OF THE ROGER N. CLARK
OF THE ROGER N. CLARK
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