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h and chi Persei
The double cluster in the constellation Perseus, normally known by its Greek designation transliterated. chi Persei (NGC884, on the left) and h Persei (NGC869) are about 7000 light-years away and less than 100 light-years apart. Although open clusters are quite common, this pair is exceptional due to the large number of young bright O and B stars in each, and their closeness whilst still being clearly distinguished. This color picture was made from CCD images taken in September 1997 at the Burrell Schmidt telescope of the Warner and Swasey Observatory of the Case Western Reserve University, located on Kitt Peak in southwestern Arizona.
Créditos:N.A.Sharp/NOIRLab/NSF/AURA
About the Image
Id: | noao-hcper |
Tipo: | Observation |
Release date: | 30 de Junio de 2020 a las 21:34 |
Size: | 4050 x 2732 px |
Sobre el Objeto
Nombre: | chi Persei, h Persei, NGC 869, NGC 884 |
Constellation: | Perseus |
Categoría: | Star Clusters |
Formatos de Imágenes
Large JPEG
5,5 MB
Publication TIFF 4K
24,2 MB
Publication JPEG
5,2 MB
Screensize JPEG
449,6 KB
Fondos de Pantalla
1024x768
592,4 KB
1280x1024
919,4 KB
1600x1200
1,3 MB
1920x1200
1,5 MB
2048x1536
6,0 MB
Coordenadas
Posición (AR): | 2 22 20.46 |
Posición (Dec): | 56° 51' 0.55" |
Campo visual: | 68.53 x 46.23 arcminutes |
Orientación: | North is 1.5° left of vertical |