M3, NGC 5272

This image was obtained with the wide-field view of the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory. M3 is a giant globular cluster that consists of several hundred thousand stars. It is slightly larger and more distant than M13. Like in all globular clusters, the stars are all old. Because the core of the cluster is very bright, many short exposures had to be taken so that it would not be over exposed. The image was generated with observations in B (blue), V (green) and I (red) filters. In this image, North is left, East is down.

Créditos:

T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOIRLab/NSF/AURA)

About the Image

Id:noao-m3-kpno-mayall-4-m
Tipo:Observation
Release date:30 de Junio de 2020 a las 21:34
Size:4929 x 4928 px

Sobre el Objeto

Nombre:M3, NGC 5272
Constellation:Canes Venatici
Categoría:Star Clusters

Formatos de Imágenes

Large JPEGLarge JPEG
11,5 MB
Screensize JPEGScreensize JPEG
353,3 KB

Zoomable


Fondos de Pantalla

1024x7681024x768
332,2 KB
1280x10241280x1024
488,3 KB
1600x12001600x1200
664,6 KB
1920x12001920x1200
794,1 KB
2048x15362048x1536
4,6 MB

Coordenadas

ObjectValue
Posición (AR):13 42 4.60
Posición (Dec):28° 20' 54.57"
Campo visual:21.50 x 21.56 arcminutes
Orientación:North is 90.0° left of vertical


Colores y Filtros

BandaLongitud de OndaTelescopio
Optical
B
436 nmNicholas U. Mayall 4-meter Telescope
Mosaic I
Optical
V
537 nmNicholas U. Mayall 4-meter Telescope
Mosaic I
Optical
I
805 nmNicholas U. Mayall 4-meter Telescope
Mosaic I