M3 (NGC 5272)
M3. Image credit: NOAO/AURA/NSF.
M3 (NGC 5272) is one of the largest and brightest of the 250 or so known globular clusters in the Milky Way Galaxy. M3 contains approximately 500,000 stars, is easily visible with binoculars, and can even be seen with the unaided eye on a clear, dark night. It lies in the constellation Canes Venatici.
M3 has an age of roughly 8 billion years and contains mostly old, red stars. The existence within it of a number of young blue stars was once puzzling to astronomers, but these so-called blue stragglers are now thought to form as a result of stellar interactions.
|linear diameter||180 light-years (55 pc)|
|distance||34,000 light-years (10,400 pc)|
|position||RA 13h 42m 11s,
Dec -28° 22' 32"
|other designations||GCl 25, C 1339+286|
|In this color-magnitude diagram of M3, apparent magnitude, v, is plotted against the color index (B-V). The RR Lyrae variables, used to measure the distance of the cluster, lie at v = 15.7 – the gap in the horizontal branch.