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A smattering of stars against a black background.
Hubble · Messier 48 · NASA, ESA, A. Riess (The Johns Hopkins University): Processing: Gladys Kober (NASA/Catholic University of America)

Messier 48

Star cluster in Hydra · 1,500 light-years

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TypeStar cluster
ConstellationHydra
Right ascension8h 13m 43s
Declination−5° 45′
Object distance1,500 light-years
Apparent magnitude5.8
Apparent size28.2′ (arc-minutes)
Approx. true diameter12.3 light-years across
Also known asM48 · NGC 2548
Messier 48 is a star cluster (also catalogued as NGC 2548) in Hydra — 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 28.2 arc-minutes on the sky. At about magnitude 5.8, it is an easy target for binoculars and small telescopes.

Although it appears about 28.2′ wide on the sky, its real span is roughly 12.3 light-years — the difference is a measure of how far away it lies.

Observing Messier 48

Messier 48 lies in the constellation Hydra and is best placed in the evening sky around January. Its maximum altitude above the horizon depends on your latitude. Lying near the celestial equator, it can be seen from both hemispheres. It is a comfortable target for binoculars and small telescopes.

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