Age of Jupiter inferred from the distinct genetics and formation times of meteorites

TS Kruijer, C Burkhardt, G Budde… - Proceedings of the …, 2017 - National Acad Sciences
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 …

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 partitioning of the inner and outer Solar System by a structured protoplanetary disk

R Brasser, SJ Mojzsis - Nature Astronomy, 2020 - nature.com
Mass-independent isotopic anomalies define two cosmochemically distinct regions: the
carbonaceous and non-carbonaceous meteorites, implying that the non-carbonaceous …

Isotopic evolution of the inner solar system inferred from molybdenum isotopes in meteorites

F Spitzer, C Burkhardt, G Budde… - The Astrophysical …, 2020 - iopscience.iop.org
The fundamentally different isotopic compositions of non-carbonaceous (NC) and
carbonaceous (CC) meteorites reveal the presence of two distinct reservoirs in the solar …

On the luminosity of young Jupiters

MS Marley, JJ Fortney, O Hubickyj… - The Astrophysical …, 2007 - iopscience.iop.org
Traditional thermal evolution models of giant planets employ arbitrary initial conditions
selected more for computational expediency than physical accuracy. Since the initial …

The formation of Jupiter by hybrid pebble–planetesimal accretion

Y Alibert, J Venturini, R Helled, S Ataiee, R Burn… - Nature …, 2018 - nature.com
The standard model for giant planet formation is based on the accretion of solids by a
growing planetary embryo, followed by rapid gas accretion once the planet exceeds a so …

Jupiter's decisive role in the inner Solar System's early evolution

K Batygin, G Laughlin - Proceedings of the National …, 2015 - National Acad Sciences
The statistics of extrasolar planetary systems indicate that the default mode of planet
formation generates planets with orbital periods shorter than 100 days and masses …

Breaking Degeneracies in Formation Histories by Measuring Refractory Content in Gas Giants

Y Chachan, HA Knutson, J Lothringer… - The Astrophysical …, 2023 - iopscience.iop.org
Relating planet formation to atmospheric composition has been a long-standing goal of the
planetary science community. So far, most modeling studies have focused on predicting the …

Jupiter's formation and its primordial internal structure

M Lozovsky, R Helled, ED Rosenberg… - The Astrophysical …, 2017 - iopscience.iop.org
The composition of Jupiter and the primordial distribution of the heavy elements are
determined by its formation history. As a result, in order to constrain the primordial internal …

[HTML][HTML] Revelations on Jupiter's formation, evolution and interior: Challenges from Juno results

R Helled, DJ Stevenson, JI Lunine, SJ Bolton… - Icarus, 2022 - Elsevier
The Juno mission has revolutionized and challenged our understanding of Jupiter. As Juno
transitioned into its extended mission, we review the major findings of Jupiter's internal …