Friday, April 17, 2015

A Double Star Cluster

A Double Star Cluster: APOD: 2013 January 1 - A Double Star Cluster


Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

2013 January 1


See Explanation. Clicking on the picture will download the highest resolution version available.
A Double Star Cluster

Image Credit & Copyright: F. Antonucci, M. Angelini, & F. Tagliani, ADARA Astrobrallo
Explanation: Few star clusters are seen to be so close to each other. Some 7,000 light-years away, though, this pair of open or galactic star clusters is an easy binocular target, a lovely starfield in the northern constellation Perseus. Also visible to the unaided eye from dark sky areas, it was cataloged in 130 BC by Greek astronomer Hipparchus. Now known as h and chi Persei, or NGC 869 (above right) and NGC 884, the clusters themselves are separated by only a few hundred light-years and contain stars much younger and hotter than the Sun. In addition to being physically close together, the clusters' ages based on their individual stars are similar - evidence that both clusters were likely a product of the same star-forming region.

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