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M107
Hubble · Messier 107 · ESA/Hubble & NASA

Messier 107

Star cluster in Ophiuchus · 20,900 light-years

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TypeStar cluster
ConstellationOphiuchus
Right ascension16h 32m 32s
Declination−13° 03′
Object distance20,900 light-years
Apparent magnitude8.8
Apparent size7.8′ (arc-minutes)
Approx. true diameter47.4 light-years across
Also known asM107 · NGC 6171
Messier 107 is a star cluster (also catalogued as NGC 6171) in Ophiuchus — 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 7.8 arc-minutes on the sky. At about magnitude 8.8, it shows up well in a small backyard telescope.

Although it appears about 7.8′ wide on the sky, its real span is roughly 47.4 light-years — the difference is a measure of how far away it lies.

Observing Messier 107

Messier 107 lies in the constellation Ophiuchus and is best placed in the evening sky around May. Its maximum altitude above the horizon depends on your latitude. Lying near the celestial equator, it can be seen from both hemispheres. A small backyard telescope will show it; binoculars may hint at it under dark skies.

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Sources

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