Draft:List of galaxies by surface brightness
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Comment: Most lists following the format "List of X by Y" usually get declined, see WP:NLIST - not saying it isn't useful, lists like these are just too much of a headache to maintain. monkeysmashingkeyboards (talk) 23:06, 2 December 2025 (UTC)
This is a list of galaxies sorted by surface brightness. Surface brightness is a measure of how bright an diffuse object like a galaxy or nebula appears as its surface. The brightness over the entire galaxy is called apparent magnitude.

Table
[edit]The surface brightness is calculated via . Where is surface brightness, is total magnitude, and is the total area in square arcseconds. Area is calculated using the formula for an ellipse; , where is the semi-major axis and is the semi-minor axis. Each axis is half of the dimension, because each dimension is the entire length/height but the axis is only the length/height to the centre, this combined with the symmetry of an ellipse means that half the dimension is the axis.
Combining this with the original formula we get: , which simplifies to .
| Galaxy | Image | Surface Brightness(mag/arcsecond2) | Apparent Magnitude | Dimensions | Distance(Mly) | Type | Notes | Citations |
|---|---|---|---|---|---|---|---|---|
| Messier 82 | 20.91 | 8.4 | 9x4 arcminutes(540x240 arcseconds) | 12 | Spiral | Has rapid star formation due to interactions with M81 making red streaks. | [1][2] | |
| Messier 32 | 20.93 | 8.1 | 8x6 arcminutes(480x360 arcseconds) | 2.5 | Elliptical | Satellite galaxy of the Andromeda Galaxy | [3][4] | |
| NGC 3632 | 21.17 | 10.6 | 3x2 arcminutes(180x120 arcseconds) | 70 | Spiral | [5][6] | ||
| Messier 81 | 21.33 | 6.9 | 21x10 arcminutes(1260x600 arcseconds) | 11.6 | Spiral | Faintest galaxy visible to the naked eye, despite the naked eye limiting magnitude of a star being fainter, surface brightness limits this for galaxies.[7] | [8][9] | |
| Andromeda Galaxy | 22.19 | 3.44 | 178x63 arcminutes(10680x3780 arcseconds) | 2.54 | Spiral/ring | It's core is significantly brighter than it's outer disk.[10] | [11][12][13] | |
| Messier 87 | 22.45 | 9.6 | 7 arcminutes(138544.23 square arcseconds) | 54 | Elliptical | Roughly round, so is used along with angular diameter. | [14][15] | |
| Messier 49 | 22.6 | 9.4 | 9x7.5 arcminutes(540x450 arcseconds) | 60 | Elliptical | [16][17] | ||
| Triangulum Galaxy | 23 | 5.7 | 70.8x41.7 arcminutes(4248x2502 arcseconds) | 3 | Spiral | [18][19] |
References
[edit]- ^ "Messier 82 (The Cigar Galaxy) - NASA Science". 2017-10-19. Retrieved 2025-12-03.
- ^ "Messier 82 - M82 - Cigar Galaxy". astropixels.com. Retrieved 2025-12-03.
- ^ "Messier 32 - NASA Science". 2017-10-19. Retrieved 2025-12-03.
- ^ "Messier 32 - M32". astropixels.com. Retrieved 2025-12-03.
- ^ "Caldwell 40 - NASA Science". 2020-08-19. Retrieved 2025-11-15.
- ^ "NGC 3626 (Caldwell 40)". www.skyledge.net. Retrieved 2025-11-15.
- ^ "M81 Naked EYE?????". Cloudy Nights. 2007-04-20. Retrieved 2025-11-15.
- ^ "Messier 81 - NASA Science". 2017-10-19. Retrieved 2025-11-15.
- ^ "M81 and M82 - Bode and Cigar Galaxies". astropixels.com. Retrieved 2025-11-15.
- ^ "How bright is Andromeda's center, in magnitudes per square arcminute or something similar?". Astronomy Stack Exchange. Retrieved 2025-11-15.
- ^ admin (2015-04-28). "Messier 31: Andromeda Galaxy". Messier Objects. Retrieved 2025-11-15.
- ^ "Messier 31 - M31 - Andromeda Galaxy". astropixels.com. Retrieved 2025-11-15.
- ^ "ESA Science & Technology - ISO unveils the hidden rings of Andromeda". sci.esa.int. Retrieved 2025-11-18.
- ^ "Messier 87 - NASA Science". 2017-10-19. Retrieved 2025-11-15.
- ^ "Messier 87 - M87". astropixels.com. Retrieved 2025-11-15.
- ^ "Messier 49 - NASA Science". 2022-08-26. Retrieved 2025-12-03.
- ^ "Messier 49 - M49". astropixels.com. Retrieved 2025-12-03.
- ^ "Messier 33 (The Triangulum Galaxy) - NASA Science". 2019-01-07. Retrieved 2025-11-15.
- ^ "The Triangulum Galaxy | Second Nearest Spiral Galaxy to the Milky Way". AstroBackyard. Retrieved 2025-11-15.
Category:Astronomy Category:Astronomy-related lists Category:Galaxies
