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What Herschel Found in a Dark Cloud


A thousand light years away in the constellation of Aquila the Eagle lies a great dark cloud. This cloud (called a nebula) stretches between the stars for some some 65 light years - that's over sixteen times the diameter of our solar system.

Dust completely conceals the interior of this nebula. At least it did until the end of 2009 when the Herschel Space Observatory was able to penetrate the dust to photograph it for the first time. What astronomers found is a stellar nursery, a place where new stars are forming.

A dark nebula is a good place for star formation. Although the material in a nebula is diffuse, it's there in great quantities. A triggering event of some kind, such as a nearby supernova explosion, can cause the cloud to become unstable and start collapsing under its own gravity. It breaks up into fragments which then continue to collapse, becoming denser as they evolve into stars.

Inside the Eagle's nebula astronomers have found six hundred of these condensed regions that will become stars. After some ten thousand years an embryo star, called a protostar, forms in the center of the condensation, giving out heat and light. When it becomes hot enough to sustain nuclear fusion, it becomes a true star.

The Herschel photograph shows these future stars embedded in dark filaments, but hot young stars are already illuminating the nebula to produce two bright regions.

But how did Herschel see through the dust when other instruments couldn't?

Our eyes can't see through dust and neither can telescopes that detect visible light. However light comes in many wavelengths that are invisible to our eyes, including the longer wavelengths of infrared and submillimeter. These can penetrate dust and also see the cooler part of the universe, such as the star-forming regions, which radiate at these wavelengths.

Earth-based telescopes can't detect this light because our atmosphere absorbs it. However Herschel's sensitive instruments can see the entire spectrum of the far infrared and submillimeter radiation, the first to do so.

Herschel was launched in May 2009 by the European Space Agency (ESA), the largest telescope ever sent into orbit. At 3.5 meters (about eleven and a half feet) the main mirror is 0.9 meter (almost three feet) greater in diameter than that of the Hubble Space Telescope.

The telescope was named for William and Caroline Herschel. They were German-born, but worked in England in the seventeenth and eighteenth centuries. William was the discoverer of the planet Uranus and also of infrared radiation. With the assistance of his sister Caroline, he laid the foundations for modern astronomy. Caroline, who was the first woman to discover a comet, got her brother interested in nebulae. Together they surveyed the sky and cataloged the nebulae of the northern hemisphere.

The Herschel Space Observatory has been studying low-temperature objects to help us understand, amongst other things, how stars and galaxies form and evolve, and the chemistry of nebulae.

On April 29, 2013 the mission ended when the infrared observatory finally exhausted its helium coolant.

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Content copyright © 2014 by Mona Evans. All rights reserved.
This content was written by Mona Evans. If you wish to use this content in any manner, you need written permission. Contact Mona Evans for details.

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