List of largest nebulae
Below is a list of the largest nebulae so far discovered, ordered by actual size (a list by angular diameter is listed separately below). This list is prone to change because of inconsistencies between studies, the great distances of nebulae from our stellar neighbourhood, and the constant refinement of technology and engineering. Nebulae have no standardized boundaries, so the measurements are subject to revision. Lastly, scientists are still defining the features and parameters of nebulae. Because of these rapid developments and adjustments, this list might be unreliable.
List
Nebula | Maximum dimension (in light-years/parsecs) |
Type | Notes |
---|---|---|---|
NGC 262 Halo Cloud | 1,300,000 ly (400,000 pc)[1] | H I region | Spiral nebula surrounding NGC 262, which is one of the largest known galaxies. |
Leo Ring | 650,000 ly (200,000 pc)[2] | HVC | |
Magellanic Stream | 600,000 ly (180,000 pc)[3] | complex of HVCs | Connects the Large and Small Magellanic clouds; extends across 180° of the sky. |
Lyman-alpha blob 1 | 300,000 ly (92,000 pc)[4] | LαB | Largest blob in the LAB Giant Concentration |
Himiko Gas Cloud | 55,000 ly (17,000 pc)[5] | Intergalactic cloud (possible LαB) |
One of the most massive lyman-alpha blobs known |
HVC 127-41-330 | 20,000 ly (6,100 pc)[6] | HVC | |
Smith's Cloud | 9,800 ly (3,000 pc)[7] | HVC | Extends about 20° of the sky |
Tarantula Nebula | 1,895 ly (581 pc)[8][lower-alpha 1] | H II region | Most active starburst region in the Local Group |
NGC 604 | 1,520 ly (470 pc)[9][10][lower-alpha 2] | H II region | Located in the Triangulum Galaxy |
N44 | 1,000 ly (310 pc)[11] | Emission nebula | |
N11 | 1,000 ly (310 pc)[12] | H II region | |
NGC 2404 | 940 ly (290 pc) | H II region | Largest H II region located in the spiral galaxy NGC 2403 |
NGC 595 | 880 ly (270 pc)[13] | H II region | |
NGC 6822 | 838 ly (257 pc) | H II region | |
Gum Nebula | 809–950 ly (248–291 pc)[14][15] | Emission nebula | |
Bubble Nebula (NGC 6822) | 758 ly (232 pc)[16][17][18] | H II region | |
NGC 6188 | 600 ly (180 pc) | Emission nebula | |
NGC 592 | 590 ly (180 pc)[19][20] | H II region | |
N119 | 570 ly (170 pc)[21] | H II region | Peculiar S-shape |
Sh2-310 | 531–681 ly (163–209 pc)[22][lower-alpha 3] | H II region | Nebula surrounding VY Canis Majoris, which is one of largest known stars. |
Carina Nebula | 460 ly (140 pc)[23] | H II region | Nearest giant H II region to Earth |
Dragonfish Nebula | 450 ly (140 pc)[24] | Emission nebula | |
RCW 49 | 350 ly (110 pc)[25] | H II region | |
Heart Nebula | 330 ly (100 pc) | H II region | |
Westerhout 5 (Soul Nebula) | 330 ly (100 pc) | H II region | |
Henize 70 (N70 or DEM L301)[26] | 300 ly (92 pc)[27] | 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 | 300 ly (92 pc)[28][29] | H II region | |
Sh2-54 | 252 ly (77 pc)[30][31] | H II region | |
Prawn Nebula | 250 ly (77 pc)[32] | H II region | |
NGC 7822 | 150 ly (46 pc)[33] | Emission nebula | |
IC 2944 | 142 ly (44 pc)[34][35] | Emission nebula | |
Eagle Nebula | 140 ly (43 pc)[36] | H II region | Part of another diffuse nebula IC 4703. |
Rosette Nebula | 130 ly (40 pc) | H II region | |
Lagoon Nebula | 110 ly (34 pc) | H II region | |
NGC 3576 | 100 ly (31 pc) | Emission nebula | |
Veil Nebula | 100-130 ly (31-40 pc) | Supernova remnant |
By angular diameter
Celestial object | Angular diameter or size | Relative size |
---|---|---|
Magellanic Stream | over 100° | |
Gum Nebula | 36° | 1,000 ly |
Milky Way | 30° (by 360°) | 105,700 ly |
Serpens-Aquila Rift | 20° by 10° | 575 ly or more |
Canis Major Overdensity | 12° by 12° | |
Smith's Cloud | 11° | |
Large Magellanic Cloud | 10.75° by 9.17° | Brightest galaxy in the night sky, 0.9 apparent magnitude (V) |
Barnard's loop | 10° | |
Zeta Ophiuchi Sh2-27 nebula | 10° | |
Sagittarius Dwarf Spheroidal Galaxy | 7.5° by 3.6° | |
Coalsack nebula | 7° by 5° | |
Rho Ophiuchi cloud complex | 4.5° by 6.5° | |
Hyades | 5°30′ | Brightest star cluster in the night sky, 0.5 apparent magnitude (V) |
Small Magellanic Cloud | 5°20′ by 3°5′ | |
Andromeda Galaxy | 3°10′ by 1° | About six times the size of the Sun or the Moon. Only the much smaller core is visible without long-exposure photography. |
Veil Nebula | 3° | |
Heart Nebula | 2.5° by 2.5° | |
Westerhout 5 | 2.3° by 1.25° | |
Sh2-54 | 2.3° | |
Carina Nebula | 2° by 2° | Brightest nebula in the night sky, 1.0 apparent magnitude (V) |
North America Nebula | 2° by 100′ | |
Orion Nebula | 1°5′ by 1° | |
Sun | 31′27″ – 32′32″ | 30–31 times the maximum value for Venus (orange bar below) / 1887–1952″ |
Moon | 29′20″ – 34′6″ | 28–32.5 times the maximum value for Venus (orange bar below) / 1760–2046″ |
Helix Nebula | About 16′ by 28′ | |
Spire in Eagle Nebula | 4′40″ | Length is 280″ |
See also
Notes
- distance × sin( diameter_angle ) = 1,895 ly
- distance × sin( diameter_angle ) = 1,520 ly
- Those measurements are based on an apparent diameter of 480 arcminutes (') plus an assumed distance of 1.5 kpc and the current distance of VY CMa which is about 1.17 kpc as the nebula is sometimes found to have the same distance as VY CMa.
References
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30 Doradus .. 49 kpc +- 3 kpc
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- NASA Astronomy Picture of the Day: Cosmic Construction Zone RCW 49 (3 June 2004)
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- SEDS: IC 2944
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Sources
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- Karachentsev, I. D.; Karachentseva, V. E.; Hutchmeier, W. K.; Makarov, D. I. (April 2004), "A Catalog of Neighboring Galaxies", Astronomical Journal, vol. 127, no. 4, pp. 2031–2068, Bibcode:2004AJ....127.2031K, doi:10.1086/382905
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