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Explanation: What's happening in the center of nearby spiral galaxy M77? The face-on galaxy lies a mere 47 million light-years away toward the constellation of the Sea Monster (Cetus). At that estimated distance, this gorgeous island universe is about 100 thousand light-years across. Also known as NGC 1068, its compact and very bright core is well studied by astronomers exploring the mysteries of supermassive black holes in active Seyfert galaxies. M77's active core glows bright at x-ray, ultraviolet, visible, infrared, and radio wavelengths. The featured sharp image of M77 was taken by the Hubble Space Telescope. The image shows details of the spiral's winding spiral arms as traced by obscuring red dust clouds and blue star clusters, all circling the galaxy's bright white luminous center.
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: spiral galaxy
Publications with words: spiral galaxy
See also:
- Portrait of NGC 1055
- APOD: 2025 September 4 B NGC 4565: Galaxy on Edge
- APOD: 2025 August 22 B A Tale of Two Nebulae
- APOD: 2025 August 19 B Giant Galaxies in Pavo
- APOD: 2025 August 18 B NGC 1309: A Useful Spiral Galaxy
- APOD: 2025 July 4 B NGC 6946 and NGC 6939
- APOD: 2025 June 30 B NGC 4651: The Umbrella Galaxy