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The Caldwell Objects

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5 6<br />

Pac-Man Nebula<br />

NGC246<br />

Type: Planetary<br />

Nebula<br />

Con: Cetus<br />

RA: 00 h 47 m 03.3 s<br />

Dec:-11° 52' 19"<br />

Mag: 10.9<br />

Dim: 4.6' χ 4. 1’<br />

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

Disc: William Herschel, 1785<br />

W. H E R S C H E L: [Observed27November 1785]<br />

Four or five pretty [bright] stars forming a<br />

trapezium of about 5' in diameter. <strong>The</strong> enclosed<br />

space is filled up with faintly terminated milky<br />

nebulosity. <strong>The</strong> stars seem to have no<br />

[connection] with the nebulosity. (H V-25)<br />

NGC 246 is ONE OF THE CALDWELL CATALOG'S most<br />

visually intriguing planetary nebulae. Look at the<br />

photograph above. Here we see a broken shell of<br />

gas centered on a 12th-magni-tude star. Several<br />

other conspicuous stars are superimposed on the<br />

gas shell as well, and still others lie just beyond<br />

the nebula's confines. Now read William<br />

Herschel's discovery description. Does it cause<br />

you to raise an eyebrow? Where is the 5'-wide<br />

trapezium of stars? And isn't it strange that he<br />

would write "four or five pretty [bright] stars"<br />

[emphasis mine]? Note, too, that Herschel does<br />

not say that the nebulosity is centered on a 12thmagnitude<br />

star. Instead he says that the nebula<br />

fills the space within the trapezium. <strong>The</strong> New<br />

General Catalogue is more satisfying because it<br />

seems to better describe what is seen, at least in<br />

long-exposure photographs — namely four<br />

bright stars associated with a diffuse nebula<br />

(though these four stars do not form a trapezoid).<br />

Here's another mystery, which could be<br />

56<br />

GC / NGC: Very faint, large, 4 stars in a diffused nebula.<br />

related to the first. In the December 1984 issue of<br />

Sky & Telescope, Walter Scott Houston reported<br />

that, with an 8-inch f/5 reflector, skilled deep-sky<br />

observer Ronald Morales of Arizona easily saw<br />

NGC 246 "as a round, diffuse glow behind three<br />

stars of similar brightness. A fourth was<br />

glimpsed, but the central star was not seen."<br />

Really? Would a skilled observer like Morales<br />

miss seeing a 12th-mag-nitude star in an 8-inch<br />

telescope? You wouldn't think so. Yet Morales<br />

apparently is not alone. In August 1986 veteran<br />

observer Barbara Wilson didn't see the central<br />

star either, and she used a 13.1-inch f/4.5 reflector<br />

at 222x. A drawing in Volume 2 of the Webb<br />

Society Deep-Sky Observers Handbook does show<br />

the central star in an annulus whose periphery is<br />

dappled with the light of three obvious stars; the<br />

drawing is based on a view through an 8-inch<br />

telescope at 75x, and the stars in the drawing<br />

match those seen in photographs. Ernst Hartung<br />

also saw the central star. In his<br />

<strong>The</strong> <strong>Caldwell</strong> <strong>Objects</strong> 223

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