Universe FinderFly · Explore · Discover
2MASS near-infrared telescope survey centred on Owl Nebula
Owl Nebula · Telescope survey view · 2MASS · University of Massachusetts and IPAC/Caltech; funded by NASA and NSF. Colour mosaic and cutout: CDS/Aladin.

Owl Nebula

Nebula in Ursa Major · 2,030 light-years

🔭 Explore Owl Nebula in the 3D map →View Owl Nebula images →
TypeNebula
ConstellationUrsa Major
Right ascension11h 14m 48s
Declination+55° 01′
Object distance2,030 light-years
Apparent magnitude9.9
Apparent size3.6′ (arc-minutes)
Approx. true diameter2.1 light-years across
Also known asM97 · NGC 3587
Messier 97, popularly known as the Owl Nebula, is a nebula (also catalogued as NGC 3587) in Ursa Major — a glowing cloud of interstellar gas and dust. 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 9.9, it shows up well in a small backyard telescope.

Although it appears about 3.6′ wide on the sky, its real span is roughly 2.1 light-years — the difference is a measure of how far away it lies.

Observing Owl Nebula

Owl Nebula lies in the constellation Ursa Major and is best placed in the evening sky around March. Its maximum altitude above the horizon depends on your latitude. It is best placed for observers in the northern hemisphere, and sits low for those far south. A small backyard telescope will show it; binoculars may hint at it under dark skies. Note that the listed magnitude is spread across the whole object — diffuse galaxies and nebulae are often harder to see than the number alone suggests, so dark, moonless skies help a great deal.

See Owl Nebula in Universe Finder

Open the interactive 3D map to fly to Owl Nebula and see it in context among the real stars around it. Launch the 3D view →

Sources

Related objects