Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  HD119391  ·  M 3  ·  NGC 5272
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Messier 3, jrtb
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Messier 3

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Messier 3, jrtb
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Messier 3

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Description

Messier 3 (M3) is a globular cluster in the constellation Canes Venatici. It was discovered by Charles Messier in 1764 and was the first astronomical object that he discovered himself.

Globular clusters are spherical collections of stars that orbit a galaxy's core. M3 is one of the largest and brightest globular clusters, containing an estimated half a million stars, and it's located about 33,900 light-years away from Earth. It has a diameter of about 180 light years.

M3 is one of the most studied globular clusters, and observations have detected a high rate of variable stars (stars that fluctuate in brightness). Nearly 274 variable stars are known in M3, which is more than in any other known globular cluster. These variable stars are important because their periodic fluctuations in brightness provide astronomers with a tool to measure distances.

As it is one of the most prominent and well-studied globular clusters, it is often featured in educational content relating to astronomy. However, due to its more subtle appearance compared to galaxies and nebulae, it does not feature as frequently in popular culture. Nonetheless, for stargazers and amateur astronomers, M3 is a popular object to observe, especially in the Northern Hemisphere's spring months.

36 x 180 second exposures for 1:48 of total integration, shot across 2 nights

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Messier 3, jrtb