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OF THE ROGER N. CLARK

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VISUAL ASTRONOMY <strong>OF</strong> <strong>THE</strong> DEEP SKY<br />

A VISUAL ATLAS <strong>OF</strong> DEEP-SKY OBJECTS<br />

NGC 7662, PLANETARY NEBULA IN<br />

ANDROMEDA<br />

R.A. 23h 25.9m, Dec. 42° 33' (2000.0)<br />

Technical. NGC 7662 is a small planetary<br />

nebula somewhere between 2000 and 6000<br />

light-years away. (The distances of all planetary<br />

nebulae are poorly known.) Its diameter<br />

is between 0.3 and 0.8 light-years, depending<br />

on the distance adopted. The central star has<br />

a surface temperature around 75 000 Kelvin<br />

and has been suspected of variability, though<br />

no systematic photometric study has been<br />

completed. The nebula consists of an inner,<br />

broken ellipse surrounded by a fainter elliptical<br />

disk. The dark area in the center is<br />

perhaps similar in brightness to the outer<br />

ellipse.<br />

--<br />

Visual. NGC 7662 has a total magnitude of<br />

8.5 and an angular size of 32 by 28 arc.<br />

seconds, for a very high mean surface bright.<br />

ness: 15.6 magnitudes per square arc-second<br />

The planetary is visible in 7 X 50 binocula<br />

and small telescopes as a star, but will begin<br />

to show its disk at powers near 50 X. Through<br />

the 8-inch telescope under moderate skies<br />

the darker center was suspected at 334x and<br />

seen fairly well at 592 X.<br />

This object provides a good example of<br />

how the upper limit to useful magnification<br />

depends on image brightness. In the dim<br />

light levels of deep-sky astronomy, the eye<br />

has very poor resolution, so small detail may<br />

have to be magnified very highly to be detect.<br />

able. The 8-inch had no clock drive for tracking,<br />

so examination of this object was rather<br />

difficult at very high powers. Telescopes of<br />

similar size with clock drives could use higher<br />

powers still. The lesson is that if you are<br />

observing an object and feel that higher magnification<br />

may bring out more detail, go<br />

ahead and ignore the "accepted" magnification<br />

limit of 60 X per inch of objective diameter<br />

(480X on an 8-inch telescope) . See<br />

Chapter 3 for more on this subject.<br />

Photograph of NGC 7662. South is up . (Courtesy<br />

Jack B. Marling.)<br />

---1' ---<br />

Drawing of NGC 7662.<br />

Scale: 0.25 arc-min/cm<br />

8-inch fll l.5 Cassegrain<br />

12.4mm Erfle (188X)<br />

7mm Erfle (334x)<br />

l2.4mm Erfle + 3. l5x<br />

barlow (592X)<br />

Viewing Distance (cm)<br />

50X:275 300X:46<br />

IOOX: 138 400x:34<br />

200x: 69 600x:23<br />

air mass: l.41, faintest star: 13.8 at zenith, 188x;<br />

no tracking<br />

9/5/83 14:00- 1 4:20 UT at Hawaii Kai, Hawaii; R.<br />

Clark<br />

242<br />

243

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