Results 91 to 100 of about 21,167 (278)

Satellites and Small Bodies With ALMA: Insights Into Solar System Formation and Evolution

AGU Advances, Volume 6, Issue 6, December 2025.
Abstract Our understanding of the formation and evolution of planetary systems has made major advances in the past decade. This progress has been driven in large part by the Atacama Large Millimeter/submillimeter Array (ALMA), which has given us an unprecedented view of solar system bodies themselves, and of the structure and chemistry of forming ...
Katherine de Kleer, Michael E. Brown, Martin Cordiner, Richard Teague   +3 more
wiley   +1 more source

APPLICATION OF GAS DYNAMICAL FRICTION FOR PLANETESIMALS. I. EVOLUTION OF SINGLE PLANETESIMALS [PDF]

The Astrophysical Journal, 2015
Accepted to ...
Evgeni Grishin, Hagai B. Perets
openaire   +2 more sources

Birth and Decline of Magma Oceans in Planetesimals: 2. Structure and Thermal History of Early Accreted Small Planetary Bodies [PDF]

, 2022
Cyril Sturtz, Angela Limare, S. Tait, É. Kaminski   +3 more
openalex   +1 more source

Consequences of the simultaneous formation of giant planets by the core accretion mechanism [PDF]

, 2010
The core accretion mechanism is presently the most widely accepted cause of the formation of giant planets. For simplicity, most models presently assume that the growth of planetary embryos occurs in isolation.
A. Brunini, Adachi, Alibert, Alibert, Balbus, Benvenuto, Bodenheimer, Brunini, Chambers, Dodson-Robinson, Fortier, Fortier, Gammie, Guillot, Haisch, Hasegawa, Hayashi, Hubickyj, Ida, Ida, Inaba, Inaba, Johansen, Kokubo, Kokubo, Kokubo, Kornet, Lissauer, Lodders, Matsumura, Mayer, Militzer, Mizuno, Morbidelli, Mordasini, O. G. Benvenuto, O. M. Guilera, Ohtsuki, Ormel, Pollack, Pringle, Sano, Shakura, Shiraishi, Tanaka, Tanaka, Teiser, Thommes, Tsiganis, Wetherill, Zhou   +50 more
core   +5 more sources

Issue Information

Meteoritics &Planetary Science, Volume 61, Issue 1, Page 1-2, January 2026.
wiley   +3 more sources

Phyllosilicate Infrared Spectral Features as Tracers of Aqueous Alteration in CM Chondrites and Implications for Remote Sensing of Hydrated Asteroids

Journal of Geophysical Research: Planets, Volume 130, Issue 12, December 2025.
Abstract CM (Mighei‐type) carbonaceous chondrites host abundant OH/H2O‐bearing phyllosilicates formed from water‐rock reactions in primitive planetesimals. Their infrared (IR) spectral features resemble those of C‐type asteroids, making laboratory analyses of CMs essential for interpreting asteroid observations.
W. M. Lawrence, B. L. Ehlmann
wiley   +1 more source

Formation of the terrestrial planets in the solar system around 1 au via radial concentration of planetesimals [PDF]

, 2018
No planets exist inside the orbit of Mercury and the terrestrial planets of the solar system exhibit a localized configuration. According to thermal structure calculation of protoplanetary disks, a silicate condensation line (~ 1300 K) is located around ...
M. Ogihara, E. Kokubo, T. Suzuki, A. Morbidelli   +3 more
semanticscholar   +1 more source

Planetesimal Drift in Eccentric Disks: Possible Outward Migration

The Astrophysical Journal
Radial drift of solid particles in the protoplanetary disk is often invoked as a threat to planet formation, as it removes solid material from the disk before it can be assembled into planets.
Kedron Silsbee
doaj   +1 more source

Dynamical Stability of Polar Circumbinary Orbits and Planet Formation in the Planetary Disk of 99 Herculis

The Astronomical Journal, 2023
A possible polar-ring debris disk, the dynamics of which can be described by the outer hierarchical restricted three-body problem, has been detected in 99 Herculis.
Ying Wang, Wei Sun, Ji-lin Zhou, Ming Yang, Fu-yao Liu   +4 more
doaj   +1 more source

Evolution of Terrestrial Planetary Bodies and Implications for Habitability

Reviews of Geophysics, Volume 63, Issue 4, December 2025.
Abstract The terrestrial planetary bodies of our solar system—Mercury, Venus, Earth, and Mars—share a common origin through nebular accretion and early magma ocean differentiation, yet they diverged significantly in geological evolution, tectonic regimes, and habitability.
Peter A. Cawood, Eva E. Stüeken, Priyadarshi Chowdhury, Chris J. Hawkesworth, Jacob A. Mulder   +4 more
wiley   +1 more source