The Bubble Nebula | Hubble’s Inside the Image
In this video, Dr. Ken Carpenter dives into the mesmerizing details of the Bubble Nebula and discusses how Hubble's observations continue to reveal the intricate beauty and complexity of the universe.
The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8,000 light-years away. It is also referred to as Sharpless 162, or Caldwell 11. It is an H II region emission nebula in the constellation Cassiopeia. It lies close to the direction of the open cluster Messier 52. The "bubble" is created by the stellar wind from a massive hot, 8.7 magnitude young central star, SAO 20575 (BD+60°2522).
The nebula is near a giant molecular cloud which contains the expansion of the bubble nebula while itself being excited by the hot central star, causing it to glow. It was discovered in 1787 by William Herschel.
Credit: NASA's Goddard Space Flight Center
Producer, Director & Editor: James Leigh
Director of Photography: James Ball
Executive Producers: James Leigh & Matthew Duncan
Production & Post: Origin Films
Video Credits:
Hubble Space Telescope Animation:
ESA/Hubble - M. Kornmesser & L. L. Christensen
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