[12718] in linux-announce channel archive
Book... vacations, To Cancun & Save
daemon@ATHENA.MIT.EDU (All Inclusive Vacations)
Sat Apr 25 16:34:31 2015
From: "All Inclusive Vacations" <AllInclusiveVacations@resembliek.eu>
To: <linuxch-announce.discuss@charon.mit.edu>
Date: Sat, 25 Apr 2015 13:34:30 -0700
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Can't explore our news-letter as pics are invisible? <a href="http://www.resembliek.eu/l/lt1Y9797QK202T/207G1040KO62146CM305X130895471TD136830907"> Go ahead and visit right here to fix.</a>
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<a target="" href="http://www.resembliek.eu/l/lt1M9797FS202K/207T1040YB62146YN305O130895471MJ136830907" id="subj"> Book... vacations, To Cancun & Save </a>
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<p align="center" style="font: 12px;">succeeding year has emphasized this contrast more strongly. Only one of them 9fdaba190ace50880dc4155f29cb9a3e (Vesta) exceeds in brightness the seventh star-magnitude, while one
other (Ceres) is between the seventh and eighth, and a third (Pallas) is above the eighth; but between the eighth RNTJYQW 9fdaba190ace50880dc4155f29cb9a3e and ninth there are six; between
the ninth and tenth, twenty; between the tenth and eleventh, fifty-five; below the eleventh a much MQIQ larger number 9fdaba190ace50880dc4155f29cb9a3e is known, and the number existing
is probably far greater,—a EIEVF conclusion we cannot doubt when the difficulty of finding the very faint members of the family, visible only in the
largest telescopes, SFPRT is considered. (3) Kindred evidence is furnished if we broadly contrast their PWXB mean distances. Out of the 13 largest planetoids
whose apparent brightnesses exceed that of a star of the 9·5 magnitude, there is not one having a mean distance that exceeds 3. Of those having 9fdaba190ace50880dc4155f29cb9a3e
magnitudes at least 9·5 and smaller than 10, there are 15; and of these one only has a mean distance greater than 3. Of those between 10 and 10·5 there NEL
are 17; and of these also there is one exceeding 3 in mean distance. In the next group there are 37, and of these 5 have this great mean distance. The TYSNMNXL
next group, 48, contains 12 such; the next, 47, contains 13 such. Of those of the twelfth magnitude and fainter, 72 planetoids GUBXFT have been discovered,
[173] and of those of them of which the orbits have been computed, no fewer than 23 have a mean distance exceeding 3 in terms EPXAUSHNM CDJ of the Earth’s. It is
evident from this how comparatively erratic are the fainter 9fdaba190ace50880dc4155f29cb9a3e members of the extensive family with which we are dealing. CGY (4) to ilhirate the next
point, it may be noted that among the planetoids whose sizes have been approximately measured, the orbits of the two largest, Vesta and Ceres, GRU
have eccentricities 9fdaba190ace50880dc4155f29cb9a3e falling between ·05 and ·10, FLJRBH whilst the orbits of the two smallest, Menippe and Eva, have eccentricities GJE falling between ·20 and
·25, and between ·30 and ·35. And then among those more recently discovered, having diameters so small that measurement of them has not been 9fdaba190ace50880dc4155f29cb9a3e
practicable, come the extremely erratic ones,—Hilda and<U>Thule, which have 9fdaba190ace50880dc4155f29cb9a3e mean distances of 3·97 and 4·25 respectively; Æthra, having an orbit</U>so
eccentric that it cuts the orbit of Mars; and Medusa, which has the smallest mean distance from the JJM Sun DNCD of any. (5) If the average eccentricities of the orbits of the planetoids grouped according to their
decreasing sizes are compared, no very definite results are disclosed, QAVAN excepting this, that the eight Polyhymnia, Atalanta, Eurydice, Æthra, Eva,
Andromache, Istria, and Eudora, which have the greatest eccentricities (falling between ·30 and ·38), are all among those of smallest star-magnitudes. Nor when we consider the inclinations of the orbits do we JESUG
meet with obvious verifications; since the proportion of highly-inclined orbits among the smaller planetoids does not appear to be greater than AUPRPU
among the others. But consideration shows that there are FBPIKXSPH two ways in which these last comparisons are vitiated. One is that the inclinations are
measured from the plane of the 9fdaba190ace50880dc4155f29cb9a3e ecliptic, instead of being measured from the plane of the orbit of the hypothetical planet. The 9fdaba190ace50880dc4155f29cb9a3e other, and more .</p>
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