‘Dark Markings of the Sky’ are Hiding Star Formation

by Nancy Atkinson on February 15, 2012

Want to stay on top of all the space news? Follow @universetoday on Twitter

This image from the APEX telescope, part of the Taurus Molecular Cloud, shows a sinuous filament of cosmic dust more than ten light-years long. Credit: ESO/APEX (MPIfR/ESO/OSO)/A. Hacar et al./Digitized Sky Survey 2. Acknowledgment: Davide De Martin.

This stunning new image shows a sinuous filament of cosmic dust more than ten light-years long. The makeup of filamentary cloud structures like this used to be a mystery, and in the early 20th century, Edward Emerson Barnard compiled a photographic atlas of these features, calling them “dark markings of the sky,” as these regions appeared as dark lanes, with no stars visible. Barnard correctly argued that this appearance was due to “obscuring matter in space.” Today we call segments in this particular cloud Barnard 211 and Barnard 213, or the Taurus Molecular Cloud. And we now know that these are clouds of interstellar gas and dust grains. But also, within these clouds, newborn stars are hidden, and dense clouds of gas are on the verge of collapsing to form yet more stars.

The Taurus Molecular Cloud is one of the closest regions of star formation to us. It is located in the constellation of Taurus about 450 light-years from Earth. The cosmic dust grains are so cold that observations at wavelengths of around one millimeter, such as these made with the LABOCA camera on APEX (Atacama Pathfinder Experiment) telescope in Chile, are needed to detect their faint glow.

This image shows two parts of a long filament. The dust grains — tiny particles similar to very fine soot and sand — absorb visible light, blocking our view of the rich star field behind the clouds. The Taurus Molecular Cloud is particularly dark at visible wavelengths, as it lacks the massive stars that illuminate the nebulae in other star-formation regions such as Orion.

But active star formation is taking place. This is why observations at longer wavelengths, such as the millimeter range, are essential for understanding the early stages of star formation.

Read more about this particular region at the ESO website.

About 

Nancy Atkinson is Universe Today's Senior Editor. She also is the host of the NASA Lunar Science Institute podcast and works with Astronomy Cast. Nancy is also a NASA/JPL Solar System Ambassador.

lcrowell February 16, 2012 at 3:39 PM

The APEX (Atacama Pathfinder Experiment) is pretty robust in looking at star systems. We may find that star formation is more common than thought. A lot of it may not be associated with rapid starburst activity. Much of it may be fairly staid and subdued, and occurring in dark clouds or what I think used to be called coal sacks.

The picture here is a keeper.

LC

ITSRUF February 19, 2012 at 5:32 PM

“The picture here is a keeper.”
Agreed.
When I first looked at it, I was expecting to see that it was an artist’s impression.

johnjean3943 February 19, 2012 at 6:06 AM

Among that beautiful lights from stars there is still big mystery behind. There are still black holes and etc. behind there.

Facts About Earth

Comments on this entry are closed.

Previous post:

Next post: