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The Caldwell Objects

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19<br />

N G C 6 2 8 1<br />

T y O p e C : n l u s t e r<br />

C o S n c : o r p i u s<br />

RA: 17 h 04.8 m<br />

Dec: -37° 53'<br />

Mag: 5.4<br />

Diam: 8'<br />

Dist: 1,800 light-years<br />

<strong>The</strong> tail of Scorpius, the Scorpion, is projected<br />

against the hub of our galaxy, a region littered<br />

with open clusters and asterisms. Some might<br />

argue that once you move beyond the Messier<br />

and <strong>Caldwell</strong> Catalogs, open clusters are all the<br />

same — little puffs of concentrated starlight. But<br />

one, NGC 6281, stands out from the multitude as<br />

a fine target for small telescopes. In fact, at<br />

magnitude 5.4, NGC 6281 is the brightest non-<br />

Messier/non-<strong>Caldwell</strong> open cluster in Scorpius,<br />

though one hardly hears about it. Brent Archinal<br />

lists about 70 stars within its 8'-wide disk, with<br />

the brightest shining at magnitude 9.0. <strong>The</strong><br />

cluster's surface brightness is also quite high,<br />

making it a fine naked-eye target.<br />

Alas, the cluster is near a host of other<br />

popular objects. It is 4½° north-northeast of NGC<br />

6231 (<strong>Caldwell</strong> 76), 2° southwest of the Bug<br />

Nebula (<strong>Caldwell</strong> 69), 10° southwest of M7, and<br />

8° northeast of NGC 6124 (<strong>Caldwell</strong> 75). At least<br />

NGC 6281 is conveniently located. It simply lies<br />

2½° east-northeast of Mu 1,2 (μ 1,2 ) Scorpii, about<br />

one-third of the way toward the paired Stinger<br />

stars at the end of the Scorpion's tail. Through the<br />

Genesis NGC 6281 is best seen at 23x, when its<br />

stars form a marvelous dipper of bright suns<br />

superimposed on a fog of Milky Way. Ernst<br />

Hartung concurs, saying the cluster is "very<br />

beautiful with a pyramidal group of stars . . .<br />

standing out prominently in<br />

the centre; it contains several pairs and two<br />

bright orange stars, and the linear pattern is most<br />

striking." Christian Luginbuhl and Brian Skiff<br />

add that the cluster has "20 stars arranged over<br />

haze like Christmas tree lights," making it "a<br />

pretty cluster" for a 60-mm telescope.<br />

20<br />

SL 7<br />

T y D p a e Nebula r : k<br />

C o L n u : p u s<br />

RA: 16 h 01.8 m<br />

Dec:-41° 52'<br />

Mag: —<br />

Dim: 160' x 10'<br />

Dist: unknown<br />

Our final hidden treasure is an incredible veil of<br />

darkness in southeastern Lupus that dips ever so<br />

slightly into Norma and Scorpius. On a scale of<br />

opacity ranging from 1 to 6, SL 7 is classified as a<br />

6, meaning "highly opaque." <strong>The</strong> nebula is an<br />

elongated swath of darkness running from eastnortheast<br />

to west-southwest. Though it is about 4<br />

Moon diameters long, only about a dozen stars<br />

between 9th and 11th magnitude lie within its<br />

confines! <strong>The</strong> darkest section, to the southwest, is<br />

an empty l°-wide corridor that begins about 3¾°<br />

due south of Eta (η) Lupi, just south of a 5thmagnitude<br />

star. Compared to SL 7, the Coalsack<br />

(<strong>Caldwell</strong> 99) appears very dark to the unaided<br />

eye. Yet through a telescope the Coalsack is<br />

littered with stars; its clouds do not appear black<br />

(like those of SL 7) but gray through the 4-inch.<br />

Twenty Spectacular Non-<strong>Caldwell</strong> <strong>Objects</strong> 443

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