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The Caldwell Objects

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77<br />

of the nebulous matters between them. <strong>The</strong>re is a very<br />

minute star in the dark space between the preceding<br />

extremities of the nebula: they are extended in the<br />

parallel of the equator nearly.<br />

Several years later John Herschel would call<br />

NGC 5128 "a very problematic object" that "must<br />

be regarded at present to form a genus apart,<br />

since it evidently differs from mere 'double<br />

nebulae,' not only in the singular relation of its<br />

two halves to each other, (having each a well and<br />

an illdefined side, their sharply terminated edges<br />

being turned towards each other and exactly<br />

parallel) but also by the intervention of the<br />

delicate nebulous streak intermediate between<br />

them and lying in exactly the same general<br />

direction."<br />

How bizarre this new nebula must have<br />

seemed to John Herschel, who, like his father,<br />

believed that the Milky Way and all its nebulae<br />

were made up of noth<br />

ing but stars. What was<br />

the dark band that had<br />

seemingly ripped apart<br />

this cloud? In his 1849<br />

'Outlines of Astronomy"<br />

Herschel prophetically<br />

decided that it was a<br />

"similar but much more<br />

strongly marked case of<br />

parallel arrangement<br />

than that noticed by Mr<br />

Bond (in the Andromeda<br />

Nebula) . . . one in which<br />

two semi-ovals of an<br />

elliptically formed<br />

nebula appear cut<br />

asunder and separated<br />

by a broad obscure band<br />

parallel to the larger axis<br />

of the<br />

306<br />

nebula, in the midst of which a faint streak of<br />

light parallel to the sides of the cut appears."<br />

Herschel's reference to George P Bond . was critical,<br />

for Bond had observed in 1847 two parallel<br />

dark "canals" in the Andromeda "Nebula" — one<br />

of the last strongholds of William's Herschel's<br />

nebular theory, which stated that these masses of<br />

nebulous matter were in the process of becoming<br />

new solar systems. By 1888 Isaac Roberts had<br />

successfully photographed the dark lanes in the<br />

Andromeda "Nebula," as did Edward Emerson<br />

Barnard two years later. Soon these features<br />

would be recognized as dust lanes, part of the<br />

visible framework not of spiral nebulae but of<br />

spiral galaxies.<br />

Still, NGC 5128's appearance and nature<br />

remained a mystery. In 1918, Heber D. Curtis<br />

(Lick Observatory) classified it as an "edgewise<br />

spiral with a dark lane." Five-hour exposures<br />

taken of it from Arequipa, Peru, with the<br />

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

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