Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ViaLattea/ngc6791_kpno_big.html
Дата изменения: Fri Mar 2 19:35:56 2001
Дата индексирования: Sat Dec 22 09:12:28 2007
Кодировка:

Поисковые слова: m 11
APOD: 2000 January 12 - NGC 6791: An Old, Large Open Cluster

Astronomy Picture of the Day

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.

2000 January 12

NGC 6791: An Old, Large Open Cluster
Credit: Barbara J. Mochejska (CAMK) et al., 2.1-m Telescope, KPNO, NOAO, NSF

Explanation: NGC 6791 is one of the oldest and largest open clusters of stars known. But how did it get so dirty? Open star clusters usually contain a few hundred stars each less than a billion years old. Open star cluster NGC 6791, however, contains thousands of stars recently measured to be about 8 billion years old. What's really confusing, though, is that the stars of NGC 6791 are relatively dirty - the minuscule amounts of heavy elements (generically called metals) are high relative to most other star clusters. Older stars are supposed to be metal poor, since metals have only been slowly accumulating in our Milky Way Galaxy. This enigma makes NGC 6791, pictured above, one of the most studied open clusters and a possible example of how stars might evolve in the centers of galaxies.

Tomorrow's picture: A Skygazer's Moon


< | Archive | Index | Search | Calendar | Glossary | Education | About APOD | >

Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Technical Rep.: Jay Norris. Specific rights apply.
A service of: LHEA at NASA/ GSFC
& Michigan Tech. U.