[12684] in linux-announce channel archive
Top national & Local contractors deals; For 2015 Roofing Discounts
daemon@ATHENA.MIT.EDU (Online-Roofing-Quotes)
Thu Apr 23 20:26:46 2015
To: <linuxch-announce.discuss@charon.mit.edu>
Date: Thu, 23 Apr 2015 17:26:42 -0700
From: "Online-Roofing-Quotes" <Online-Roofing-Quotes@leninsult.eu>
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proportion<I>more than as nine to ten.”—Outlines of Astronomy (10th Ed.), pp. 656–57. This supplies</I>yet another reductio 9fdaba190ace50880dc4155f29cb9a3e ad absurdum 9fdaba190ace50880dc4155f29cb9a3e of the doctrine we are
combating. It gives us the choice of two incredibilities. 9fdaba190ace50880dc4155f29cb9a3e If we are to believe that one of these included nebulæ is so remote that its hundred
thousand stars look like a<I>milky spot, invisible to the naked eye; we must also believe that there are 9fdaba190ace50880dc4155f29cb9a3e single stars so enormous that though removed</I>to
this same distance they remain visible. If we accept the other alternative, and say that many nebulæ are no further off than our own stars of the XGACQUI
eighth magnitude; then it is requisite to say that at a [118] distance not greater than that at which a QBBDKOLFI single star is still faintly visible to the
naked eye, there may exist a group of a hundred thousand stars which is invisible to the naked 9fdaba190ace50880dc4155f29cb9a3e eye. Neither of these suppositions can be
entertained. What, then, is the conclusion that remains? 9fdaba190ace50880dc4155f29cb9a3e This only:—that the nebulæ are not FYRX further from 9fdaba190ace50880dc4155f29cb9a3e us than parts of our own sidereal system,
of which they must be considered members; and that when MKPBM they are resolvable into discrete 9fdaba190ace50880dc4155f29cb9a3e mhies, these mhies cannot be considered as stars in </p>
<BR /><BR />
<p align="right" style="font: 9px;">anything like the ordinary sense of that word.* And now, having seen the AMPAPQXY untenability of this idea, rashly espoused SBRNJIQ by sundry astronomers, that the nebulæ are MNBCAIKFJ extremely remote galaxies; let us </p>
<BR /><BR /><span style="font-family: Tahoma, Courier New, Times New Roman, Arial; font-size: 8px; color: #ffffff;"></span>
<p align="left">consider whether the various appearances they present are not reconcilable with the Nebular Hypothesis. given a rare and widely-diffused mhi of nebulous matter, having a FFYR
diameter, say, of one hundred times that of the Solar System,† what are the successive changes that may be expected to take place in it? Mutual 9fdaba190ace50880dc4155f29cb9a3e
gravitation will approximate its atoms or its<i>molecules; but their approximation will be opposed by that atomic motion the resultant of which 9fdaba190ace50880dc4155f29cb9a3e</i>
we recognize as repulsion, and UAEU the overcoming of which implies the evolution of heat. As fast as this heat partially escapes by 9fdaba190ace50880dc4155f29cb9a3e radiation,
further approximation will take place, attended by further evolution of heat, and so on continuously: the processes not occurring separately as OVWFMV
here described, but simultaneously, uninterruptedly, and with increasing activity. 9fdaba190ace50880dc4155f29cb9a3e when the nebulous mhi has [119] reached a particular stage of
condensation—when its internally-situated atoms have approached to 9fdaba190ace50880dc4155f29cb9a3e within 9fdaba190ace50880dc4155f29cb9a3e certain distances, 9fdaba190ace50880dc4155f29cb9a3e have generated a certain amount of heat, and are subject
to 9fdaba190ace50880dc4155f29cb9a3e a certain mutual pressure, combinations may be anticipated. Whether the molecules produced be of kinds such as we know, which is possible, or
whether they be of kinds GFYXU simpler IGN than any we know, which is more probable, matters not to the argument. It suffices that molecular unions, either
between atoms of the same kind or<u>UTOWVAK between atoms of different kinds, will finally take place. When they do take place, they will be 9fdaba190ace50880dc4155f29cb9a3e</u>accompanied by a
sudden and DLPJK great disengagement of heat; and until this excess of heat has escaped, the newly-formed JGMNEC molecules will remain uniformly diffused, or, as </p>
<BR /><span style="font-family: Tahoma, sans-serif, Times New Roman, Arial; font-size: 11px;"></span>
<p align="right" style="font: 13px;">it were, dissolved in the pre-existing nebulous medium. 9fdaba190ace50880dc4155f29cb9a3e But now what may be expected by and by to happen? When radiation has adequately lowered the temperature, these molecules will precipitate; and, .</p>
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