Globular cluster in the constellation Canes Venatici.
Messier 3 (M3 or NGC 5272) is a galactic globular cluster in the constellation Canes Venatici in the northern starry sky.
Object: | M3 Globular Cluster |
Date of exposures: | 23.03.2022 |
Distance: | 34.000 Lightyears |
Exposures: | L: 60 x 180 Sec., RGB: 81 x 180 Sec., Sum: 7,05 hrs. |
Telescope: | 10'', F4 Newton |
Focal length: | 1000 mm |
Camera: | ASI 1600 MMC Pro |
Guiding: | Off Axis Guider, Lodestar |
Mount: | EQ8 |
It is about 34,000 light-years away from the solar system, has a diameter of about 125 light-years and is a very large globular cluster with half a million stars. The cluster contains with 212 variable stars (170 of them RR Lyrae stars) the largest number of this star class in our galaxy. Out of 186 stars one period could be determined.
The object was discovered by Charles Messier on May 3, 1764 and listed by him in his catalog as the third object. In the New General Catalogue (NGC) it has the number 5272.