Results 251 to 260 of about 320,575 (284)
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Icarus, 1998
Abstract Water is important in the solar nebula both because it is extremely abundant and because it condenses out at 5 AU, allowing all three phases of H 2 O to play a role in the composition and evolution of the Solar System. In this paper, we undertake a thorough examination of and model the inward radial drift of ice particles from 5 AU.
Kimberly E. Cyr +2 more
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Abstract Water is important in the solar nebula both because it is extremely abundant and because it condenses out at 5 AU, allowing all three phases of H 2 O to play a role in the composition and evolution of the Solar System. In this paper, we undertake a thorough examination of and model the inward radial drift of ice particles from 5 AU.
Kimberly E. Cyr +2 more
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On the thickness and evolution of the dust layer during the formation of the solar system
Chinese Astronomy and Astrophysics, 1984Abstract We discuss certain dynamical processes during the final stage of the sinking of the dust layer. We supposed that turbulance gave rise to a state of slow sinking (quasi-equilibrium) and evaluated the critical thickness at the onset of gravitational instability in the radial direction.
Yue Zeng-yuan, Zhang Bin
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The formation and evolution of the Solar System
European Review, 2002Astronomers have built the main components of a scenario for the formation of the Solar System. Small planetary bodies accreted others by collisions within a rotating protoplanetary disk that formed at the same time as the Sun. While terrestrial planets near the warming Sun could accumulate only solid metallic and silicate material, the giant planets ...
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The Formation and Evolution of the Solar System
2018The formation and evolution of our solar system (and planetary systems around other stars) are among the most challenging and intriguing fields of modern science. As the product of a long history of cosmic matter evolution, this important branch of astrophysics is referred to as stellar-planetary cosmogony.
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Moscow University Physics Bulletin, 2014
In the present paper, the early evolution of the Solar System with regard to the process of the formation and mass growth of small bodies in protoplanetary rings is considered. This process is modeled with the use of the results that were obtained in the analysis of the libration motions of asteroids.
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In the present paper, the early evolution of the Solar System with regard to the process of the formation and mass growth of small bodies in protoplanetary rings is considered. This process is modeled with the use of the results that were obtained in the analysis of the libration motions of asteroids.
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Contemporary Physics, 2012
Extra-Solar Planets: The Detection, Formation, Evolution and Dynamics of Planetary Systems, edited by Bonnie Steves, Martin Hendry and Andrew C.
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Extra-Solar Planets: The Detection, Formation, Evolution and Dynamics of Planetary Systems, edited by Bonnie Steves, Martin Hendry and Andrew C.
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The Formation and Evolution of Planetary Systems: placing our Solar System in context
2006Jeroen Bouwman +5 more
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Beyond horizontal gene transfer: the role of plasmids in bacterial evolution
Nature Reviews Microbiology, 2021Jerónimo Rodríguez-Beltrán +2 more
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