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The Caldwell Objects

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43 & 44<br />

then tapers off to form a short and extremely dim<br />

needle of light. No feature like this can be seen on<br />

the northwestern end.<br />

Higher power does not enhance the view. In<br />

fact, with it the galaxy is much more difficult to<br />

observe because its dim light is being spread over<br />

a greater area. But with patience the view<br />

supports all that was seen at the other<br />

magnifications. <strong>The</strong> neighboring 7.2-magni-tude<br />

star (which appears in the photograph on page<br />

173) looks distinctly yellowish, but this might<br />

have been caused by smog from neighboring<br />

Kilauea, since the star has a blue-white spectral<br />

type of AO. Vog (volcanic smog) tends to redden<br />

starlight, and the effect is especially noticeable at<br />

high magnifications.<br />

Out of idle curiosity, on one night in<br />

February 1997 I decided to try for NGC 7814<br />

from inside the Dillingham Ranch house, which<br />

has large glass windows. Earlier experiments had<br />

shown that the windows did not visibly affect<br />

star images at 23x. But I wondered how the glass<br />

would affect dim nebulous objects like NGC<br />

7814. (Apparently the notion of the Great Square<br />

as a "window" spurred me to try this.) Alas, I<br />

could not detect the galaxy through the<br />

windows, though I did see it once I moved my<br />

telescope outdoors. On one sparkling, clear night<br />

in November 1999 NGC 7814 was nearly<br />

overwhelmed by light from a four-day-old<br />

Moon. This suggests that light pollution will<br />

certainly compromise its visibility in small<br />

telescopes.<br />

Our second <strong>Caldwell</strong> galaxy, NGC 7479, lies<br />

about 3° south of Alpha (α) Pegasi, or Markab,<br />

the southwestern corner of the Great Square; it's<br />

also 4½° east of magnitude-4.2 Xi (ξ) Pegasi in<br />

the Horse's mane. Observers with telescopes on<br />

equatorial mounts should take these "express<br />

routes" to the galaxy. Here are some other fun<br />

ways to find it. If the owner of a Telrad sighting<br />

device places Markab on the<br />

176<br />

northern side of her finder's third and outermost<br />

ring, NGC 7479 will be just within the southern<br />

side of the second, or middle, ring. A Qwik Point<br />

owner should place his LED spot near the<br />

imaginary southern apex of a right triangle made<br />

with Markab and Xi Pegasi. You can also star-hop<br />

from 55 Pegasi, the westernmost of four 5thmagnitude<br />

stars forming a tight 1°-long trapezoid<br />

5½° south of Markab. From 55 Pegasi, follow a<br />

chain of three 7th- to 8th-magnitude stars (each<br />

separated by less than 1°) to the north-northwest;<br />

NGC 7479 will be ½° northeast of the last star in<br />

the chain, at the end of another chain of 9th- to<br />

llth-mag-nitude stars. (<strong>The</strong> former chain, but not<br />

the latter, is shown on our finder chart below.)<br />

NGC 7479 is a highly asymmetrical barred<br />

spiral that belongs to the Pegasus Cloud of<br />

galaxies, a generous gathering of 51 island universes<br />

some 100 million light-years distant. <strong>The</strong><br />

galaxy is slightly more than twice as far as NGC<br />

7814, yet it shines with nearly the same<br />

brightness and appears nearly as large in angular<br />

terms. That's because the system is quite large<br />

intrinsically, having a total mass of<br />

Deep-Sky Companions: <strong>The</strong> <strong>Caldwell</strong> <strong>Objects</strong>

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