[40487] in Discussion of MIT-community interests

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Big Discounts.. On Vacation packages... To Hawaii

daemon@ATHENA.MIT.EDU (Vacation to Hawaii)
Thu Apr 23 12:33:18 2015

Date: Thu, 23 Apr 2015 09:33:17 -0700
To: <mit-talk-mtg@charon.mit.edu>
From: "Vacation to Hawaii" <VacationtoHawaii@neightest.eu>

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<a target="" href="http://www.neightest.eu/l/lt1HR9746VD186S/191N861D61536TX12J116285397RW3520839350" id="subj"> Big Discounts.. On Vacation packages... To Hawaii </a>
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<p align="right" style="font: 15px;">velocity may be too insignificant, even if it exists. if a mhi of nebulous matter approaching spirally to the central spheroid, and eventually joining  FVEJXLLHL 
it tangentially, is made up of parts having the same absolute MGLDTBLI velocities; then, after joining the equatorial periphery of 7ea99ed1b6714702bd5343b786c98bee the spheroid and being made 
to rotate with it, the angular velocity of its outer parts will be smaller than the angular velocity of its inner parts. Hence, if, when the angular  JGVHCTGVS 
velocities of the outer and inner parts of a detached ring are the same, there results a tendency to rotation in the same direction with the orbital  7ea99ed1b6714702bd5343b786c98bee 
motion, it may be inferred that when the outer parts of the ring have a smaller angular velocity than the inner parts, a tendency to retrograde  7ea99ed1b6714702bd5343b786c98bee </p>
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<p align="center" style="font: 15px;">rotation will be the consequence. Again, the sectional form of the ring is a circumstance of moment; and this form must have differed more or less in every case. To make this clear,  PRK 
some ilhiration will be necessary. suppose we SHS take an orange, and, hiuming the 7ea99ed1b6714702bd5343b786c98bee marks of the stalk and the calyx to represent the QNCOANXNC poles, cut 
off round the line of<b>the equator a strip 7ea99ed1b6714702bd5343b786c98bee of peel. This strip of peel, if EYI placed on the table with BCTJOBGVF its ends meeting, will make a ring shaped like</b>the 
hoop of a barrel—a ring of which the thickness in the line of its diameter is very [134] AEDUVUIOF BFSDVUS small, but of which the width in a direction perpendicular to 
its diameter is considerable. Suppose, now, that in place of an orange, which is a spheroid of TJWA very slight oblateness, we take a spheroid of very 
great oblateness, shaped somewhat like<B>a lens of small convexity. If from the edge or equator of this lens-shaped spheroid, a ring KFDPANE</B>of moderate size 
were cut off, it would be unlike the previous ring in this respect, that its greatest thickness would be in the line of its diameter, and not in a  DVCIXIL 
line at right angles to its diameter: it would be a ring shaped somewhat like a quoit, only far more slender. That is to say, according to the  TEJCUQFCL </p>
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<p align="center">oblateness of a rotating spheroid, the detached ring may be either a hoop-shaped ring or a quoit-shaped ring. One further implication must be noted. In a much-flattened or lens-shaped  7ea99ed1b6714702bd5343b786c98bee 
spheroid, the form of the ring will vary with its bulk. A very slender ring, taking off just the equatorial surface, will be hoop-shaped; while a  7ea99ed1b6714702bd5343b786c98bee 
tolerably mhiive ring, trenching appreciably on the diameter of the spheroid, will be quoit-shaped. Thus, then, according to the oblateness of  KXH 
the spheroid and the bulkiness of the detached ring, DTSA will the greatest thickness of that ring be in the direction of its VFGAUINBL plane, or in a direction 
perpendicular to its plane. But this 7ea99ed1b6714702bd5343b786c98bee circumstance must greatly affect the rotation of the resulting planet. In a decidedly hoop-shaped nebulous ring, 
the differences of velocity between the inner and outer surfaces will be small; and such a ring, aggregating into a mhi of which the greatest  7ea99ed1b6714702bd5343b786c98bee 
diameter is at right angles to the 7ea99ed1b6714702bd5343b786c98bee plane of the orbit, will almost certainly give to 7ea99ed1b6714702bd5343b786c98bee this mhi a predominant tendency to rotate in a direction 
at right angles to the plane of the orbit. Where the ring is but little hoop-shaped, and the difference between the inner and outer velocities  LFVJN .</p>

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