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The Caldwell Objects

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magnitude field star 2' to the north-northeast.)<br />

<strong>The</strong> best way to detect Aldebaran's true<br />

companion star is during a lunar occultation of<br />

Aldebaran itself. Aldebaran is the brightest star<br />

that the Moon can occult (other than the Sun!).<br />

<strong>The</strong>se occultations occur in bunches, and<br />

magazines like Sky & Telescope announce the<br />

events in their pages. <strong>The</strong> last series to be seen<br />

from the United States ended in 1999. Observers<br />

in the contiguous United States will have to wait<br />

for the year 2015 to see the next series begin.<br />

Despite Aldebaran's prominent position in<br />

the Bull's face, it is not a true member of the<br />

Hyades cluster. That much has been confirmed<br />

by the Hipparcos satellite. Launched in August<br />

1989, the High Precision Parallax Collecting<br />

Satellite was one of modern astronomy's true<br />

technological wonders. Equipped with two<br />

telescope systems aimed 58° apart, the rotating<br />

spacecraft was designed to measure star<br />

positions, brightnesses, and motions. Most<br />

fundamentally, by utilizing the Earth's orbit as a<br />

baseline for triangulation, Hipparcos pro-vided<br />

astronomers with parallaxes, and thereby<br />

distances, for tens of thousands of stars. Of the<br />

118,218 stars in the Hipparcos catalog, the<br />

distances of 22,396 are now known to an accura-<br />

cy of better than 10<br />

percent. (Before Hipparcos's<br />

data were<br />

released in 1997 the<br />

distances to fewer than<br />

1,000 stars were known<br />

so precisely.) Among<br />

those 22,396 precisely<br />

triangulated stars are<br />

many in the Hyades.<br />

<strong>The</strong> satellite has ended<br />

a century-long debate<br />

<strong>The</strong> <strong>Caldwell</strong> <strong>Objects</strong><br />

41<br />

over the cluster's distance — a critical quantity<br />

for calibrating the distance scale of the entire<br />

visible universe. Hipparcos has pinpointed the<br />

Hyades' center of mass at 151 light-years from<br />

Earth, plus or minus a mere 0.9 light-year.<br />

Taking advantage of the Hipparcos data, Sky<br />

& Telescope editor and Millennium Star Atlas<br />

coauthor Roger W Sinnott . created the 3-D<br />

stereogram of the Hyades shown below. T see o<br />

the cluster in three dimensions, hold the page<br />

against your face so each box is in front of one<br />

eye. Relax and gaze into the distance "through"<br />

the paper while slowly moving it away to reading<br />

distance or a little beyond. <strong>The</strong> two views<br />

should merge in your mind's eye. Note that<br />

Aldebaran is omitted; at its distance of 65 lightyears<br />

(also measured by Hipparcos), Aldebaran<br />

is less than half as far away as the Hyades.<br />

Of course, few will argue that Aldebaran's<br />

rosy hue does not attract our gaze toward the<br />

Bull's illustrious V. If you disagree, go outside,<br />

close one eye, and block the light of Aldebaran<br />

with your thumb while gazing outward with<br />

your open eye. (You can also do this with a star<br />

chart by simply covering Aldebaran with a finger.)<br />

Without Aldebaran, the Bull's face is lost,<br />

and the V suddenly transforms into the letter<br />

NorZ.<br />

165

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