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So, returning to the misty ring, weask and sometimes how it happened that each part is vaguematter which gave rise to a separate planetoid sgustilis and then separated,got movement around the Sun is so characterized by its eccentricity andinclination from the movements of their neighbors? Then is still the question of howmanaged this part of the misty ring uplotnitelya in planetoid,to fight their way through all the differently-moving like masses of nebulousmatter and keep their individuality? It seems to me that you can not evenimagine the answer to these questions. We now turn to another hypothesis.In a revision of the previous experience and prepare for the new editionpublished in the 1883 volume, which placed this experience, I was struck by the idea thatthe study of distributions and movements of the planetoids must have some understanding of themorigin. If, as suggested by Olbers, they were due to ruptureplanets, when rotating in the area occupied by them nowthe conclusion will be as follows. First, the fragments should be more abundant inthe space closest to the initial orbit of the planet itself, and lessrich far from it. Second, large fragments should berelatively few, while the number of small fragments should be increased bydecreasing their size; third, as some of the smaller pieceshad to be thrown farther than large, the greatest evasion inaverage distance from average distance of the original planet will bethe smallest members of that cluster, and, fourth, most of these smallmembers will have orbits that differ from the rest in eccentricity andinclination. In the fourth edition of the writings of chambers "Guidedescriptive and practical astronomy" (the first volume of which has only recentlywas released) is a list of items (taken from the BerlinAstronomical year-book for 1890 ), all the small planets (number 281),which were opened before the end of 1888 the Visible luminosity, expressedtheir respective values, is the only indicationlikely comparative size of great majority of planetoidsthe only exceptions are some of the first open planetoids.
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