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Before proceeding to a more detailed discussion, see whatwe can conclude from the history of the discovery of the planetoids and from the data regardingsizes of those that were opened at a later time. In 1878Professor Newcomb, discussing the preponderance of the evidence in favor of the opinion,the number and size of planetoids limited, said that "the newly discoveredplanetoids do not seem to be in General much smaller open ten years agoago"; and further, that "the discovery of new planetoids, in all probability,will happen less and less, before hundreds of them will be opened." Ifwe consider the tables, namely the just-released fourththe publication "Descriptive astronomy" chambers (t I), we see that the averagethe size of the planetoid opened in 1868 (the year, was elected for Newcombcomparison), is equal to 11.56, while the average size of a planetoid,opened in 1888, equals to 12,43. Further, note that, although afteras written by Professor Newcomb, has opened more than ninety planetoid, theless new discoveries of them in any case did not become less: in 1888, wasadded to the list of ten planetoids; consequently, the number ofopened planetoids remained approximately the same as in the previousten years. So, if the instructions made by Professor Newcomb, justified,it would be possible to assume that the number of planetoids limited tootherwise we can conclude that their number is unlimited. Quitejust seems that these planetoids are considered to be not hundreds, butthousands that more powerful telescopes will continue to open stillsmaller and that the addition to the list will only end whenowing to insignificant dimensions, they will become invisible. Proceeding now to a careful assessment of the two hypotheses regarding the Genesis ofthese many bodies, I may first note that Laplace canto be, and wouldn't suggest your hypothesis, if I had known that instead of foursuch bodies there are hundreds, if not thousands. The assumption that theyoccurred due to falling of a misty ring into numerous smallpart, instead of to draw together in one mass, maybe in this casedid not seem to him so It likely would have seemed to him even lesslikely, if he knew all that since it was opened about the hugethe difference orbits according to their size, their various and often greatthe eccentricity and their diverse and often significant moodConsider these, and other of their features.
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