The origin of the solar system: The capture theory

1990 ◽  
Vol 62 (3-4) ◽  
pp. 341
Author(s):  
A.E. Roy
Keyword(s):  

Planets produced by the capture-theory model would condense into compact partially segregated bodies in a period of 10 3 –10 4 a (years). A resisting medium, which would be a byproduct of the capture process, is shown to give rounding of planetary orbits in 10 4 –10 8 a, the rounding time being dependent on planetary mass. A collision between two planets is postulated and it is shown that the larger planet could be ejected from the Solar System. The collision could also provide sufficient energy to break up the smaller planet and so to provide the material for the minor planets.


A theory of the origin of the Solar System is described which involves the capture of material from a light diffuse star which passed close to the Sun. It is shown that planetary condensations could be formed and that these would take up orbits with radii having the required range of values.


1962 ◽  
Vol 14 ◽  
pp. 149-155 ◽  
Author(s):  
E. L. Ruskol

The difference between average densities of the Moon and Earth was interpreted in the preceding report by Professor H. Urey as indicating a difference in their chemical composition. Therefore, Urey assumes the Moon's formation to have taken place far away from the Earth, under conditions differing substantially from the conditions of Earth's formation. In such a case, the Earth should have captured the Moon. As is admitted by Professor Urey himself, such a capture is a very improbable event. In addition, an assumption that the “lunar” dimensions were representative of protoplanetary bodies in the entire solar system encounters great difficulties.


1962 ◽  
Vol 14 ◽  
pp. 133-148 ◽  
Author(s):  
Harold C. Urey

During the last 10 years, the writer has presented evidence indicating that the Moon was captured by the Earth and that the large collisions with its surface occurred within a surprisingly short period of time. These observations have been a continuous preoccupation during the past years and some explanation that seemed physically possible and reasonably probable has been sought.


1962 ◽  
Vol 11 (02) ◽  
pp. 137-143
Author(s):  
M. Schwarzschild

It is perhaps one of the most important characteristics of the past decade in astronomy that the evolution of some major classes of astronomical objects has become accessible to detailed research. The theory of the evolution of individual stars has developed into a substantial body of quantitative investigations. The evolution of galaxies, particularly of our own, has clearly become a subject for serious research. Even the history of the solar system, this close-by intriguing puzzle, may soon make the transition from being a subject of speculation to being a subject of detailed study in view of the fast flow of new data obtained with new techniques, including space-craft.


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