Results 21 to 30 of about 42,393 (296)
A Consistent Model of Terrestrial Planet Magnetospheres and Rotations in Our Solar System
World Journal of Condensed Matter Physics, 2021 The Sun comprises 99.9% of the solar system mass so it is expected that Sun terrestrial planet interactions can influence the motion as well as the rotation of the terrestrial planets. Gravity affects the planet orbital motions while the changing magnetic fields of the Sun can influence the planet rotations.
F. J. Cadieu
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Dynamical Shake‐up of Planetary Systems. II.N‐Body Simulations of Solar System Terrestrial Planet Formation Induced by Secular Resonance Sweeping [PDF]
The Astrophysical Journal, 2008 To appear in ...
Edward W. Thommes +2 more
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Earth and Planetary Science Letters, 2022 Nucleosynthetic isotope signatures in meteorites provide key insights into the structure and dynamics of the solar protoplanetary disk and the accretion history of the planets. We present high-precision Zr isotopic data of a comprehensive suite of non-carbonaceous (NC) and carbonaceous (CC) meteorites, and find that various meteorite groups, including ...
Jan Render +3 more
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Comment on "Did the terrestrial planets of the Solar System form by pebble accretion?" [PDF]
Comment on arXiv:2411.09271 (slight correction to abstract here), 6 pages, 1 figure, comments and questions ...
Anders Johansen +2 more
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Observations of Locally Generated Whistler-mode Waves in the Martian Magnetotail Current Sheet
The Astrophysical Journal, 2023 The whistler-mode wave is an electromagnetic wave that commonly occurs in space plasma and has been extensively studied, especially within the Earth's magnetosphere. They have also been reported in the near-Mars space, such as Martian upstream solar wind,
Xiao Ma +6 more
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Atmosphere, 2021 Electrification represents a fundamental process in planetary atmospheres, widespread in the Solar System. The atmospheres of the terrestrial planets (Venus, Earth, and Mars) range from thin to thick are rich in heavier gases and gaseous compounds, such ...
Marija Radmilović-Radjenović +2 more
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Surrounded by Giants: Habitable Zone Stability Within the HD 141399 System
The Astronomical Journal, 2023 The search for exoplanets has revealed a diversity of planetary system architectures, the vast majority of which diverge significantly from the template of the solar system.
Stephen R. Kane
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Terrestrial planet and asteroid belt formation by Jupiter–Saturn chaotic excitation
Scientific Reports, 2023 The terrestrial planets formed by accretion of asteroid-like objects within the inner solar system’s protoplanetary disk. Previous works have found that forming a small-mass Mars requires the disk to contain little mass beyond ~ 1.5 au (i.e., the disk ...
Patryk Sofia Lykawka, Takashi Ito
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The Dynamical Consequences of a Super-Earth in the Solar System
The Planetary Science Journal, 2023 Placing the architecture of the solar system within the broader context of planetary architectures is one of the primary topics of interest within planetary science. Exoplanet discoveries have revealed a large range of system architectures, many of which
Stephen R. Kane
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