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The Caldwell Objects

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15<br />

outer shell falls upon the retina's rod-lined<br />

of their characteristics suggest that FLIERs are<br />

like sparks flung outward from the central star<br />

about 1,000 years ago. Yet their shapes, as revealed<br />

by HST, suggest that they are stationary,<br />

and that material ejected from the star flows past<br />

them, scraping gas from their surfaces.<br />

It's best to approach this curious object in<br />

four simple steps. First locate 3rd-magnitude<br />

Delta (δ) Cygni, which marks the western arm of<br />

the Northern Cross asterism. Seven degrees<br />

north-northwest of Delta Cygni is 4th-magnitude<br />

Iota (ι) Cygni. Next locate the beautiful<br />

double star 16 Cygni 2¼° degrees to the southeast;<br />

the sight of its 6th-magnitude Sun-like stars,<br />

separated by 40", equals that of the planetary<br />

itself. (What's more, we now know that the<br />

southeastern member of the pair is orbited every<br />

2.2 years by a planet or substellar brown dwarf<br />

that may have as little as 1.5 times the mass of<br />

Jupiter.) NGC 6826 is about ½° east-southeast of<br />

periphery, which sends electrical signals to the the double. In fact, you can look for a "double<br />

brain, making the outer shell suddenly pop into star" at the planetary's position, for it forms a<br />

view. Alternating between direct and indirect pair with a much dimmer 12th-magnitude star<br />

vision makes a double-shelled planetary appear 1.6' to the south. See if you can detect the<br />

to blink.<br />

planetary with 7x35 binoculars; the task should<br />

<strong>The</strong> blinking phenomenon is a rather good be easy.<br />

metaphor for the brief lives of these phantom gas At 23x through the 4-inch NGC 6826 is vir-<br />

clouds. A planetary nebula lasts but for a "blink tually stellar, though averted vision and a few<br />

of an eye" in astronomical terms. A Sunlike star minutes of staring shows its slightly swollen<br />

can live for 10 billion years, but the shell we see form. Increasing the magnification to 72x reveals<br />

around NGC 6826 will last for no more than the planetary as a small disk with a soft aqua hue<br />

some 10,000 years. Hubble Space Telescope reminiscent of the colors one sees when peering<br />

images of the Blinking Planetary cause us to at Uranus or Neptune through a telescope.<br />

blink yet another way: in surprise. For in them Steven Hynes, the author of Planetary Nebulae,<br />

we see mysterious knots of dense gas that noted a blue-green hue to NGC 6826 through his<br />

astronomers have dubbed FLIERs (/ast l -o<br />

w 10-inch reflector at 155x. At 189x in the 4-inch,<br />

ionization emission regions). FLIERs cause the nebula's 10.6-magnitude central star stands<br />

astronomers to blink because they challenge their out as a strong punctuation mark at the center of<br />

understanding of planetary nebulae. No model of a large, diffuse shell of uniform light, though<br />

stellar evolution presently can explain their there is a hint of brightening toward the central<br />

existence. In one sense, says Bruce Balick star. Viewing through a 16½-inch telescope,<br />

(University of Washington), some<br />

Webb Society member<br />

<strong>The</strong> <strong>Caldwell</strong> <strong>Objects</strong> 69

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