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The Caldwell Objects

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76<br />

76<br />

False Comet Cluster<br />

NGC 6231 Type:<br />

Open Cluster<br />

Con: Scorpius<br />

RA: 16 h 54.2 m<br />

Dec:-41° 50'<br />

Mag: 2.6<br />

Diam: 14.0'<br />

Dist: 6,000 light-years<br />

Disc: Giovanni Batista<br />

Hodierna, before 1654; but<br />

known since antiquity<br />

J. HERSCHEL: A fine bright large cluster pretty rich,<br />

class VII. 10', stars [from] 10[th to] 13th<br />

magnitude]. Place of a double star 5th<br />

magnitude], the preceding [western] but one of 7<br />

H AD THE 18TH- CENTURY F RENCH COMET<br />

hunter Charles Messier lived farther south than<br />

Paris he most certainly would have noticed the<br />

bright 2°-long "comet" that perpetually shines in<br />

the Scorpion's Tail. I'm confident Messier would<br />

have noticed it, because my wife, Donna, never<br />

fails to discover the same "comet" each time she<br />

looks upon the stunning Scorpius Milky Way<br />

with her unaided eyes from Hawaii. Of course,<br />

the object is not a comet, but it is the most<br />

cometlike naked-eye spectacle in the heavens that<br />

is not a comet. Open cluster NGC 6231 (<strong>Caldwell</strong><br />

76) forms the "head" of our pseudocomet and lies<br />

only 30' north of the 4th-magnitude double star<br />

Zeta 1,2 (ζ 1,2 ) Scorpii; the comet's "tail" is the large,<br />

elongated open cluster Trumpler 24 to the north.<br />

Although these objects have separate catalog<br />

identities, they belong to the same group of<br />

luminous stars, the Scorpius OB1 Association.<br />

This widely scattered family of young stars<br />

marks<br />

300<br />

bright stars in the middle, (h 3652)<br />

GC / NGC: Cluster, bright, considerably large, pretty rich,<br />

consisting of stars of 10th to 13th magnitude.<br />

the onetime location of a giant Η II region. It<br />

resides in the Sagittarius-Carina spiral arm,<br />

which lies closer to the galactic center than the<br />

one containing our Sun. Both of these clusters<br />

would have been appropriate for Messier's catalog<br />

had he known of their existence.<br />

Which brings us to the next point. Most<br />

sources credit Nicolas Louis de Lacaille for discovering<br />

NGC 6231 during his exploration of the<br />

southern skies from the Cape of Good Hope in<br />

the 1750s. But true credit belongs to long-forgotten<br />

Giovanni Batista Hodierna, an astronomer<br />

at the court of the Duke of Montechiaro, who<br />

compiled a catalog of nebulous objects that he<br />

observed with a simple 20x Galilean refractor.<br />

Printed in Palermo in 1654, his work listed 40<br />

nebulous objects, 19 of which (NGC 6231<br />

included) were of his own discovery Since<br />

Galileo had resolved the misty Milky Way into<br />

stars, Hodierna believed that all the heavens'<br />

nebulous objects were star clusters, and<br />

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

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