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The Caldwell Objects

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54<br />

About half of the stars on NGC 2506's main<br />

sequence are binaries, as are more than 20<br />

percent of the cluster's 800 or so total members.<br />

Some blue stragglers — stars that apparently<br />

linger on the main sequence — also have been<br />

confirmed as members of this cluster. Most<br />

astronomers believe that a blue straggler forms<br />

when two closely orbiting stars merge, producing<br />

an unusually massive single star that has yet to<br />

depart the hydrogen-fusing main-sequence stage<br />

of stellar evolution.<br />

NGC 2506's apparent size of 12' is deceivingly<br />

small. <strong>The</strong> cluster lies 10,000 light-years<br />

from Earth; that's twice as far as M46 and more<br />

than 5 times the distance of M48. NGC 2506<br />

spans some 37 light-years, making it 16 percent<br />

larger intrinsically than M46 and nearly 50<br />

percent larger than M48. If we could bring NGC<br />

2506 as close as M48, it would shine at 4th<br />

magnitude and span a full degree of sky, making<br />

it a near rival to M44, the famous Beehive Cluster<br />

in Cancer. And if we could bring NGC 2506 as<br />

close as the Beehive Cluster (515 light-years), we<br />

would see a spectacular 1st-magnitude object 4°<br />

across. Poets would have been inspired to glorify<br />

this scintillating fury of grizzled suns, and we<br />

amateurs would have<br />

216<br />

had the chance to ponder another cluster as<br />

magnificent as the Pleiades.<br />

We can at least imagine such glory as we<br />

peer at NGC 2506 through our telescopes. To find<br />

it I follow a river of suns that meanders eastward<br />

from Sirius, past 4th-magnitude Gamma (γ)<br />

Canis Majoris and beyond the clusters M46 and<br />

M47, until I get to 5th-mag-nitude 19 Puppis — a<br />

journey of more than 20°. Confirming 19 Puppis's<br />

identity is simple, because the star is<br />

superimposed on the southeastern side of<br />

another dramatic open cluster, 6.5-magnitude<br />

NGC 2539. <strong>The</strong> star is also the southernmost in a<br />

4°-long chain of three stars pointing to the northnorthwest.<br />

That chain's other two stars shine at<br />

magnitude 6.3 and 6.2, respectively; the<br />

magnitude-6.2 star, at the chain's northern end, is<br />

also a visual double star. You will need to<br />

confirm that you've correctly located these stars<br />

in your finderscope or in binoculars before<br />

carrying on. NGC 2506 makes a near-equilateral<br />

triangle with chain's northernmost two stars, to<br />

the west.<br />

In 7x35 binoculars NGC 2506 looks unimpressive,<br />

almost inconsequential — a celestial<br />

afterthought. But stick with it for a moment,<br />

because with averted vision a bright core should<br />

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

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