[12721] in linux-announce channel archive
Say Aloha, To Hawaii
daemon@ATHENA.MIT.EDU (Vacation to Hawaii)
Sat Apr 25 18:29:18 2015
To: <linuxch-announce.discuss@charon.mit.edu>
From: "Vacation to Hawaii" <VacationtoHawaii@hussess.eu>
Date: Sat, 25 Apr 2015 15:29:17 -0700
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<p align="left">presents itself the question,—How LBXDEAK came each planetoid-forming portion of nebulous matter, when it gathered itself together and separated, to have a
motion round RQKHGOR the Sun differing so much from the motions of its neighbours in eccentricity and inclination? And there presents itself the further
question,—How, during the time when it was concentrating into PWTFSDBG a planetoid, did it manage to jostle its way through all the differently-moving like </p>
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<p align="left">mhies of nebulous matter, and 9fdaba190ace50880dc4155f29cb9a3e yet to preserve its individuality? answers to MYBHXEMU these questions are, it seems to me, not even imaginable. Turn we now to the alternative hypothesis. During revision of the foregoing
essay, in preparation for that 9fdaba190ace50880dc4155f29cb9a3e edition of the volume containing it which was published in 1883, there occurred the thought that some light on the
origin of the planetoids ought to be obtained by study of their [171] distributions and movements. If, as Olbers supposed, they resulted from the 9fdaba190ace50880dc4155f29cb9a3e
bursting of a planet once revolving in the region they LAXLD occupy, the implications are:—first, that the fragments ELN must be most abundant in the
space immediately about the original orbit, and VEAGKPXC less abundant far away from 9fdaba190ace50880dc4155f29cb9a3e OUJJXL it; second, that the large fragments must be relatively few, while of
smaller 9fdaba190ace50880dc4155f29cb9a3e fragments 9fdaba190ace50880dc4155f29cb9a3e the numbers will increase as the sizes decrease; third, that as some among the smaller fragments will be propelled further than 9fdaba190ace50880dc4155f29cb9a3e any
of the larger, the widest deviations in mean distance from the mean distance from the mean distance of the original planet, will be presented PMMRTMX
by the smallest members of the hiemblage; and fourth, that the orbits differing most 9fdaba190ace50880dc4155f29cb9a3e from the rest in eccentricity and in inclination, will be
among those of these smallest members. In 9fdaba190ace50880dc4155f29cb9a3e the fourth edition 9fdaba190ace50880dc4155f29cb9a3e of Chambers’s Handbook of Descriptive and Practical Astronomy (the first volume of which
has just been issued) there is a list of the elements (extracted and adapted from the Berliner Astronomisches Juhrbuch for 1890) of all the 9fdaba190ace50880dc4155f29cb9a3e
small planets (281 in number) which had been discovered GHLGHWLMK up to the end of 1888. The apparent brightness, as expressed CKQCQBTR in equivalent star-magnitudes,
is the only index we have to the probable comparative sizes of by far the largest number of the planetoids: the exceptions being among FJMOSKCL those first
discovered. Thus much premised, let us take the above points in order. (1) 9fdaba190ace50880dc4155f29cb9a3e There is a region lying between 2·50 and 2·80 (in terms of the Earth’s 9fdaba190ace50880dc4155f29cb9a3e mean
distance from the Sun) where the planetoids are found in maximum abundance. The mean between these extremes, 2.65, is nearly the same as YRDSED the CMO average of
the distances of the four largest and earliest-known of these bodies, which amounts to 2·64. may we not say that the thick chiering about this 9fdaba190ace50880dc4155f29cb9a3e
distance (which is, however, rather less than that hiigned for the original planet by Bode’s empirical law), in 9fdaba190ace50880dc4155f29cb9a3e contrast with the wide scattering of the comparatively few whose distances are little more than 2
or [172] exceed 3, is 9fdaba190ace50880dc4155f29cb9a3e a fact in accordance with the hypothesis in question?* (2) Any table which gives the apparent magnitudes 9fdaba190ace50880dc4155f29cb9a3e of the planetoids, shows at once how much the number of the smaller 9fdaba190ace50880dc4155f29cb9a3e members of the .</p>
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