic anomalies in meteorites may be used to reconstruct the early dynamical evolution of the solar system and to identify the origin and nature of the materi…

astro-ph.EP2021★ 38 cited

Terrestrial planet formation by torque-driven convergent migration of planetary embryos

M. Brož, O. Chrenko, D. Nesvorný +1

Massive cores of the giant planets are thought to have formed in a gas disk by accretion of pebble-size particles whose accretional cross-section is enhanced by aerodynamic gas dra…