List of largest nebulae

NGC 604, one of largest nebulae (H II region) is localed in the Triangulum Galaxy
(viewed by the Hubble Space Telescope).

Below is a list of the largest nebulae so far discovered, ordered by size.

List

List of the largest nebulae
Nebula Size (ly/pc) Type Notes
NGC 604 1,520 ly (470 pc)[1] H II region Located in the Triangulum Galaxy
Gum Nebula 1,100 ly (340 pc) Emission Nebula
N44 1,000 ly (310 pc)[2] Emission Nebula
Sharpless 310 681 ly (209 pc)[3] H II region Nebula surrounding VY Canis Majoris, which is one of largest known stars.
Tarantula Nebula 600 ly (180 pc)[4] H II region Most active starburst region in the Local Group
N119 430 ly × 570 ly (130 pc × 170 pc) H II region Peculiar S-shape
Carina Nebula 460 ly (140 pc)[5] H II region Nearest giant H II region to Earth
RCW 49 350 ly (110 pc) H II region
N70 300 ly (92 pc) H II region The N 70 Nebula, in the Large Magellanic Cloud has a shell structure and is really a bubble in space. It is a "Super Bubble".
Barnard's Loop 100 or 300 ly (31 or 92 pc) H II region
Eagle Nebula 110 ly × 140 ly (34 pc × 43 pc) H II region
Rosette Nebula 130 ly (40 pc) H II region
Lagoon Nebula 40 ly × 110 ly (12 pc × 34 pc) H II region
Veil Nebula 100 ly (31 pc) Supernova remnant

List of largest lyman-alpha blobs

Polarized image of Lyman-alpha blob 1, shown as the faint, green gas cloud
List of the largest lyman-alpha blobs
Lyman-alpha blobs Size (ly/pc) Type Notes
LAB Giant Concentration
(coinciding with EQ J221734.0+001701)
200,000,000 ly (61,000,000 pc)[6] complex of LαBs Also on record as one of the largest structures in the universe.
Lyman-alpha blob 1 300,000 ly (92,000 pc)[7] LαB Largest blob in the LAB Giant Concentration
Himiko Gas Cloud 55,000 ly (17,000 pc)[8] intergalactic cloud
(possible LαB)
One of the most massive lyman-alpha blobs known

List of largest High-velocity clouds

List of the largest High-velocity clouds
High-velocity clouds Size (ly/pc) Type Notes
NGC 262 Halo Cloud 1,300,000 ly (400,000 pc) H I region Spiral nebula surrounding NGC 262, which is one of the largest known galaxies.
Leo Ring 650,000 ly (200,000 pc)[9] HVC
Magellanic Stream 600,000 ly (180,000 pc) complex of HVCs Connects the Large and Small Magellanic clouds; extends across 180° of the sky.
HVC 127-41-330 20,000 ly (6,100 pc)[10] HVC
Smith's Cloud 3,300 ly × 9,800 ly (1,000 pc × 3,000 pc)[11] HVC Extends about 20° of the sky

See also

References

  1. distance × sin( diameter_angle / 2 ) = 760 ly. radius
  2. "Roses in the Southern Sky". ESO. 3 November 2003. Retrieved 7 May 2012.
  3. Sharpless, Stewart (1959). "A Catalogue of H II Regions". The Astrophysical Journal Supplement Series. 4: 257. Bibcode:1959ApJS....4..257S. doi:10.1086/190049.
  4. Lebouteiller, V.; Bernard-Salas, J.; Brandl, B.; Whelan, D. G.; et al. (June 2008). "Chemical Composition and Mixing in Giant H II Regions: NGC 3603, 30 Doradus, and N66". The Astrophysical Journal. 680 (1): 398–419. arXiv:0710.4549. Bibcode:2008ApJ...680..398L. doi:10.1086/587503.
  5. "NGC 3372 - The Eta Carinae Nebula". Atlas of the Universe. Retrieved 2013-10-01.
  6. Ravilious, Kate. "Giant "Blob" is Largest Thing in Universe". National Geographic News. Retrieved June 23, 2011.
  7. "Giant Space Blob Glows from Within". ESO Press Release. 17 August 2011. Retrieved 18 August 2011.
  8. Hsu, Jeremy (2009-04-22). "Giant Mystery Blob Discovered Near Dawn of Time". SPACE.com. Retrieved 2009-04-24.
  9. Léo Michel-Dansa; Pierre-Alain Duc (2010). "The mysterious Leo giant gas ring explained by a billion year old collision between two galaxies". Canada France Hawaii Telescope.
  10. Josh Simon (2005). "Dark Matter in Dwarf Galaxies: Observational Tests of the Cold Dark Matter Paradigm on Small Scales" (PDF). Archived from the original (PDF) on September 13, 2006.
  11. Lockman, Felix J.; Benjamin, Robert A.; Heroux, A. J.; Langston, Glen I. (May 2008). "The Smith Cloud: A High-Velocity Cloud Colliding with the Milky Way" (PDF). The Astrophysical Journal. 679 (1): L21. arXiv:0804.4155. Bibcode:2008ApJ...679L..21L. doi:10.1086/588838. Retrieved April 3, 2012.
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