The great isotopic dichotomy of the early Solar System
TS Kruijer, T Kleine, LE Borg - Nature Astronomy, 2020 - nature.com
The isotopic composition of meteorites and terrestrial planets holds important clues about
the earliest history of the Solar System and the processes of planet formation. Recent work …
the earliest history of the Solar System and the processes of planet formation. Recent work …
History of the solar nebula from meteorite paleomagnetism
We review recent advances in our understanding of magnetism in the solar nebula and
protoplanetary disks (PPDs). We discuss the implications of theory, meteorite …
protoplanetary disks (PPDs). We discuss the implications of theory, meteorite …
Age of Jupiter inferred from the distinct genetics and formation times of meteorites
The age of Jupiter, the largest planet in our Solar System, is still unknown. Gas-giant planet
formation likely involved the growth of large solid cores, followed by the accumulation of gas …
formation likely involved the growth of large solid cores, followed by the accumulation of gas …
The effect of Jupiter's formation on the distribution of refractory elements and inclusions in meteorites
We present a comprehensive evolutionary model of the Sun's protoplanetary disk,
constructed to resolve the" CAI storage problem" of meteoritics. We predict the abundances …
constructed to resolve the" CAI storage problem" of meteoritics. We predict the abundances …
How accretion of planet-forming disks influences stellar abundances
LA Hühn, B Bitsch - Astronomy & Astrophysics, 2023 - aanda.org
Millimeter-sized dust grains experience radial velocities exceeding the gas velocities by
orders of magnitude. The viscous evolution of the accretion disk adds disk material onto the …
orders of magnitude. The viscous evolution of the accretion disk adds disk material onto the …
Identification of a primordial asteroid family constrains the original planetesimal population
M Delbo', K Walsh, B Bolin, C Avdellidou, A Morbidelli - Science, 2017 - science.org
A quarter of known asteroids is associated with more than 100 distinct asteroid families,
meaning that these asteroids originate as impact fragments from the family parent bodies …
meaning that these asteroids originate as impact fragments from the family parent bodies …
Hf-W chronology of CR chondrites: Implications for the timescales of chondrule formation and the distribution of 26Al in the solar nebula
Renazzo-type carbonaceous (CR) chondrites are distinct from most other chondrites in
having younger chondrule 26 Al-26 Mg ages, but the significance of these ages and whether …
having younger chondrule 26 Al-26 Mg ages, but the significance of these ages and whether …
Refractory inclusions in carbonaceous chondrites: Records of early solar system processes
AN Krot - Meteoritics & Planetary Science, 2019 - Wiley Online Library
Chondrites consist of three major components: refractory inclusions (Ca, Al‐rich inclusions
[CAI s] and amoeboid olivine aggregates), chondrules, and matrix. Here, I summarize recent …
[CAI s] and amoeboid olivine aggregates), chondrules, and matrix. Here, I summarize recent …
[HTML][HTML] The origin and early evolution of life on Earth
J Oró, SL Miller, A Lazcano - Annual Review of Earth and …, 1990 - adsabs.harvard.edu
The Origin and Early Evolution of Life on Earth ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS …
completely retired in October 2019. This page will automatically redirect to the new ADS …
Lifetime of the outer solar system nebula from carbonaceous chondrites
The evolution and lifetime of protoplanetary disks (PPDs) play a central role in the formation
and architecture of planetary systems. Astronomical observations suggest that PPDs evolve …
and architecture of planetary systems. Astronomical observations suggest that PPDs evolve …