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Explanation: The dark dusty Keyhole Nebula gets its name from its unusual shape. Officially designated NGC 3324, the Keyhole Nebula is a smaller region superposed on the larger Eta Carina Nebula. These nebulae were created by the dying star Eta Carina, which is prone to violent outbursts during its final centuries. Noted and discussed as early as 1840 when a spectacular explosion became visible, the Eta Carina system now appears to be undergoing an unusual period of change. An emission nebula that contains much dust, the Keyhole Nebula is roughly 9,000 light years distant. This photogenic nebula can be seen in the south with even a small telescope. The Keyhole Nebula was recently discovered to contain highly structured clouds of molecular gas.
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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 - dark nebula - emission nebula - Keyhole Nebula - Eta Carinae
Publications with words: nebula - dark nebula - emission nebula - Keyhole Nebula - Eta Carinae
See also:
- APOD: 2025 March 18 Á LDN 1235: The Shark Nebula
- APOD: 2025 February 18 Á Thors Helmet versus the Seagull
- APOD: 2025 February 11 Á The Spider and the Fly
- APOD: 2024 December 17 Á Near to the Heart Nebula
- The Elephant s Trunk in Cepheus
- IC 348 and Barnard 3
- APOD: 2024 October 27 Á LDN 43: The Cosmic Bat Nebula