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The Caldwell Objects

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91<br />

9 1<br />

<strong>The</strong> Pincushion Cluster<br />

NGC 3532<br />

Type: Open Cluster<br />

Con: Carina<br />

RA: 11 h 05.5 m<br />

Dec: -58° 44'<br />

Mag: 3.0; 3.2 (O'Meara)<br />

Diam: 50.0'<br />

Dist: 1,600 light-years<br />

Disc: Abbe Nicolas Louis de Lacaille (in his 1755 catalog), but<br />

probably known since antiquity<br />

J. H ERSCHEL: Chief star of a very large, round, loosely scattered<br />

cluster of stars [of] 8[th to] 12th magnitude, which fills 2 or 3 fields.<br />

A fine bright object, (h 3315)<br />

M IDWAY BETWEEN THE F ALSE C ROSS AND the<br />

Southern Cross lies one of the heavens' true<br />

stellar spectacles, the 3rd-magnitude open star<br />

cluster NGC 3532 (<strong>Caldwell</strong> 91). It is a burst of<br />

visual splendor in the swirling tempest of the rich<br />

Carina starcloud. Together with the Eta Carinae<br />

Nebula (<strong>Caldwell</strong> 92, just 3° to the westsouthwest)<br />

and IC 2602, the Southern Pleiades<br />

(<strong>Caldwell</strong> 102), NGC 3532 is part of the most<br />

magnificent tract of Milky Way in the entire<br />

heavens. Doubtlessly it has been a visual<br />

landmark ever since aboriginal people first began<br />

looking to the heavens. Yet its discovery is<br />

credited to an 18th-century European explorer,<br />

Abbe Nicolas Louis de Lacaille; he included it in<br />

his 1755 catalog as the 10th member of his Class<br />

II (nebulous clusters). It seems almost<br />

blasphemous to consider this object an 18thcentury<br />

European revelation, and I'm certain<br />

Lacaille himself would have agreed. That being<br />

said, this cluster's brightest stars shine at<br />

magnitude 8, so they are too faint to discern<br />

individually without optical aid. To the naked<br />

eye the cluster looks like an enhancement of<br />

GC / NGC: Remarkable, cluster, extremely large, round,<br />

little compressed, stars of magnitude 8 to 12.<br />

the Milky Way, a fantastic knot in the fabric of<br />

space — but not a star cluster. It took Lacaille's<br />

meager ½-inch 8x telescope to reveal, for the first<br />

time, that this diffuse glow was actually "a<br />

prodigious number of faint stars forming a semicircle<br />

of 20/25 [arc]minutes diameter."<br />

Nearly three-quarters of a century later<br />

James Dunlop trained his 9-inch telescope on the<br />

southern skies and encountered NGC 3532,<br />

which he described as "a very large cluster of<br />

stars about the 9th magnitude, with a red star of<br />

the 7-8th magnitude, north following [northeast<br />

of] the centre of the cluster. Elliptical figure: the<br />

stars are pretty regularly scattered." Dunlop's<br />

description falls far short of declaring the object's<br />

true glory, which John Herschel and, later,<br />

William Pickering extolled. Herschel called NGC<br />

3532 a "superb" cluster, "the most brilliant object<br />

of the kind I have ever seen." And like Herschel<br />

before him, Pickering saw it as the finest<br />

irregular star cluster in the sky.<br />

Today NGC 3532 is classified as a very rich,<br />

intermediate-age open cluster. Recent estimates<br />

date it at about 300 million years; that's<br />

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

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