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Explanation: Why isn't the star in the center of the nebula? NGC 6369 appears to be a fairly ordinary planetary nebula. It can be seen with a good telescope in the constellation of Ophiuchus. The gas expelled by the central star is bunched in the shape of a donut or cylinder. During the planetary nebula phase, the central star sheds its outer atmosphere as it is evolving to become a white dwarf star. The above image was taken with the Hubble Space Telescope. A closer look at NGC 6369 indicates that the central star is closer to a dimmer edge of the nebula than to the opposing brighter edge.
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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: nebula
Publications with words: nebula
See also:
- APOD: 2025 July 5 Á Ou4: The Giant Squid Nebula
- APOD: 2025 March 18 Á LDN 1235: The Shark Nebula
- APOD: 2024 June 11 Á Colorful Stars and Clouds near Rho Ophiuchi
- APOD: 2024 January 23 Á Deep Nebulas: From Seagull to California
- APOD: 2023 June 14 Á The Shark Nebula
- NGC 7380: The Wizard Nebula
- A Galaxy Beyond Stars, Gas, Dust