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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 />

Moving Clusters<br />

Certain open clusters, for which the individual stars<br />

have a pronounced motion toward a convergent point,<br />

are known as Moving Clusters. <strong>The</strong> Hyades is one <strong>of</strong><br />

the earliest known and the nearest <strong>of</strong> these clusters.<br />

Except for small peculiar motions, all stars that are<br />

members <strong>of</strong> a moving cluster move in space along<br />

more or less parallel paths, much like meteors in a<br />

meteor stream. <strong>The</strong> individual proper motions <strong>of</strong> these<br />

stars seem to converge toward or diverge from a<br />

common point in the sky in the same way that<br />

meteors in showers appear to diverge from their<br />

radiants (see Meteors). <strong>The</strong> point <strong>of</strong> divergence<br />

marks the direction in space toward which the Sun is<br />

moving with respect to the cluster. <strong>The</strong> point <strong>of</strong><br />

convergence <strong>of</strong> the proper motions (opposite the point<br />

<strong>of</strong> divergence on the celestial sphere) marks the<br />

direction toward which the cluster is moving with<br />

respect to the Sun.<br />

<strong>The</strong> Ursa Major cluster is <strong>of</strong> particular interest to us<br />

since it occupies the same volume <strong>of</strong> space as our<br />

Sun. In fact, it is moving through our space, although<br />

the Sun is not a member <strong>of</strong> this cluster. <strong>The</strong> Ursa<br />

Major cluster is composed <strong>of</strong> two subgroups which<br />

consist <strong>of</strong> a moderately compact cluster <strong>of</strong> 14 stars<br />

with the same proper motion and an extended stream<br />

<strong>of</strong> stars which has approximately the same motion.<br />

<strong>The</strong> nucleus <strong>of</strong> this cluster is located about 23<br />

parsecs from the Sun and occupies (roughly)<br />

ellipsoidal region 4x6x10 parsecs in diameter. <strong>The</strong><br />

shortest diameter is perpendicular to the galactic<br />

plane, while the longest is in the direction <strong>of</strong> the<br />

motion <strong>of</strong> the cluster. <strong>The</strong> motion <strong>of</strong> the local centroid<br />

is 29 km/sec.<br />

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