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The Caldwell Objects

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102<br />

1 0 2<br />

<strong>The</strong>ta Carinae Cluster;<br />

Southern Pleiades<br />

IC 2602<br />

Type: Open Cluster<br />

Con: Carina<br />

RA: 10 h 42.9 m<br />

Dec: -64° 24'<br />

Mag: 1.9<br />

Diam: 100'<br />

Dist: 492 light-years<br />

Disc: Abbe Nicolas Louis<br />

de Lacaille, included in his<br />

1755 catalog<br />

H ERSCHEL: None.<br />

GC/NGC: None.<br />

IC: Cluster, coarse, includes θ Carinae.<br />

D ROP A VISUAL PLUMB LINE 4¾° DUE<br />

SOUTH of the magnificent Eta (η) Carinae<br />

Nebula and it will collide with another brilliant<br />

deep-sky wonder, IC 2602, the dazzling <strong>The</strong>ta (θ)<br />

Carinae Cluster (<strong>Caldwell</strong> 102). Louis de Lacaille<br />

discovered this mine of celestial diamonds<br />

during his great mid-18th-century exploration of<br />

the southern skies. <strong>The</strong> object is included in his<br />

1755 catalog, where it is the 9th listed under his<br />

Class II category ("nebulous clusters"). Lacaille<br />

called the object "<strong>The</strong>ta Argus" (Carina is the keel<br />

of the now-defunct constellation Argo Navis) and<br />

estimated its brightness as 3rd magnitude.<br />

Through his diminutive ½-inch 8x telescope<br />

Lacaille saw <strong>The</strong>ta Carinae "surrounded by many<br />

6/7/8 mag [stars] like the Pleiades." And that is<br />

why on modern charts IC 2602 is labeled "<strong>The</strong><br />

Southern Pleiades."<br />

With a declination of-64° 23.7', IC 2602 is<br />

only above 5½° my Volcano, Hawaii, horizon<br />

when at upper culmination. Yet even at that<br />

402<br />

meager altitude it is clearly visible to the unaided<br />

eye. <strong>The</strong> cluster is one of three major glows in the<br />

rich Carina Milky Way, the other two being NGC<br />

3532 (<strong>Caldwell</strong> 91) and the Eta Carinae Nebula<br />

(<strong>Caldwell</strong> 92). Together with the dense starclouds<br />

of the attendant Milky Way, the sight of these<br />

three objects is without question the most<br />

stunning in the entire heavens. Several of IC<br />

2602's stars are visible to the naked eye, but just<br />

how many depends upon the cluster's altitude,<br />

your site's darkness, and your ability to resolve<br />

stars packed tightly together. Photometry of two<br />

15'-wide fields, conducted in 1991 with the 1meter<br />

Swope telescope at Las Campanas<br />

Observatory in Chile, revealed that half the stars<br />

visible to the telescope in IC 2602 were<br />

background stars — not surprising for an open<br />

cluster in a rich Milky Way field. Brent Archinal<br />

says IC 2602 harbors at least 60 definite members<br />

spread across 100'; some 30 of these are brighter<br />

than<br />

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

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