Messier 75
This globular cluster holds roughly 400,000 stars.
Distance
67,500 light-years
Apparent Magnitude
8.6
constellation
Sagittarius
object type
Globular Cluster
This beautiful image features the globular star cluster M75. Pierre Méchain discovered M75 in August of 1780. Charles Messier observed the cluster in October 1780 and added it to his catalog after determining its position.
Located in the western part of Sagittarius, M75 has a magnitude of 8.6. The cluster holds some 400,000 stars and is surprisingly easy to see in binoculars and telescopes thanks to its extremely condensed center of stars. However, because of its compact nature, M75 looks very similar to a star when viewed in binoculars. Telescopes 10 inches across or larger should be able to resolve some of the stars in the cluster. September is the best month to observe M75.

M75 is the most centrally concentrated globular cluster in Messier’s catalog, with the majority of its stars located in a large nucleus. Astronomers think M75 is around 13 billion years old and is located approximately 67,500 light-years away from Earth.
For more information about Hubble's observations of M75, see:
Explore Hubble's Messier Catalog
The following pages contain some of Hubble’s best images of Messier objects.

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