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The Caldwell Objects

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89<br />

trending chain of stars surrounded by a magnificent<br />

halo of unresolved suns. S Normae<br />

immediately draws attention to itself with its<br />

orange color. A 9th-magnitude star pops into<br />

view at the extreme northern edge of the halo,<br />

and a pair of 8th- and 9th-magnitude suns marks<br />

the halo's southern boundary. Overall, the<br />

binocular view reminds me of a granite Celtic<br />

cross — the kind you'd find glowing in a<br />

cemetery, as if moonlit on a foggy night. I cannot<br />

see this background glow with the naked eye,<br />

only the bright bar of stars; the background<br />

swells into view only when binoculars and<br />

averted vision are used.<br />

NGC 6087 is a relatively young open cluster,<br />

about 65 million years old. It has been of<br />

352<br />

particular interest to astronomers because of its<br />

association with its Cepheid lucida. Cepheids<br />

have extremely stable periods of variability and<br />

very reproducible light curves. In the early 20th<br />

century Henrietta S. Leavitt discovered that<br />

Cepheids have a very special relationship<br />

between their intrinsic brightnesses, or luminosities,<br />

and their periods of variability.<br />

Basically, the brighter a Cepheid is, the longer it<br />

takes to complete one cycle of brightening and<br />

fading. By observationally determining the<br />

period of a Cepheid variable, we learn its<br />

intrinsic brightness. <strong>The</strong>n, by comparing how<br />

bright it appears with how bright it really is, we<br />

can deduce its distance. Applying the periodluminosity<br />

rule to S Normae, we get a distance<br />

of 1 kiloparsec, or 3,300<br />

light-years.<br />

At 23x in the Genesis<br />

it's almost hard to believe<br />

you're looking at a<br />

star cluster with half the<br />

angular size of the full<br />

Moon, because NGC<br />

6087's brightest stars do<br />

not seem to blend<br />

together very well.<br />

Except for a 5'-wide<br />

gathering of suns<br />

close to S Normae, the cluster's remaining<br />

constituents appear to be scattered like stellar<br />

marbles, forming all manner of geometrical<br />

patterns — right angles, lines, arcs, diamonds —<br />

in a most haphazard way. Add the rich Milky<br />

Way background and it's a visual mess. But if<br />

you relax your gaze and let your eye roam<br />

around the field you should see that the cluster's<br />

edges fit within the confines of a boxlike<br />

arrangement of field stars. It looks as if several<br />

trucks loaded with stars had approached S<br />

Normae from various directions, dropped their<br />

wares on top of it, and then departed. In<br />

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

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