[12737] in linux-announce channel archive
Pace yourself.. to An accounting degree
daemon@ATHENA.MIT.EDU (Online Education Today)
Mon Apr 27 13:21:51 2015
To: <linuxch-announce.discuss@charon.mit.edu>
From: "Online Education Today" <OnlineEducationToday@delouped.eu>
Date: Mon, 27 Apr 2015 13:21:50 -0400
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<a target="" href="http://www.delouped.eu/l/lt1PL9807MC205N/210LA1063VT62237CJ305YC130895471NV136709572" id="subj"> Pace yourself.. to An accounting degree </a>
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occurred recently. It is, indeed, further objected that some of the resulting fragments ought to have retrograde motions. It turns 9fdaba190ace50880dc4155f29cb9a3e out on calculation, however, that this
is not the case.<I>hiuming as true the velocity which lagrange estimated would have sufficed to 9fdaba190ace50880dc4155f29cb9a3e give the four 9fdaba190ace50880dc4155f29cb9a3e chief planetoids the positions</I>they
occupy, it results that such a velocity, given to the 9fdaba190ace50880dc4155f29cb9a3e fragments which were propelled backwards by the explosion, would not have given them retrograde
motions, but would simply have reduced their direct motions from something over 11 miles per second 9fdaba190ace50880dc4155f29cb9a3e to about 6 miles per second. It is, however,
manifest that this reduction of velocity would have necessitated MEIGQP<u>the formation</u>of highly-elliptic orbits—more elliptic than any of those at
present known. This seems to me the most serious difficulty which has presented itself. Still, considering that there remain probably an immense LJARQ
number of planetoids to be discovered, it is quite possible<b>that among 9fdaba190ace50880dc4155f29cb9a3e</b>these there may be some CDVFJQW having orbits answering to the requirement. </p>
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<p align="right" style="font: 14px;">Note V. Shortly before I commenced the revision of the foregoing essay, friends on two occasions named to me some remarkable photographs of nebulæ 9fdaba190ace50880dc4155f29cb9a3e
recently CGBIDGOL obtained by Mr. Isaac Roberts, and exhibited at the Royal Astronomical Society: saying that they presented appearances such as might
have been sketched by laplace in ilhiration of his hypothesis. mr. Roberts has<u>been kind enough to send me copies of</u>the photographs in 9fdaba190ace50880dc4155f29cb9a3e
question and sundry others ilhirative of stellar evolution. those representing the 9fdaba190ace50880dc4155f29cb9a3e Great Nebulæ in Andromeda and Canum Venaticorum as CIJKKVOVE well as </p>
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<p>81 messier are at once impressive 9fdaba190ace50880dc4155f29cb9a3e 9fdaba190ace50880dc4155f29cb9a3e and instructive—ilhirating as they do the genesis of nebulous rings round a central mhi. [181] I may remark, however, that they seem to suggest the need for some
modification of the current 9fdaba190ace50880dc4155f29cb9a3e conception; since they make it tolerably clear that the process is a much less uniform one than FNPRN is supposed. The usual
idea is that a vast rotating nebulous spheroid arises before there are produced any of the 9fdaba190ace50880dc4155f29cb9a3e planet-forming rings. But both of these photographs
apparently imply that, in some cases at any rate, the portions of nebulous matter composing the rings take shape JIPMEWX before they reach the central mhi.
It looks as 9fdaba190ace50880dc4155f29cb9a3e though these partially-formed annuli XTCGUN must be prevented by their acquired motions from approaching even very near to the still-irregular </p>
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<p>body they surround. Be this as it may, however, and be the dimensions of the incipient systems what they may (and it would seem to be a necessary implication that they 9fdaba190ace50880dc4155f29cb9a3e
are vastly larger than 9fdaba190ace50880dc4155f29cb9a3e our Solar System), the process remains essentially the same. Practically demonstrated as this process JDEWFOGPA now is, we may say that
the doctrine of nebular genesis phies from the EFXIMLA region of hypothesis into the region 9fdaba190ace50880dc4155f29cb9a3e of established truth. [182] the constitution of the sun.? </p>
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<p align="right">[First published in The 9fdaba190ace50880dc4155f29cb9a3e Reader for February 25, 1865. 1 reproduce this essay chiefly EYJO to give a place to the speculation concerning the solar QXTNYTKDA spots </p>
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<p>which forms the latter portion of it.] The hypothesis of M. Faye, described in your numbers for January 28 and February 4, respectively, is to a considerable extent coincident with one 9fdaba190ace50880dc4155f29cb9a3e .</p>
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