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A cometary globule shows its true color.

Breaking up is not hard to do -- at least not if you're a tiny interstellar cloud constantly pounded by radiation from hot, nearby stars. For the first time, astronomers have captured a color image of such a faint cloud, caught in the act of coming apart.

This Milk Way resident, called a cometary globule because it sports a comet-like tail of gas and dust dragged out by the bombardment of starlight, lies about 100 light-years from Earth. And in reflecting light from nearby stars, it exhibits a variety of colors that reveal much about its own composition as well as the influence of its surroundings, says David Malin of the Anglo-Australian Observatory in Epping, Australia.

Malin became interested in a cometary globule called CG4 when photographs taken with the United Kingdom Schmidt Telescope in Epping showed that the object appeared dramatically different depending on whether it was viewed through a red or a blue filter. This suggested that CG4 might display an unusual array of colors. Images taken by Malin late last year with color filters at the 3.9-meter Anglo-Australian Telescope in Coonabarabran confirmed that hunch, he says.

Malin reported his results this week at a meeting of the Royal Astronomical Soceity in Durham, England.

Unlike the majority of interstellar clouds, which serve as nurseries for new stars and measure some 10 to 30 light-years across, most cemeary globules span only about one-tenth that distance and lack sufficient gas and dust to form stars. The globules become visible when background stars lie near enough to illuminate them. Each color reflected by the clouds -- pale hues of red, blue and green -- tells a separate story.

For instance, the blue coloring of CG4's tail indicates the presence of tiny dust particles -- less than a millionth of a meter in diameter -- that scatter blue light preferentially, Malin says.

The faint red glow near the center of CG4 reveals a violent, two-step process that over millions of years contributes to the total destruction of the cloud, he adds. Radiation from nearby stars heats up molecular bonds in the cloud, breaking them apart and liberating atomic hydrogen. The radiation is so intense, it also ionizes the released hydrogen, producing the red glow. While astronomers had conjectured that light from surrounding stars might release hydrogen, they hadn't expected it to have enough energy to ionize it, Malin says.

He adds that the yellow-green regions of CG4 reveal red-absorbing dust particles that lie between the cloud and Earth.

Malin constructed the color image from three black-and-white negatives of CG4 taken through different filters. Because the cloud, which lies in the southern constellation Puppis, extends some 20 arc-minutes across the sky, he chose large-formet photographic plates -- 25 centimeters to a side -- to make the images. In contrast, the solid-state light detectors known as charged-coupled devices are about the size of a postage stamp and cannot easily record faint, extended objects, he notes.

Millions of years from now, says Malin, after neighboring stars have died and the contents of CG4 have completely dispersed, some of its molecules may come together again elsewhere in the galaxy, perhaps to start anew as yet another interstellar cloud.
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Author:Cowen, Ron
Publication:Science News
Date:Apr 11, 1992
Words:526
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