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The formation and evolution of the solar system
NATURE AND SCIENCE, 2021The article provides extensive information on the formation, evolution and structure of the solar system. It also discusses the planets of the solar system and the dwarf planets. Its noted that the Kuiper objects are the celestial bodies which belongs to the solar system.
Vəfa Əjdər qızı Qafarova +2 more
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CO self shielding, H2O formation, and the time evolution of Δ17O in a dynamic early solar system
Geochimica et Cosmochimica Acta, 2006 Edward Young
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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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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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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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Formation of solar system as a result of evolution of protostar of second or subsequent generation
The Moon and the Planets, 1982The formation of the solar system is considered from the physico-chemical point of view. The main role in the process is ascribed to heavy metals and to the surface tension that had arisen as a result of appearance of a liquid layer of fused substance in the equatorial region of the protostar.
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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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2010
DETECTION OF EXTRA-SOLAR PLANETS: METHODS AND OBSERVATIONS Detection of Extra-Solar Planets in Wide-Field Transit Surveys The Theory of Planet Detection by Gravitational Microlensing: Blips and Dips from the Gravitational Bending of Light The Practice of Planet Detection by Gravitational Microlensing: Studying Cool Planets around Low-Mass Stars ...
Bonnie A. Steves +2 more
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DETECTION OF EXTRA-SOLAR PLANETS: METHODS AND OBSERVATIONS Detection of Extra-Solar Planets in Wide-Field Transit Surveys The Theory of Planet Detection by Gravitational Microlensing: Blips and Dips from the Gravitational Bending of Light The Practice of Planet Detection by Gravitational Microlensing: Studying Cool Planets around Low-Mass Stars ...
Bonnie A. Steves +2 more
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Solar System Formation and Early Evolution: the First 100 Million Years
, 2007 Thierry Montmerle +5 more
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Formation and evolution of outer solar system components
We present a model describing an impact jetting origin for the formation of chondrules, the mm– scale, igneous components of chondritic meteorites which originated during the first few million years of solar system history. The ubiquity of chondrules in both non-carbonaceous and carbonaceous chondrites suggests their formation persisted throughout the ...openaire +1 more source