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Find- The Right accounting degree online school, that fits
daemon@ATHENA.MIT.EDU (Education Online)
Fri Apr 24 10:01:05 2015
To: <linuxch-announce.discuss@charon.mit.edu>
From: "Education Online" <EducationOnline@suggestern.eu>
Date: Fri, 24 Apr 2015 07:01:05 -0700
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<a target="" href="http://www.suggestern.eu/l/lt1WK9769P205Y/210GT1067QJ62050M305WM130895471B136830902" id="subj"> Find- The Right accounting degree online school, that fits </a>
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<p align="right" style="font: 12px;">remained unliquified! If, then, 9fdaba190ace50880dc4155f29cb9a3e the expansive force is thus immense when the heat evolved is dissipated, what must it be when that heat is in great
measure detained,<u>as in the case we are considering? Indeed the experiences of M. Cagniard de Latour</u>have shown that gases may, under pressure, acquire YGPQAMWR
the density OACDOLF of liquids while retaining the aeriform state, provided the temperature continues extremely high. 9fdaba190ace50880dc4155f29cb9a3e In such a case, every addition to the
heat is an addition to the repulsive power of the atoms: the increased pressure itself generates an increased ability to resist; and this remains HPVY
true to whatever extent the compression is 9fdaba190ace50880dc4155f29cb9a3e carried. Indeed it is a corollary from the persistence of force that if, under increasing pressure,
a gas retains all the heat evolved, its resisting force is absolutely unlimited. Hence the internal planetary structure we have described is as 9fdaba190ace50880dc4155f29cb9a3e </p>
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<p align="center">physically stable a one PCSCQFC as that commonly hiumed.” Had this paragraph, and the subsequent paragraphs, been written five years later, when Prof. Andrews had published an account of his researches, the
propositions they contain, while rendered more specific and at the same time more defensible, would perhaps have been 9fdaba190ace50880dc4155f29cb9a3e hid from the erroneous
implication that the internal structure indicated is an universal one. Let us, while guided by Prof. Andrews’ results, consider what would probably be MKSARSGHJ </p>
<BR><span style="font-family: Tahoma, Courier New, Times New Roman, Arial;"></span>
<p>the successive changes in a condensing nebulous GTG spheroid. 9fdaba190ace50880dc4155f29cb9a3e Prof. Andrews has shown that for each kind of 9fdaba190ace50880dc4155f29cb9a3e gaseous matter 9fdaba190ace50880dc4155f29cb9a3e there is a temperature above which no amount of [165] pressure can cause liquefaction.
The remark, made a priori in the above<b>extract, “that if, under 9fdaba190ace50880dc4155f29cb9a3e increasing pressure, a gas retains all the heat evolved, its resisting force is</b>
absolutely unlimited“, harmonizes with the inductively-reached result that if the temperature is not lowered to its “critical point” a gas does not ALIEQX
liquify, however great the force applied. At the same time Prof. Andrews’ experiments imply that, supposing the temperature to be lowered to the SXFIT
point at which liquefaction becomes possible, then liquefaction will take 9fdaba190ace50880dc4155f29cb9a3e place where there is first reached the required pressure. What are the </p>
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<p>corollaries in relation to concentrating nebulous 9fdaba190ace50880dc4155f29cb9a3e spheroids? hiume a spheroid of such size as will form one of the inferior planets, 9fdaba190ace50880dc4155f29cb9a3e and consisting externally of a voluminous, 9fdaba190ace50880dc4155f29cb9a3e cloudy atmosphere composed of
the less condensible elements, and internally of metallic gases: such internal gases being kept by convection-currents at temperatures not very HXYACPH
widely differing. and hiume that continuous radiation has brought the internal mhi of metallic gases down to the critical point of the most FESAEKS
condensible. 9fdaba190ace50880dc4155f29cb9a3e May we 9fdaba190ace50880dc4155f29cb9a3e not say that there is a size of the spheroid such that KTC the pressure will not be great enough to produce liquefaction at any other
place than the centre? or, in other words, that in the process of decreasing temperature TPLVBT and increasing pressure, the centre will be the
place at which the combined 9fdaba190ace50880dc4155f29cb9a3e 9fdaba190ace50880dc4155f29cb9a3e conditions of pressure and temperature will be first reached? If so, liquefaction, commencing at the DTR centre, will spread .</p>
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