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The Caldwell Objects

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(which does not appear on Sky Atlas 2000.0 but is<br />

plotted in the Millennium Star Atlas and<br />

Uranometria 2000.0) is commonly picked up<br />

through telescopes with moderately large<br />

apertures and mistaken for a comet. (NGC 4562<br />

appears in the lower right-hand corner of the<br />

photograph on page 150.) Another galaxy that<br />

may be stumbled upon in the search for NGC<br />

4565 is NGC 4494, a 10th-magnitude elliptical<br />

galaxy about ½ ° east-southeast of 17 Comae<br />

Berenices.<br />

Perhaps the greatest visual challenge posed<br />

by NGC 4565, though, is to sight the edge-on<br />

spiral in 7x35 binoculars. Its thinness and its<br />

prominent dust lane both cause the galaxy to be<br />

close to the limit of detectability. I succeeded at<br />

an altitude of 4,200 feet under very dark<br />

Hawaiian skies. It was a very difficult observation,<br />

requiring a lot of time and patience for me<br />

to be confident I had seen the galaxy's slender<br />

body. Sky & Telescope editor Joshua Roth saw it in<br />

his 60-mm f/5.9 refractor from the Amateur<br />

Telescope Makers of Boston's dark-sky site in<br />

Westford, Massachusetts, and called it a<br />

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

38<br />

"sweet little needle of light."<br />

Since NGC 4565 and its rival, NGC 891 in<br />

Andromeda, lie at about the same altitude after<br />

sunset (at opposite ends of the sky) around the<br />

start of spring in the Northern Hemisphere, try<br />

observing them both on the same night. <strong>The</strong> two<br />

galaxies are essentially the same distance from<br />

us, and are roughly the same size, but NGC 4565<br />

is much more conspicuous because its surface<br />

brightness is twice that of NGC 891. This<br />

difference in surface brightness can be attributed<br />

at least in part to extinction — the absorption and<br />

scattering of starlight by intervening dust, which<br />

lies in our Milky Way and within the edge-on<br />

spirals. NGC 891 lies on a sightline that skirts our<br />

home galaxy's midplane, and the passage<br />

through our galaxy's dusty disk dims NGC 891's<br />

light by 0.2 magnitude, or 17 percent. NGC 4565,<br />

by contrast, is a mere 3½° west of the north<br />

galactic pole — an essentially transparent<br />

window onto extra-galactic space — and its light<br />

is reduced by only 0.05 magnitude (5 percent).<br />

Roth says he has yet to see NGC 891 in his 60-mm<br />

telescope.<br />

153

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