Well positioned in the evening sky for viewers in the northern hemisphere, Messier 2, also known as NGC 7089, is one of the largest globular clusters known, with about 150,000 stars stretching across 175 light years. Thought to be about 13 billion years old, the cluster’s eccentric orbit carries it as far as 171,000 light years from the center of the Milky Way and up to 165,000 light years above and below the galactic plane. Currently about 55,000 light years from Earth in the constellation Aquarius, M2 was discovered by the French astronomer Jean-Dominique Maraldi in 1746 and added to Charles Messier’s famous list in 1760. It is visible to the unaided eye on extraordinarily clear nights and easily resolved into a spectacular star swarm in moderate-size telescopes. As viewed by the Hubble Space Telescope, as seen here, M2 is nothing short of jaw dropping, with a dense core of close-packed stars.
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A research team has used the NASA/ESA Hubble Space Telescope’s Cosmic Origins Spectrograph to study a body known as BD+44°493, the brightest known second-generation star in the sky. BD+44°493 is thought to have been enriched by elements from one of the first generation of stars and the researchers detected several elements that had never been seen before in such a star.