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A splotch of stars sits at the center of the image. Its bright-white core is filled with stars. White, yellow-orange, and blue stars dot the view beyond the bright core.
Hubble · Messier 75 · ESA/Hubble & NASA, F. Ferraro et al.

Messier 75

Star cluster in Sagittarius · 67,500 light-years

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TypeStar cluster
ConstellationSagittarius
Right ascension20h 06m 05s
Declination−21° 55′
Object distance67,500 light-years
Apparent magnitude8.3
Apparent size3.6′ (arc-minutes)
Approx. true diameter70.7 light-years across
Also known asM75 · NGC 6864
Messier 75 is a star cluster (also catalogued as NGC 6864) in Sagittarius — a gravitationally bound family of stars sharing a common origin. It was recorded by Charles Messier in his famous catalogue of 110 deep-sky objects. It spans roughly 3.6 arc-minutes on the sky. At about magnitude 8.3, it shows up well in a small backyard telescope.

Although it appears about 3.6′ wide on the sky, its real span is roughly 70.7 light-years — the difference is a measure of how far away it lies.

Observing Messier 75

Messier 75 lies in the constellation Sagittarius and is best placed in the evening sky around July. Its maximum altitude above the horizon depends on your latitude. It is best placed for observers in the southern hemisphere, and sits low for those far north. A small backyard telescope will show it; binoculars may hint at it under dark skies.

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Sources

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