M3

This ball of 500,000 stars is approximately 100 light years across. From a galactic perspective, this cluster is passing over our heads (galactic north) and is one of the first bright clusters to become available before the others closer to the galactic center. Some people believe that this cluster inspired Charles Messier to begin systematically recording the location of deep sky objects that through his telescope appeared as nebulous. Charles Messier was interested in finding comets and considered these non-comet fuzzies to be a bit of a distraction. Even with modest equipment today, the true nature of these objects are easily revealed.

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.

Créditos:

KPNO/NOIRLab/NSF/AURA/Michael Schock/Flynn Haase

About the Image

Id:noao-m3schock
Tipo:Observation
Release date:24 de Junio de 2014 a las 08:35
Size:1800 x 1263 px

Sobre el Objeto

Nombre:M3
Constellation:Canes Venatici
Categoría:Star Clusters

Formatos de Imágenes

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719,1 KB
Screensize JPEGScreensize JPEG
299,6 KB

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Coordenadas

ObjectValue
Posición (AR):13 41 35.76
Posición (Dec):28° 20' 12.07"
Campo visual:20.96 x 14.69 arcminutes
Orientación:North is 157.2° right of vertical


Colores y Filtros

BandaLongitud de OndaTelescopio
Optical
B
438 nmVisitor Center 0.5-meter Telescope
Other CCD
Optical
G
475 nmVisitor Center 0.5-meter Telescope
Other CCD
Optical
R
625 nmVisitor Center 0.5-meter Telescope
Other CCD