Messier 68

Hubble captured this globular cluster's core at visible and infrared wavelengths of light.

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33,000 light-years

Apparent Magnitude




object type

Globular Cluster

ESA/Hubble & NASA

Discovered by Charles Messier in 1780, M68 is a dense collection of stars known as a globular cluster. Mutual gravitational attraction amongst the hundreds of thousands or even millions of stars in such a cluster keeps stellar members packed tightly together for many billions of years.

Roughly 150 of these objects reside in our Milky Way galaxy. On a galactic scale, globular clusters are relatively small. In M68’s case, its constituent stars span a volume of space with a diameter of little more than a hundred light-years. The disk of the Milky Way, on the other hand, extends over 100,000 light-years.

M68 is located 33,000 light-years from Earth in the constellation Hydra. It has an apparent magnitude of 8 and can be spotted with a pair of binoculars. The cluster is best observed during April.

This Hubble image of the core of M68 was created using observations at visible and infrared wavelengths of light.

For more information about Hubble’s observations of M68, see:

locator star chart for M68
This star chart for M68 represents the view from mid-northern latitudes for the given month and time.
Image courtesy of Stellarium

Explore Hubble's Messier Catalog

The following pages contain some of Hubble’s best images of Messier objects.

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Messier 3

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