Results 51 to 60 of about 838,568 (119)
The Astrophysical Journal, 2023 The temperature structure of protoplanetary disks provides an important constraint on where in the disks rocky planets like our own form. Recent nonideal magnetohydrodynamical (MHD) simulations have shown that the internal Joule heating associated with ...
Katsushi Kondo +2 more
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Impact of Jupiter’s Heating and Self-shadowing on the Jovian Circumplanetary Disk Structure
The Planetary Science JournalDeciphering the structure of the circumplanetary disk (CPD) that surrounded Jupiter at the end of its formation is key to understanding how the Galilean moons formed.
Antoine Schneeberger, Olivier Mousis
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The Early Solar System - Chapter 6 [PDF]
, 2010 This chapter presents a (partial) review of the information we can derive on the early history of the Solar System from radioactive nuclei of very different half-life, which were recognized to have been present alive in pristine solids. In fact, radioactivities open for us a unique window on the evolution of the solar nebula and provide tools for ...
arxiv +1 more source
Evolution of the Early Solar System in Terms of Big History and Universal Evolution
Journal of Big History, 2018 The present contribution is devoted to some aspects of history and evolution of the early Solar system. The origin of the Sun, Earth, other planets and its satellites has long been a matter of great concern for people.
Leonid Grinin
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Solar System Formation in the Context of Extra-Solar Planets [PDF]
, 2018 Exoplanet surveys have confirmed one of humanity's (and all teenagers') worst fears: we are weird. If our Solar System were observed with present-day Earth technology -- to put our system and exoplanets on the same footing -- Jupiter is the only planet that would be detectable. The statistics of exo-Jupiters indicate that the Solar System is unusual at
arxiv +1 more source
The Astrophysical JournalFor the origin of the radially concentrated solar system’s terrestrial planets, planet formation from a ring of solids at about 1 au from the Sun with convergent/suppressed type I migration is preferred.
Masahiro Ogihara +2 more
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Accretion and Uneven Depletion of the Main Asteroid Belt
The Planetary Science JournalThe main asteroid belt (MAB) is known to be primarily composed of objects from two distinct taxonomic classes, generically defined here as S- and C-complex.
Rogerio Deienno +5 more
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THE PHYSICAL MEANING OF THE TITIUS-BODE FORMULA
Odessa Astronomical Publications, 2016 It is proposed an special hypothesis of the formation of symmetric objects in space with the help of the interference of standing waves which act in the process of evolution of the primordial gas-dust cloud including the formation of the Solar system ...
V. A. Smirnov
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Solar System Processes Underlying Planetary Formation, Geodynamics, and the Georeactor [PDF]
arXiv, 2006 Only three processes, operant during the formation of the Solar System, are responsible for the diversity of matter in the Solar System and are directly responsible for planetary internal-structures, including planetocentric nuclear fission reactors, and for dynamical processes, including and especially, geodynamics.
arxiv
Life, 2014 The asteroid (4) Vesta, parent body of the Howardite-Eucrite-Diogenite meteorites, is one of the first bodies that formed, mostly from volatile-depleted material, in the Solar System. The Dawn mission recently provided evidence that hydrated material was
Diego Turrini, Vladimir Svetsov
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