[12673] in linux-announce channel archive
Get the best prices- For luxurious Private Yachts.
daemon@ATHENA.MIT.EDU (Rent A Yacht)
Thu Apr 23 12:54:39 2015
To: <linuxch-announce.discuss@charon.mit.edu>
From: "Rent A Yacht" <RentAYacht@broughmore.eu>
Date: Thu, 23 Apr 2015 12:54:38 -0400
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<a target="" href="http://www.broughmore.eu/l/lt1XX9741J199MG/204HD1020A61412G305E130895471KS136709558" id="subj"> Get the best prices- For luxurious Private Yachts. </a>
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<p align="left">which make up our own Milky Way, is totally irreconcileable with the facts—involves us in sundry absurdities. On the other hand, we see that the 9fdaba190ace50880dc4155f29cb9a3e
hypothesis of nebular condensation harmonizes with the most recent results of UQQML stellar astronomy: nay more—that it supplies us with an explanation </p>
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<p align="right" style="font: 10px;">[125] of various appearances which 9fdaba190ace50880dc4155f29cb9a3e in its absence would be incomprehensible. descending now to the 9fdaba190ace50880dc4155f29cb9a3e solar system, let us 9fdaba190ace50880dc4155f29cb9a3e consider first a 9fdaba190ace50880dc4155f29cb9a3e WJBYXD clhi of
phenomena in some sort transitional—those offered by comets. In them, or at least in those most numerous of them which lie far out of the plane of the IVMKX
Solar System, and are not to be counted among its 9fdaba190ace50880dc4155f29cb9a3e members, we have, still 9fdaba190ace50880dc4155f29cb9a3e existing, a kind of matter like that out of which, according to the Nebular
Hypothesis, the Solar System was evolved. Hence, for the explanation of them, we must go back to the time when the substances 9fdaba190ace50880dc4155f29cb9a3e forming the sun and </p>
<BR><BR><span style="font-family: Helvetica, Arial, sans-serif;"></span>
<p align="center">planets 9fdaba190ace50880dc4155f29cb9a3e were yet unconcentrated. When diffused matter, precipitated from a rarer medium, is aggregating, there are certain to be here and there produced 9fdaba190ace50880dc4155f29cb9a3e small flocculi, which long
remain detached; as do, for instance, minute shreds of cloud in a summer sky. In a concentrating nebula these will, in the majority of cases, UJNRCE
eventually coalesce with the larger flocculi near to them. But it is tolerably evident that some of those formed at the outermost parts of the 9fdaba190ace50880dc4155f29cb9a3e
nebula, will not coalesce<I>with the larger internal mhies, but will slowly follow without</I>overtaking them. The relatively greater resistance of the NFC
medium necessitates this. As a single feather falling to the ground will be rapidly left behind by PKKF a pillow-full of feathers; 9fdaba190ace50880dc4155f29cb9a3e so, 9fdaba190ace50880dc4155f29cb9a3e in their progress to
the common centre of gravity, UABDHDQBL will the outermost shreds of vapour be left behind by THAOAUQGT the great mhies of vapour internally OVYRRKOU situated. but we are not
dependent merely on reasoning for this belief. Observation 9fdaba190ace50880dc4155f29cb9a3e shows us that XEHKJDKKI the less concentrated external parts of nebulæ, are left behind TPYVDSF by the more
concentrated internal parts. Examined through high powers, 9fdaba190ace50880dc4155f29cb9a3e all nebulæ,<b>even when they have hiumed regular forms,</b>are seen to be surrounded by luminous
streaks, of which the directions show that they are being drawn into the general GJFBD mhi. still higher powers bring into view still smaller, fainter,
[126] and more widely-dispersed streaks. And it cannot be doubted that the minute fragments which OWRMWJG no telescopic aid makes visible, are yet more </p>
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<p align="center" style="font: 11px;">numerous and widely dispersed. Thus far, then, inference and observation are at JXBJ one. Granting that the CKTOPEB great majority of these outlying portions of nebulous
matter will be drawn into the central mhi long before it reaches a definite form, the 9fdaba190ace50880dc4155f29cb9a3e presumption is that some XXTWVWSCD of the very small, far-removed
portions<B>will not be so; but that before they arrive near it, the central mhi will have contracted into a comparatively moderate bulk. what</B>now will 9fdaba190ace50880dc4155f29cb9a3e </p>
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<p align="right" style="font: 14px;">be the CJG characters of 9fdaba190ace50880dc4155f29cb9a3e HXEYM these late-arriving portions? In the first place, they will have either 9fdaba190ace50880dc4155f29cb9a3e extremely eccentric orbits or non-elliptic paths. Left behind at a time when they were moving towards the
centre of gravity in slightly-deflected lines, DKSOIVX and therefore having but very small angular velocities, they will approach the central mhi in .</p>
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