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The Caldwell Objects

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includes a visual description of the dwarf system,<br />

so I had no way of knowing what to expect. But I<br />

believe this "not knowing" was good, albeit<br />

frustrating, because I had no preconceived<br />

expectations. In the early morning hours on one<br />

extremely windy and clear August night that<br />

same year, when the region neared the meridian,<br />

I saw IC 1613 with the Genesis at 23x. In Hawaii,<br />

as on the mainland, cold fronts can bring<br />

incredible transparency, suddenly turning our<br />

night skies into dizzying starscapes of galactic<br />

wonder. When this happens I feel as if I am<br />

looking into the very soul of night. Peering into a<br />

telescope is difficult when the naked-eye sky is<br />

grabbing hold of your heart. Nevertheless, I<br />

immediately set my sights on IC 1613 and very<br />

easily located it. If there is a lesson to be learned<br />

from this celestial adventure of mine, it would be<br />

that the visibility of a celestial object (be it a faint<br />

star, a comet, a tight double star, a galaxy, a<br />

nebula,<br />

206<br />

51<br />

or whatnot) cannot be determined solely by<br />

effort alone. <strong>The</strong> atmosphere's clarity and the<br />

observer's physical condition also matter, as does<br />

his or her level of experience.<br />

At 23x IC 1613 shimmers just above the sky<br />

background; it is definitely a "tube tapper." At<br />

first it appears as a pale circular glow sandwiched<br />

between the 7th-magnitude star and two<br />

11th-magnitude stars 11' to the southwest. With a<br />

concentrated effort and averted vision, the galaxy<br />

displays a mottled form. Its most noticeable<br />

concentration is about 5' northeast of the<br />

southernmost 11th-magnitude star. Two knots,<br />

joined by a tendril of nebulosity, lie to the<br />

northwest and southeast of this "core" of stellar<br />

material. Another knot is displaced several<br />

arcminutes to the northeast. <strong>The</strong> galaxy is much<br />

more difficult to observe at 72x. I find it best to<br />

take numerous short glimpses over a long period<br />

of time, say 20 minutes, alternating photon<br />

collection with rest. When I do this, the galaxy<br />

appears more triangular in shape, and its bar<br />

becomes a scintillating strand of light with pale,<br />

mottled chunks. <strong>The</strong> knot to the northeast is<br />

clearly separated from the bar. Here is that gulf<br />

of darkness mentioned above, and a region of<br />

star birth. Imagine the processes going on in the<br />

celebrated Orion Nebula but across a much<br />

larger area and in another galaxy.<br />

Owners of large Dobsonian telescopes<br />

should challenge themselves not only by trying<br />

to see this fascinating system, but also by hunting<br />

down the numerous anonymous galaxies we can<br />

see around and through it. Do not be intimidated<br />

by their minuscule photographic appearance or<br />

by the fact that they are not plotted on the<br />

Millennium Star Atlas. <strong>The</strong>y should be readily<br />

visible at the eyepiece of a large reflector.<br />

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

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