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The Astrology of Space - Matrix Software

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<strong>The</strong> <strong>Astrology</strong> <strong>of</strong> <strong>Space</strong><br />

Direction <strong>of</strong> Motion <strong>of</strong> the Galaxy<br />

R.A. Decl. Long Lat MC L2 B2<br />

063 00 14 +35 26 11 067 35 13 +14 04 05 064 56 59 163 00 00 -11 00 00<br />

<strong>The</strong> direction <strong>of</strong> this motion is approximately at a right<br />

angle to the direction <strong>of</strong> the center <strong>of</strong> the local<br />

supercluster, the Virgo Cluster. A question<br />

astronomers are attempting to decide is: is the local<br />

supercluster rotating, and are we orbiting the Virgo<br />

cluster? We cannot be in a bound Keplerian-type <strong>of</strong><br />

orbit, for at our present distance from the center <strong>of</strong> the<br />

Virgo Cluster, such an orbit would take a time period<br />

<strong>of</strong> ten times the age <strong>of</strong> the Universe!<br />

It is suggested that we may have moved away from a<br />

closer orbit in the same fashion that the ends <strong>of</strong><br />

spiral-arms trail away from the nuclei <strong>of</strong> galaxies. At<br />

any rate, it appears that we are moving at about a<br />

right angle or edge-on toward SGL (super-galactic<br />

longitude) = 351° and SGB = -26°. We are moving, so<br />

it appears, away from the center <strong>of</strong> the supergalaxy<br />

(the Virgo Cluster) and slightly below the<br />

Supergalactic plane.<br />

As we have seen, galaxies are <strong>of</strong>ten members <strong>of</strong><br />

pairs, triplets and groups <strong>of</strong> increasing multiplicity. In<br />

fact, grouping or clustering (as it is called) is the rule<br />

rather than the exception. <strong>The</strong> Large Small<br />

Magellanic Clouds form a close pair and along with<br />

our galaxy, a loose triplet. M.31 (Andromeda) is the<br />

major component <strong>of</strong> a triplet including the two elliptical<br />

galaxies M.32 and NGC 205, and <strong>of</strong> a loose group<br />

with M.33 and the smaller ellipticals NGC 147 and<br />

185.<br />

261

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