Explanation: Few star clusters this close to each other. Visible to the unaided eye from dark sky areas, it was cataloged in 130 BC by Greek astronomer Hipparchus. Some 7,000 light-years away, this pair of open star clusters is also an easy binocular target, a striking starfield in the northern constellation of the mythical Greek hero Perseus. 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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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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NASA Official: Jay Norris. Specific rights apply.
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& Michigan Tech. U.

Publikacii s klyuchevymi slovami: open cluster - Rasseyannoe skoplenie Publikacii so slovami: open cluster - Rasseyannoe skoplenie
Sm. takzhe: Dvoinoe skoplenie v Persee Pleyady: zvezdnoe skoplenie Sem' sester NGC 7380: tumannost' Koldun NGC 3572 i Yuzhnye Golovastiki M44: skoplenie Ulei Tri skopleniya v Korme V serdce tumannosti Serdce Vse publikacii na tu zhe temu >>