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Bubble Nebula

Emission nebula in the constellation Cassiopeia

Bubble Nebula

Emission nebula in the constellation Cassiopeia

FieldValue
nameNGC 7635
imageFile:The Bubble Nebula - NGC 7635 - Heic1608a.jpg
captionWide field image of NGC 7635 as captured by the Hubble Space Telescope
typeH II REGION
epochJ2000
ra
dec
dist_ly7100 to 11000
dist_pc3,400
appmag_v10
size_v15 × 8
radius_ly3 to 5
constellationCassiopeia
notesShell around SAO 20575
namesBubble Nebula
Sharpless 162 (Sh2-162)
Caldwell 11

Sharpless 162 (Sh2-162) Caldwell 11

The Bubble Nebula, also known as NGC 7635, Sharpless 162, or Caldwell 11, is an H II region emission nebula in the constellation Cassiopeia. It lies close to 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 November 1787 by William Herschel. The star BD+60°2522 is thought to have a mass of about .

Amateur observation

NGC 7635 and its environs imaged through an 8-inch amateur telescope

With an 8 or telescope, the nebula is visible as an extremely faint and large shell around the star. The nearby 7th magnitude star on the west hinders observation, but one can view the nebula using averted vision. Using a 16 to scope, one can see that the faint nebula is irregular, being elongated in the north south direction.

Notes

References

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References

  1. "NGC-IC Project Database".
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