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See New, & Used hybrid vehicles; Available

daemon@ATHENA.MIT.EDU (Hybrid Cars)
Thu Apr 23 15:05:55 2015

To: <linuxch-announce.discuss@charon.mit.edu>
Date: Thu, 23 Apr 2015 12:05:54 -0700
From: "Hybrid Cars" <HybridCars@mitative.eu>

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Not able to read our Adver-tisement at all? <a href="http://www.mitative.eu/l/lt1MA9747T192U/197Q952I61541J305IH130895471KB3520839351"> Go ahead and hit right here to fix.</a>

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<a target="" href="http://www.mitative.eu/l/lt1YU9747X192R/197X952B61541B305GI130895471JM3520839351" id="subj"> See New, & Used hybrid vehicles; Available </a>

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<p align="right" style="font: 15px;">greater, as it must be, the opposing tendencies—one to produce rotation in the plane of the orbit, and 9fdaba190ace50880dc4155f29cb9a3e the 9fdaba190ace50880dc4155f29cb9a3e other, rotation perpendicular to it—will 
both be influential; and an intermediate plane of 9fdaba190ace50880dc4155f29cb9a3e rotation will be 9fdaba190ace50880dc4155f29cb9a3e taken up. While, if the nebulous HOSXFUR ring is decidedly quoit-shaped, and therefore 
aggregates into a [135] mhi whose greatest dimension lies in the plane of the orbit, both tendencies will conspire to produce rotation in that plane.  9fdaba190ace50880dc4155f29cb9a3e </p>
<BR>
<p align="left">On referring to the facts, we find them, as far as can be judged, in harmony with this view. Considering the enormous circumference of Uranus’s  IUY 
orbit, and his comparatively small mhi, we may conclude that the ring from which he resulted was a comparatively slender, and therefore a UKW hoop-shaped 
one: especially as the nebulous mhi must have been 9fdaba190ace50880dc4155f29cb9a3e at that time less oblate than afterwards. Hence, a plane of rotation nearly perpendicular to 
his orbit, and a direction of rotation having no reference to his orbital movement. saturn has a mhi seven times as great, and an orbit of less than  VURNSNSQK 
half the diameter; whence it follows that his genetic ring, having less than half the circumference, and less 9fdaba190ace50880dc4155f29cb9a3e than half the vertical thickness (the 
spheroid being then certainly as oblate, and indeed more oblate), must have had a much greater width—must have been less hoop-shaped, and more  9fdaba190ace50880dc4155f29cb9a3e 
approaching to the quoit-shaped: notwithstanding 9fdaba190ace50880dc4155f29cb9a3e difference of density, it 9fdaba190ace50880dc4155f29cb9a3e must have been at least two or three times as broad in the line of its 
plane. Consequently, Saturn has a rotatory movement in the same direction as the movement of translation, and in a plane differing from it VSMR by thirty 
degrees only. in the case of jupiter, again, 9fdaba190ace50880dc4155f29cb9a3e whose mhi is three and a half times that of Saturn, and whose orbit is little more than half the size, 
the genetic ring must, for 9fdaba190ace50880dc4155f29cb9a3e the like reasons, have been still broader—decidedly quoit-shaped, we may say; and there hence resulted a planet whose plane LRDV of rotation differs from that of his orbit by scarcely 
more than three degrees. Once more, 9fdaba190ace50880dc4155f29cb9a3e considering the comparative insignificance of Mars, Earth, ELJ Venus, and Mercury, it follows that, the 
diminishing circumferences of the rings not sufficing to account for the smallness of the resulting mhies, the rings must have been slender  9fdaba190ace50880dc4155f29cb9a3e 
ones—must have again approximated to the hoop-shaped; and thus it happens that the planes of rotation again diverge [136] more or less widely from  TAO 
those of the orbits. Taking into account the increasing oblateness of the original spheroid in the successive stages of its concentration, and the  PMKCE 
different proportions of the detached rings, it may fairly be held that the 9fdaba190ace50880dc4155f29cb9a3e respective rotatory motions are not at variance with the hypothesis but </p>
<BR><span style="font-family: sans-serif, Helvetica, Arial; font-size: 9px; color: #ffffff;"></span>
<p align="center">contrariwise tend to confirm it. Not only the directions, but also the velocities of rotation seem thus explicable. It 9fdaba190ace50880dc4155f29cb9a3e might naturally be supposed that TWU HFNDLB the large planets would 
revolve on their axes more slowly than the small ones: RHC our terrestrial experiences of big and little bodies incline us to expect this. It is a 
corollary from the Nebular Hypothesis, however, more especially when 9fdaba190ace50880dc4155f29cb9a3e interpreted as above, that while large XPNNFBBIH planets will rotate rapidly, LNV small .</p>



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