Cocoon Nebula

Like a cosmic butterfly, a cluster of young stars is just emerging from its cocoon – a cloud of gas and dust. The cocoon `spans about 45 light-years. But some of the beautiful butterfly is already in view. Parts of the gas cloud are lit up by the brightest of the infant stars taking shape there. That creates a glowing patch of red and blue. The whole complex is known as the Cocoon Nebula. It’s about 4,000 light-years away, in Cygnus. Hundreds of stars are being born inside it. The most impressive of those stars is about 14 times as massive as the Sun, and tens of thousands of times brighter. It’s especially bright in the ultraviolet – wavelengths that are invisible to the human eye. The U-V zaps atoms of hydrogen in the nebula, splitting them apart. When the atoms re-combine, they emit red light – the main color of the nebula. The hot star also illuminates dust grains in the nebula. It doesn’t set them aglow; instead, the light simply reflects off the grains. That colors the blue parts of the nebula. Less-massive stars – stars like the Sun or even smaller – are still coming together. They won’t shine as fully formed stars for millions of years. The Cocoon Nebula is low in the northeast at nightfall. It’s to the lower left of the bright star Deneb, which marks the tail of the swan. The nebula is too faint to see with the eye alone. Script by Damond Benningfield