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The Caldwell Objects

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55<br />

5 5<br />

Saturn Nebula; Venus Nebula;<br />

Ghost of Saturn Nebula<br />

NGC 7009<br />

Type: Planetary Nebula<br />

Con: Aquarius<br />

RA: 21 h04 m 10.8 s<br />

Dec: -11° 21' 49"<br />

Mag: 8.0<br />

Dim: 44" X 23"<br />

Dist: 1,400 light-years<br />

Disc: William Herschel, 1782<br />

W . HERSCHEL: [Observed 7 September 1782] Very bright, nearly<br />

round planetary disk not well defined. (Η IV-1)<br />

GC / NGC: A magnificent object, planetary, very bright, small,<br />

elliptic.<br />

O N THE EVENING OF A UGUST 29, 1780,<br />

Pierre Mechain, Charles Messier's contemporary<br />

and rival comet hunter, discovered a faint glow<br />

in Aquarius 4° southwest of 4.5-magni-tude Nu<br />

(ν) Aquarii. Messier searched for Mechairis find<br />

the following October (on the evenings of the 4th<br />

and 5th) and determined its position relative to<br />

Nu Aquarii. Now known to be a globular cluster,<br />

this object became the 72nd in Messier's growing<br />

list of non-comets. On those same two evenings,<br />

Messier discovered a "[c]luster of three or four<br />

faint stars, which, at first glance, resembles a<br />

nebula." Again Messier determined the new<br />

object's position relative to Nu Aquarii, and this<br />

tiny asterism became the 73rd object to enter his<br />

catalog. <strong>The</strong> irony of these discoveries and their<br />

follow-up observations is that about 1¼° due<br />

west of Nu Aquarii is one of the heavens'<br />

brightest planetary nebulae — NGC 7009. And it<br />

entirely escaped both Messier's gaze and<br />

Mechairis.<br />

218<br />

But this is not surprising. Although NGC 7009 is<br />

bright, it is also small (its brightest part spans<br />

only 23"), and it can be easily mistaken for a star<br />

at low power, especially when seen through a<br />

small telescope. <strong>The</strong> nebula did not fool William<br />

Herschel, though; he discovered it in 1782,<br />

finding it "very bright." He also classified the<br />

object now known as NGC 7009 as a planetary<br />

nebula because it was "nearly round," like a<br />

planet, and bore magnification well, like a planet.<br />

However, the nebula's hallmark ringlike<br />

extensions remained undetected until Lord Rosse<br />

(William Parsons, third Earl of Rosse) scrutinized<br />

the nebula with his 72-inch reflector. In his 1850<br />

paper, "Observations on the Nebulae," Rosse<br />

described NGC 7009 as having a fairly uniform<br />

luminous disk with "ansae which probably<br />

indicate a surrounding nebulous ring seen<br />

edgeways." Indeed, as Robert Burnham Jr. notes<br />

in his Celestial Handbook "Rosse's drawing<br />

portrays the nebula with a somewhat greater<br />

degree of symmetry and<br />

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

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