Messier 70 (M70) is a compact globular star cluster in the constellation Sagittarius, located about 29,000 light-years away and known for its extremely dense core, a result of "core collapse". Discovered by Charles Messier in 1780, it appears as a fuzzy ball in binoculars and is best viewed with a telescope, which can resolve individual stars, especially in its bright core. It's found near the "Teapot" asterism, close to other clusters like M69 and M54.
Type: Globular cluster (NGC 6681)
Location: Constellation Sagittarius, near the "Teapot" asterism
Distance: Approximately 29,000 light-years from Earth
Appearance: A compact, fuzzy ball with a very bright, dense core, visible in telescopes
Special Feature: Has undergone core collapse, making its center exceptionally dense with stars
Locate the "Teapot" in Sagittarius.
Find M70 on the bottom edge of the teapot, between the stars Kaus Australis and Ascella.
It is best observed in the summer months (June, July, August). Image Credit ESA/Hubble & NASA
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