Dynamical evolution of the early solar system
D Nesvorný - Annual Review of Astronomy and Astrophysics, 2018 - annualreviews.org
Several properties of the Solar System, including the wide radial spacing of the giant
planets, can be explained if planets radially migrated by exchanging orbital energy and …
planets, can be explained if planets radially migrated by exchanging orbital energy and …
The late heavy bombardment
Heavily cratered surfaces on the Moon, Mars, and Mercury show that the terrestrial planets
were battered by an intense bombardment during their first billion years or more, but the …
were battered by an intense bombardment during their first billion years or more, but the …
The Lidov-Kozai oscillation and hugo von Zeipel
T Ito, K Ohtsuka - arXiv preprint arXiv:1911.03984, 2019 - arxiv.org
The so-called Lidov-Kozai oscillation is very well known and applied to various problems in
solar system dynamics. This mechanism makes the orbital inclination and eccentricity of the …
solar system dynamics. This mechanism makes the orbital inclination and eccentricity of the …
Mars' growth stunted by an early giant planet instability
Many dynamical aspects of the solar system can be explained by the outer planets
experiencing a period of orbital instability sometimes called the Nice Model. Though often …
experiencing a period of orbital instability sometimes called the Nice Model. Though often …
Dynamical evidence for an early giant planet instability
R de Sousa Ribeiro, A Morbidelli, SN Raymond… - Icarus, 2020 - Elsevier
The dynamical structure of the Solar System can be explained by a period of orbital
instability experienced by the giant planets. While a late instability was originally proposed …
instability experienced by the giant planets. While a late instability was originally proposed …
The role of early giant-planet instability in terrestrial planet formation
The terrestrial planets are believed to have formed by violent collisions of tens of lunar-to
Mars-size protoplanets at time t< 200 Myr after the protoplanetary gas disk dispersal (t 0) …
Mars-size protoplanets at time t< 200 Myr after the protoplanetary gas disk dispersal (t 0) …
Isotopic trichotomy of main belt asteroids from implantation of outer solar system planetesimals
D Nesvorný, N Dauphas, D Vokrouhlický… - Earth and Planetary …, 2024 - Elsevier
Recent analyses of samples from asteroid (162173) Ryugu returned by JAXA's Hayabusa2
mission suggest that Ryugu and CI chondrites formed in the same region of the …
mission suggest that Ryugu and CI chondrites formed in the same region of the …
Consequences of planetary migration on the minor bodies of the early solar system
Pebble accretion is an efficient mechanism that is able to build up the core of the giant
planets within the lifetime of the protoplanetary disc gas-phase. The core grows via this …
planets within the lifetime of the protoplanetary disc gas-phase. The core grows via this …
Constraining the giant planets' initial configuration from their evolution: Implications for the timing of the planetary instability
Recent works on planetary migration show that the orbital structure of the Kuiper Belt can be
very well reproduced if, before the onset of planetary instability, Neptune underwent a long …
very well reproduced if, before the onset of planetary instability, Neptune underwent a long …
Early bombardment of the moon: Connecting the lunar crater record to the terrestrial planet formation
The lunar crater record features∼ 50 basins. The radiometric dating of Apollo samples
indicates that the Imbrium basin formed relatively late—from the planet formation …
indicates that the Imbrium basin formed relatively late—from the planet formation …