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Cygnus OB2 Animations
Click for low-resolution animation
Tour of Cygnus OB2
Quicktime MPEG
The Milky Way and other galaxies in the universe are home to many star clusters and associations that each contain hundreds to thousands of hot, massive, young stars. Astronomers would like to better understand how these star factories form and evolve over time. Cygnus OB2 is the closest massive star cluster to Earth, making it an excellent target for astronomers to study. A long observation from NASA's Chandra X-ray Observatory of Cygnus OB2 revealed about 1,700 X-ray sources. Scientists think that nearly 1,500 of these X-ray sources are young stars. The X-ray emission comes from the hot outer atmospheres of these stars ranging in age from one million to seven million years old. This makes the stars in Cygnus OB2 practically newborn babies when compared to a star like our Sun at about 5 billion years in age. By combining Chandra's data with those from other telescopes, a more complete story of star birth and early adolescence is made.
[Runtime: 01:11]

(Credit: NASA/CXC/A. Hobart)


Click for low-resolution animation
A Field Trip to Star School
Quicktime MPEG
If you wanted to learn about young people, you would probably visit a school where there are lots of young people, right? This photograph shows a star "school" - home to over a thousand of the biggest and brightest young stars in the sky. When astronomers want to study young stars, this cluster - called Cygnus OB2 - is one of the first places they look.

Cygnus OB2 is the largest star cluster in the northern half of the sky, containing about 30,000 times as much material as the Sun! This cluster also happens to be one of the closest to Earth. So why didn't you hear about this before? Well, it is almost completely hidden behind a massive dust cloud. To study it, astronomers have to use telescopes that can "see" in X-ray and infrared light. These types of light can go through the thick dust that is impenetrable for visible light.

One of the most interesting - but unfortunate! - discoveries that astronomers made while studying the massive, young stars in this cluster, is that most of them will host fewer planets than their brothers and sisters in less massive clusters. Some might not host planets at all!

When a star forms, there is always some material left over. This becomes a disc of dust and dirt, like a thicker version of Saturn's rings. Within this disc, small dust grains made of rock and ice can form, and these sometimes merge together into larger and larger objects - imagine rolling a snowball around in the snow: it becomes bigger and bigger as it collects snow. This is how planets are born.

Massive, young stars however, can destroy the dusty discs of their lower-mass neighbors with their intense energy spatting out, long before any planets might be born!
[Runtime: 02:20]

(Credit: NASA/CXC/April Jubett)


Return to Cygnus OB2 (November 7, 2012)