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The Caldwell Objects

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32<br />

3 2<br />

NGC 4631<br />

Type: Barred Spiral Galaxy<br />

(SBd)<br />

Con: Canes Venatici<br />

RA: 12h 42.1m<br />

Dec: +32° 32'<br />

Mag: 9.2<br />

Dim: 14.7' x 3.5'<br />

SB: 13.3<br />

Dist: 22 million light-years<br />

Disc: William Herschel,<br />

1787<br />

W. H ERSCHEL:<br />

[Observed 20 March<br />

1787] Very bright. Much<br />

extended from south<br />

preceding to north fol-<br />

lowing [from southwest to northeast]<br />

but near the parallel. Much brighter in<br />

the middle. 16' long. (H V-42)<br />

GC: Remarkable, very bright, very large, extremely extended<br />

toward approximate position angle 70°, bright in the middle to a<br />

nucleus, bright star nearby.<br />

TO THE NAKED EYE CANES VENATICI LOOKS<br />

anemic. Its brightest star, Cor Caroli, shines at<br />

3rd magnitude, and its other stars are fainter than<br />

4th magnitude. But the constellation hosts a<br />

dynasty of telescopic splendors: the "colorful"<br />

globular cluster M3; the dramatic Whirlpool<br />

Galaxy, M51; the delicate Sunflower Galaxy,<br />

M63; and the mysterious, black-hole-bearing<br />

Seyfert galaxy, M106. And there's more. In the<br />

obscure southwestern quadrant of the constellation<br />

lurks one of the most distinguished —<br />

yet often overlooked — deep-sky objects of its<br />

class: the edge-on galaxy NGC 4631. Shining at<br />

magnitude 9.2 and spanning nearly ¼°, NGC<br />

4631 is, in fact, among the brightest and largest<br />

126<br />

NGC: Remarkable, very bright, very large, extremely<br />

extended toward approximate position angle 70°,<br />

bright in the middle to a nucleus, magnitude 12 star<br />

attached at north.<br />

edge-on galaxies in the night sky, and a vivid<br />

reminder that Messier's catalog is not an<br />

exhaustive list of celestial greats.<br />

At its distance of 22 million light-years, NGC<br />

4631 is quite large, having a true linear diameter<br />

of 94,000 light-years and a total mass of some 50<br />

billion Suns. We see the system inclined only 5°<br />

from edge on. But if we could tilt NGC 4631 over<br />

and view it face on, we would probably see a<br />

late-type barred spiral with very clumpy and<br />

loosely wound arms.<br />

<strong>The</strong> late Gerard de Vaucouleurs was the<br />

first (in 1963) to suggest that NGC 4631 was a<br />

barred spiral. <strong>The</strong> radial-velocity data upon<br />

which his conclusion rested were considered<br />

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

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