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The Caldwell Objects

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with a sheen of light, especially at low magni-<br />

fications. <strong>The</strong> key, then, must be power. W need e<br />

to push the magnifications of our telescopes to<br />

the limits in order to penetrate this inner sanctum.<br />

How much power is needed? From<br />

Houston, Texas, Barbara Wilson viewed NGC<br />

7662 at 356x through a 13.1-inch f/4.5 reflector yet<br />

failed to see the star. Roger Clark suggests an<br />

astoundingly high power of 720x for telescopes 2<br />

to 8 inches in diameter. "This object provides a<br />

good example of how the upper limit to useful<br />

magnification depends on image brightness,"<br />

Clark says of NGC 7662. "<strong>The</strong> lesson is that if you<br />

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

magnification may bring out more detail, go<br />

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

limit of 60x per inch of objective diameter."<br />

Without question, the central star is there in<br />

photographs and CCD images of the Light Blue<br />

Snowball. Furthermore, while Hartung could not<br />

directly see the star with his 12-inch reflector, he<br />

did perceive its presence as a continuous streak<br />

when he inserted a prism into<br />

<strong>The</strong> <strong>Caldwell</strong> <strong>Objects</strong><br />

22<br />

the telescope's light path, spreading the star's<br />

light (and the nebula's) into a spectrum. Whoever<br />

does see the star will be rewarded by a rare sight:<br />

that of a hot, blue dwarf that has driven its own<br />

atmosphere away. As seen today from Earth, the<br />

nebula's shells are expanding outward at rates<br />

measured in tens of km per second; the bright<br />

inner shell already spans three-tenths of a lightyear<br />

and its faint outer envelope extends some 2<br />

light-years. Had its precursor been our Sun, the<br />

outer envelope of NGC 7662 would stretch<br />

halfway to the nearest neighboring star.<br />

Before you leave this fabulous object, I'd like<br />

you to search for an asterism I chanced upon<br />

while seeking NGC 7662. It is a nearly exact<br />

replica of M73, a Y-shaped grouping of four l0thmagnitude<br />

stars in Aquarius. <strong>The</strong> four close-knit<br />

stars in the Andromeda Y appear in the<br />

Millennium Star Atlas. <strong>The</strong> 3'-long group lies 2°<br />

south-southwest of 13 Andromedae and just 30'<br />

east of the 11th-mag-nitude galaxy NGC 7640.<br />

<strong>The</strong> Y is oriented northeast to southwest.<br />

95

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