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- W2158102854 abstract "The study of creation and evolution of celestial bodies and their systems is one of the main subjects in astrophysics, cosmogony and cosmology. It is known from observation that the matter of the Solar System bodies is very identical with respect to its substantial and chemical content and from this point of view all the bodies are of common origin. But the attempts to find general mechanism of creation of the bodies encounter irresistible contradiction. The point is that the planets having only ~0.015% of the system’s mass possess 98% of the orbital angular momentum. At the same time ~99.85% of the Sun’s masses produce no sooner than 2% of the moment of momentum which, in both cases, is accepted to be a conservative parameter. Also, the specific (for unit of the mass) orbital angular momentum is increased with the distance from the Sun. These results follow from the problem solution based on the hydrostatic approach." @default.
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- W2158102854 date "2011-01-01" @default.
- W2158102854 modified "2023-09-24" @default.
- W2158102854 title "Creation and Evolution of the Solar System Bodies" @default.
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- W2158102854 doi "https://doi.org/10.1007/978-94-007-0498-5_8" @default.
- W2158102854 hasPublicationYear "2011" @default.
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