Messier 81

File:300px

The HST's view of M81, with its open star clusters, globular star clusters, and regions of fluorescent gas.

Observation data (J2000 epoch)
Constellation| Ursa Major[1]
Right ascension|  09h 55m 33.1730s[2]
Declination| +69° 03′ 55.060″[2]
Redshift| 0.000130±0.00000900[2]
Helio radial velocity| −39±3 km/s
Galactocentric velocity| 73±6 km/s[2]
Distance| 11.99 ± 0.16 Mly (3.675 ± 0.049 Mpc)[2]
Apparent magnitude (V)| 6.94[3][4]
Characteristics
Type| SA(s)ab,[2] LINER[2]
Size| 29.44 kiloparsecs (96,000 light-years)
(diameter; 25.0 mag/arcsec2 B-band isophote)[2][5]
Apparent size (V)| 26.9′ × 14.1′[2]
Other designations
Bode's Galaxy, IRAS 09514+6918, NGC 3031, UGC 5318, MCG+12-10-010, PGC 28630[2][3]

Messier 81 (also known as NGC 3031 or Bode's Galaxy) is a grand design spiral galaxy about 12 million light-years away in the constellation Ursa Major. It has a D25 isophotal diameter of 29.44 kiloparsecs (96,000 light-years).[2][5]

Because of its relative proximity to the Milky Way galaxy, large size, and active galactic nucleus (which harbors a 70 million M☉[6] supermassive black hole), Messier 81 has been studied extensively by professional astronomers. The galaxy's large size and relatively high brightness also makes it a popular target for amateur astronomers.[7] In late February 2022, astronomers reported that M81 may be the source of FRB 20200120E, a repeating fast radio burst.[8][9]

## Contents

* 1 Discovery
* 2 Visibility
* 3 Interstellar dust
* 4 Globular clusters
* 5 Supernova
* 6 SMBH
* 7 Environment
* 8 Distance
* 9 See also
* 10 References
* 11 External links

## Discovery

Messier 81 was first discovered by Johann Elert Bode on 31 December 1774.[10] Thus, it is sometimes referred to as "Bode's Galaxy". In 1779, Pierre Méchain and Charles Messier reidentified Bode's object, hence listed it in the Messier Catalogue.[10]

## Visibility

The galaxy is to be found approximately 10° northwest of Alpha Ursae Majoris (Dubhe) along with several other galaxies in the Messier 81 Group.[7][11] Its apparent magnitude due to its distance means it requires a good night sky and only rises very briefly and extremely low at its southernmost limit from Earth's surface, about the 20th parallel south.

Messier 81 and Messier 82 are considered ideal for viewing using binoculars and small telescopes.[7][11] The two objects are generally not observable to the unaided eye, although highly experienced amateur astronomers may be able to see Messier 81 under exceptional observing conditions with a very dark sky.[7][12] Telescopes with apertures of 8 inches (20 cm) or larger are needed to distinguish structures in the galaxy.[11]

An infrared image of Messier 81 taken by the Spitzer Space Telescope. The blue colors represent stellar emission observed at 3.6 μm.[13] The green colors represent 8 μm emission originating primarily from polycyclic aromatic hydrocarbons in the interstellar medium.[13] The red colors represent 24 μm emission originating from heated dust in the interstellar medium.[14]

The galaxy is best observed during April.[15]

## Interstellar dust

Most of the emission at infrared wavelengths originates from interstellar dust.[14][16] This interstellar dust is found primarily within the galaxy's spiral arms, and it has been shown to be associated with star formation regions.[14][16] The general explanation is that the hot, short-lived blue stars that are found within star formation regions are very effective at heating the dust and thus enhancing the infrared dust emission from these regions.

## Globular clusters

It is estimated M81 has 210 ± 30 globular clusters.[17] In late February 2022, astronomers reported that M81 may be the source of FRB 20200120E, a repeating fast radio burst.[8][9]

## Supernova

M81 (left) and M82 (right). M82 is one of two galaxies strongly influenced gravitationally by M81. The other, NGC 3077, is located off the top edge of this image. M81 with satellite galaxy Holmberg IX in the top center-right corner

Only one supernova has been detected in Messier 81.[18] The supernova, named SN 1993J, was discovered on 28 March 1993 by F. García in Spain.[19] At the time, it was the second brightest Type II supernova observed in the 20th century,[20] peaking at an apparent magnitude of 10.7. The spectral characteristics of the supernova changed over time. Initially, it looked more like a Type II supernova (a supernova formed by the explosion of a supergiant star) with strong hydrogen spectral line emission, but later the hydrogen lines faded and strong helium spectral lines appeared, making the supernova look more like a Type Ib.[20][21]

Moreover, the variations in SN 1993J's luminosity over time were not like the variations observed in other Type II supernovae,[22][23] but did resemble the variations observed in Type Ib supernovae.[24] Hence, the supernova has been classified as a Type IIb, a transitory class between Type II and Type Ib.[21] The scientific results from this supernova suggested that Type Ib and Ic supernovae were formed through the explosions of giant stars through processes similar to those taking place in Type II supernovae.[21][25] Despite the uncertainties in modeling the unusual supernova, it was also used to estimate a very approximate distance of 8.5 ± 1.3 Mly (2.6 ± 0.4 Mpc) to Messier 81.[20] As a local galaxy, the Central Bureau for Astronomical Telegrams (CBAT) tracks novae in M81 along with M31 and M33.[26]

## SMBH

In the center of M81 there exists a supermassive black hole (SMBH) with a mass of about 7×107 M☉. The SMBH is active, having an accretion disk and one-sided relativistic jet. The observation also demonstrate that there may exist a second SMBH that orbits the primary SMBH with a period of around 30 years. The mass of the secondary SMBH is estimated at 0.1 of the primary.[27]

## Environment

Messier 81 is the largest galaxy in the M81 Group, a group of 34 in the constellation Ursa Major.[28] At approximately 11.7 Mly (3.6 Mpc) from the Earth, it makes this group and the Local Group, containing the Milky Way,[28] relative neighbors in the Virgo Supercluster.

Gravitational interactions of M81 with M82 and NGC 3077[29] have stripped hydrogen gas away from all three galaxies, forming gaseous filamentary structures in the group.[29] Moreover, these interactions have allowed interstellar gas to fall into the centers of M82 and NGC 3077, leading to vigorous star formation or starburst activity there.[29]

## Distance

The distance to Messier 81 has been measured by Freedman et al[30] to be 3.63 ± 0.34 Megaparsecs (11.8 ± 1.1 million light years) by using the Hubble Space Telescope to identify classical Cepheid variables and measure their periods using the period-luminosity relation discovered by Henrietta Swan Leavitt.

## See also

* List of galaxies
* List of Messier objects
* Messier object
* New General Catalogue

## References

1. ↑ Dreyer, J. L. E. (1988). Sinnott, R. W.. ed. The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters. Sky Publishing Corporation / Cambridge University Press. ISBN 978-0-933346-51-2.
2. ↑ 2.00 2.01 2.02 2.03 2.04 2.05 2.06 2.07 2.08 2.09 2.10 "Results for Messier 081". NASA and Caltech. https://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=Messier+081&extend=no&hconst=67.74&omegam=0.3089&omegav=0.6911&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES.
3. ↑ 3.0 3.1 "M 81". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=M+81.
4. ↑ Armando, Gil de Paz; Boissier, Samuel; Madore, Barry F.; Seibert, Mark; Joe, Young H.; Boselli, Alessandro; Wyder, Ted K.; Thilker, David et al. (2007). "The GALEX Ultraviolet Atlas of Nearby Galaxies". Astrophysical Journal 173 (2): 185–255. doi:10.1086/516636. Bibcode: 2007ApJS..173..185G.
5. ↑ 5.0 5.1 De Vaucouleurs, Gerard; De Vaucouleurs, Antoinette; Corwin, Herold G.; Buta, Ronald J.; Paturel, Georges; Fouque, Pascal (1991). Third Reference Catalogue of Bright Galaxies. Bibcode: 1991rc3..book.....D.
6. ↑ Devereux, N.; Ford, H.; Tsvetanov, Z.; Jocoby, J. (2003). "STIS Spectroscopy of the Central 10 Parsecs of M81: Evidence for a Massive Black Hole". Astronomical Journal 125 (3): 1226–1235. doi:10.1086/367595. Bibcode: 2003AJ....125.1226D.
7. ↑ 7.0 7.1 7.2 7.3 O'Meara, S. J. (1998). The Messier Objects. Cambridge University Press. ISBN 978-0-521-55332-2. https://archive.org/details/messierobjectsfi00omea.
8. ↑ 8.0 8.1 Starr, Michelle (23 February 2022). "Mysterious Repeating Fast Radio Burst Traced to Very Unexpected Location". ScienceAlert. https://www.sciencealert.com/mysterious-repeating-fast-radio-burst-traced-to-very-unexpected-location. Retrieved 24 February 2022.
9. ↑ 9.0 9.1 Kirsten, F (23 February 2022). "A repeating fast radio burst source in a globular cluster". Nature 602 (7898): 585–589. doi:10.1038/s41586-021-04354-w. PMID 35197615. Bibcode: 2022Natur.602..585K. https://www.nature.com/articles/s41586-021-04354-w. Retrieved 24 February 2022.
10. ↑ 10.0 10.1 Jones, K. G. (1991). Messier's Nebulae and Star Clusters (2nd ed.). Cambridge University Press. ISBN 978-0-521-37079-0.
11. ↑ 11.0 11.1 11.2 Eicher, D. J. (1988). The Universe from Your Backyard. Cambridge University Press. ISBN 978-0-521-36299-3. https://archive.org/details/universefromyour0000eich.
12. ↑ Stephen Uitti. "Farthest Naked Eye Object". http://www.uitti.net/stephen/astro/essays/farthest_naked_eye_object.shtml.
13. ↑ 13.0 13.1 "Infrared Array Camera (IRAC) Observations of M81". Astrophysical Journal Supplement Series 154 (1): 222–228. 2004. doi:10.1086/422913. Bibcode: 2004ApJS..154..222W.
14. ↑ 14.0 14.1 14.2 "Spatially Resolved Ultraviolet, Hα, Infrared, and Radio Star Formation in M81". Astrophysical Journal Supplement Series 154 (1): 215–221. 2004. doi:10.1086/422714. Bibcode: 2004ApJS..154..215G.
15. ↑ "Messier 81 - NASA Science". https://science.nasa.gov/mission/hubble/science/explore-the-night-sky/hubble-messier-catalog/messier-81/.
16. ↑ 16.0 16.1 Pérez-González, P. G.; Kennicutt Jr., R. C.; Gordon, K. D.; Misselt, K. A.; Gil De Paz, A.; Engelbracht, C. W.; Rieke, G. H.; Bendo, G. J. et al. (2006). "Ultraviolet through Far-Infrared Spatially Resolved Analysis of the Recent Star Formation in M81 (NGC 3031)". Astrophysical Journal 648 (2): 987–1006. doi:10.1086/506196. Bibcode: 2006ApJ...648..987P.
17. ↑ Chandar, Rupali; Whitmore, Bradley; Lee, Myung Gyoon (2004-08-10). "The Globular Cluster Systems of Five Nearby Spiral Galaxies: New Insights from Hubble Space TelescopeImaging" (in en). The Astrophysical Journal 611 (1): 220–244. doi:10.1086/421934. ISSN 0004-637X. Bibcode: 2004ApJ...611..220C.
18. ↑ "NASA/IPAC Extragalactic Database". Results for extended name search on NGC 3031. http://nedwww.ipac.caltech.edu/.
19. ↑ Ripero, J.; Garcia, F.; Rodriguez, D.; Pujol, P.; Filippenko, A. V.; Treffers, R. R.; Paik, Y.; Davis, M. et al. (1993). "Supernova 1993J in NGC 3031". IAU Circular 5731: 1. Bibcode: 1993IAUC.5731....1R.
20. ↑ 20.0 20.1 20.2 Schmidt, B.P.; Kirshner, R.P.; Eastman, R.G.; Grashuis, R.; Dell'Antonio, I.; Caldwell, N.; Foltz, C.; Huchra, John P. et al. (1993). "The unusual supernova SN1993J in the galaxy M81". Nature 364 (6438): 600–602. doi:10.1038/364600a0. Bibcode: 1993Natur.364..600S.
21. ↑ 21.0 21.1 21.2 Filippenko, A. V.; Matheson, T.; Ho, L. C. (1993). "The "Type IIb" Supernova 1993J in M81: A Close Relative of Type Ib Supernovae". Astrophysical Journal Letters 415: L103–L106. doi:10.1086/187043. Bibcode: 1993ApJ...415L.103F.
22. ↑ Benson, P. J.; Herbst, W.; Salzer, J. J.; Vinton, G.; Hanson, G. J.; Ratcliff, S. J.; Winkler, P. F.; Elmegreen, D. M. et al. (1994). "Light curves of SN 1993J from the Keck Northeast Astronomy Consortium". Astronomical Journal 107: 1453–1460. doi:10.1086/116958. Bibcode: 1994AJ....107.1453B.
23. ↑ Wheeler, J. C.; Barker, E.; Benjamin, R.; Boisseau, J.; Clocchiatti, A.; De Vaucouleurs, G.; Gaffney, N.; Harkness, R. P. et al. (1993). "Early Observations of SN 1993J in M81 at McDonald Observatory". Astrophysical Journal 417: L71–L74. doi:10.1086/187097. Bibcode: 1993ApJ...417L..71W.
24. ↑ Richmond, M. W.; Treffers, R. R.; Filippenko, A. V.; Palik, Y.; Leibundgut, B.; Schulman, E.; Cox, C. V. (1994). "UBVRI photometry of SN 1993J in M81: The first 120 days". Astronomical Journal 107: 1022–1040. doi:10.1086/116915. Bibcode: 1994AJ....107.1022R.
25. ↑ Filippenko, A. V.; Matheson, T.; Barth, A. J. (1994). "The peculiar type II supernova 1993J in M81: Transition to the nebular phase". Astronomical Journal 108: 2220–2225. doi:10.1086/117234. Bibcode: 1994AJ....108.2220F.
26. ↑ Bishop, David. "Extragalactic Novae". Rochester Astronomy. https://www.rochesterastronomy.org/novae.html.
27. ↑ Jiang, Wu; Shen, Zhiqiang; Martí-Vidal, Ivan; Yan, Zhen; Huang, Lei; Gold, Roman; Li, Ya-Ping; Xie, Fuguo et al. (1 December 2023). "Observational Evidence of a Centi-parsec Supermassive Black Hole Binary Existing in the Nearby Galaxy M81". The Astrophysical Journal 959 (1): 11. doi:10.3847/1538-4357/ad063d.
28. ↑ 28.0 28.1 Karachentsev, I. D. (2005). "The Local Group and Other Neighboring Galaxy Groups". Astronomical Journal 129 (1): 178–188. doi:10.1086/426368. Bibcode: 2005AJ....129..178K.
29. ↑ 29.0 29.1 29.2 Yun, M. S.; Ho, P. T. P.; Lo, K. Y. (1994). "A high-resolution image of atomic hydrogen in the M81 group of galaxies". Nature 372 (6506): 530–532. doi:10.1038/372530a0. PMID 7990925. Bibcode: 1994Natur.372..530Y.
30. ↑ Freedman, Wendy (1994). "The Hubble Space Telescope Extragalactic Distance Scale Project. I. The Discovery of Cepheids and a New Distance to M81". The Astrophysical Journal 427 (June): 628–655. doi:10.1086/174172. Bibcode: 1994ApJ...427..628F. https://articles.adsabs.harvard.edu/pdf/1994ApJ...427..628F.

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## External links

| Wikimedia Commons has media related to Messier 81.

|

* StarDate: M81 Fact Sheet
* M81, SEDS Messier pages
* SST: Messier 81
* NASA Astronomy Picture of the Day: Bright Galaxy M81 (20 June 2002)
* NightSkyInfo.com – M81, Bode's Galaxy
* Messier 81 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
* ESA/Hubble images of M81
* Galaxy Messier 81 (Bode's Galaxy)
* Spitzer Image Gallery
* Helkit Observatory
* Deep image of the M81 Area
* Bode's Galaxy at Constellation Guide

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Messier objects

List|

* M1
* M2
* M3
* M4
* M5
* M6
* M7
* M8
* M9
* M10
* M11
* M12
* M13
* M14
* M15
* M16
* M17
* M18
* M19
* M20
* M21
* M22
* M23
* M24
* M25
* M26
* M27
* M28
* M29
* M30
* M31
* M32
* M33
* M34
* M35
* M36
* M37
* M38
* M39
* M40
* M41
* M42
* M43
* M44
* M45
* M46
* M47
* M48
* M49
* M50
* M51
* M52
* M53
* M54
* M55
* M56
* M57
* M58
* M59
* M60
* M61
* M62
* M63
* M64
* M65
* M66
* M67
* M68
* M69
* M70
* M71
* M72
* M73
* M74
* M75
* M76
* M77
* M78
* M79
* M80
* M81
* M82
* M83
* M84
* M85
* M86
* M87
* M88
* M89
* M90
* M91
* M92
* M93
* M94
* M95
* M96
* M97
* M98
* M99
* M100
* M101
* M102
* M103
* Added
* M104
* M105
* M106
* M107
* M108
* M109
* M110

See also|

* Caldwell catalogue
* Catalogue of Nebulae and Clusters of Stars
* Herschel 400 Catalogue
* Index Catalogue
* New General Catalogue
* Revised New General Catalogue

* Book
* Category
* Commons
* Portal

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List of notable Seyfert galaxies

Seyfert 1|

* Arakelian 120
* Arakelian 564
* Arp 102B
* 3C 59
* ESO 141-055
* ESO 198-G24
* ESO 323-G077
* ESO 362-18
* Fairall 9
* Fairall 51
* H0557-385
* 1H 0419-577
* 1H 1707-495
* IC 3599
* IC 4329A
* IRAS 07598+6508
* IRAS 13224-3809
* IRAS 13349+1428
* Markarian 6
* Markarian 50
* Markarian 79
* Markarian 110
* Markarian 279
* Markarian 315
* Markarian 334
* Markarian 335
* Markarian 359
* Markarian 376
* Markarian 423
* Markarian 478
* Markarian 507
* Markarian 509
* Markarian 609
* Markarian 618
* Markarian 704
* Markarian 705
* Markarian 817
* Markarian 841
* Markarian 896
* Markarian 993
* Markarian 1018
* Markarian 1044
* Markarian 1239
* MCG -2-58-22
* MCG-6-30-15
* MGC +8-11-11
* Messier 81
* PG 1211+143
* PG 1244+026
* PG 1402+261
* PG 1404+226
* PKS 0558-504
* PMN J0948+0022
* RE J0134+396
* SBS 0846+513
* Ton S180
* I Zw 1
* III Zw 2
* III Zw 77

Seyfert 2|

* Circinus Galaxy
* ESO 103-G35
* ESO 428-G14
* IC 2560
* IC 3639
* IRAS 05189-2524
* IRAS 13197-1627
* IRAS 18325-5926
* IRAS 19014+4109
* IRAS F01475-0740
* Markarian 3
* Markarian 34
* Markarian 78
* Markarian 176
* Markarian 266 SW
* Markarian 273
* Markarian 463
* Markarian 477
* Markarian 573
* Markarian 1066
* Markarian 1210
* MCG-5-23-16
* Messier 77
* Messier 88
* Messier 106
* NGC 454E
* NGC 2788A
* NGC 4676B
* NGC 4922N
* Whirlpool Galaxy

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Stars of Ursa Major

Bayer|

* α (Dubhe)
* β (Merak)
* γ (Phecda)
* δ (Megrez)
* ε (Alioth)
* ζ (Mizar)
* η (Alkaid)
* θ
* ι (Talitha)
* κ (Alkaphrah)
* λ (Tania Borealis)
* μ (Tania Australis)
* ν (Alula Borealis)
* ξ (Alula Australis)
* ο (Muscida)
* π1
* π2
* ρ
* σ1
* σ2
* τ
* υ
* φ
* χ (Taiyangshou)
* ψ
* ω

Flamsteed|

* 2 (A)
* 5 (b)
* 6
* 15 (f)
* 16 (c)
* 17
* 18 (e)
* 19
* 20
* 21
* 22
* 23 (h)
* 24 (d)
* 26
* 27
* 28
* 31
* 32
* 35
* 36
* 37
* 38
* 39
* 40
* 41
* 42
* 43
* 44
* 46
* 47 (Chalawan)
* 49
* 51
* 55
* 56
* 57
* 58
* 59
* 60
* 61
* 62
* 65
* 66
* 67
* 68
* 70
* 71
* 72
* 73
* 74
* 75
* 76
* 78
* 80 (Alcor)
* 81
* 82
* 83
* 84
* 86
* 55 Cam
* 56 Cam
* 57 Cam
* 1 CVn
* 14 LMi
* 15 LMi
* 25 LMi
* 47 LMi
* 37 Lyn
* 39 Lyn
* 41 Lyn (Intercrus)
* 44 Lyn

Variable|

* R
* T
* U
* W
* Z
* RV
* ST
* SU
* SW
* SX
* TU
* TX
* TY
* UX
* UY
* VV
* VX
* VY
* XY
* ZZ
* AA
* AB
* AE
* AN
* AR
* AW
* BC
* BE
* BM
* BZ
* CG
* CH
* CO
* CQ
* CY
* DH
* DI
* DM
* DN
* DV
* DW
* EE
* EG
* EI
* EK
* EN
* EP
* ER
* ET
* EU
* EV
* EZ
* IY
* KS
* NQ
* NY

HR|

* 3236
* 3263
* 3303
* 3332
* 3400
* 3401
* 3405
* 3408
* 3436
* 3470
* 3506
* 3592
* 3603
* 3608
* 3645
* 3676
* 3725
* 3747
* 3824
* 3838
* 3854
* 3855
* 3859
* 3885
* 3911
* 3918
* 3922
* 3929
* 3939
* 3954
* 3958
* 4044
* 4046
* 4051
* 4052
* 4067
* 4096
* 4098
* 4103
* 4108
* 4132
* 4165
* 4176
* 4181
* 4191
* 4215
* 4242
* 4243
* 4264
* 4275
* 4278
* 4280
* 4283
* 4285
* 4286
* 4336
* 4340
* 4345
* 4351
* 4367
* 4383
* 4388
* 4391
* 4407
* 4412
* 4421
* 4424
* 4435
* 4439
* 4452
* 4457
* 4474
* 4481
* 4482
* 4486
* 4493
* 4500
* 4521
* 4536
* 4545
* 4562
* 4569
* 4574
* 4581
* 4584
* 4593
* 4610
* 4672
* 4767
* 4840
* 4859
* 4867
* 4917
* 4936
* 4953
* 5070
* 5076
* 5085
* 5126
* 5148
* 5169
* 5077
* 5213
* 5216
* 5256
* 5280
* 5302

HD|

* 68988
* 74389
* 80461
* 80606
* 80607
* 82408
* 82969
* 83564
* 88609
* 89221
* 93551
* 95572
* 96127
* 98618
* 99706
* 100018
* 102956
* 115043
* 118203
* 118970
* 233604

Gliese|

* GJ 3512
* Gliese 338
* Gliese 412
* Gliese 424
* Gliese 450

Other|

* ADS 7251
* Feige 34
* Feige 48
* Feige 55
* G 119-62
* G 195-19
* G 196-3
* Groombridge 1618
* Groombridge 1830
* HAT-P-3
* HAT-P-13
* HAT-P-21
* HAT-P-22
* HIP 57050
* HIP 57274
* Holmberg IX X-1
* Lalande 21185
* M82 X-1
* M82 X-2
* PG 1219+534
* PG 1351+489
* PSR B1112+50
* PSR J1012+5307
* Sidus Ludoviciana
* Winnecke 4
* WISE 1405+5534
* XTE J1118+480

List

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New General Catalogue 3000 to 3499

* 3000
* 3001
* 3002
* 3003
* 3004
* 3005
* 3006
* 3007
* 3008
* 3009
* 3010
* 3011
* 3012
* 3013
* 3014
* 3015
* 3016
* 3017
* 3018
* 3019
* 3020
* 3021
* 3022
* 3023
* 3024
* 3025
* 3026
* 3027
* 3028
* 3029
* 3030
* 3031
* 3032
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* 3034
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* 3036
* 3037
* 3038
* 3039
* 3040
* 3041
* 3042
* 3043
* 3044
* 3045
* 3046
* 3047
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* 3051
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* 3053
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* 3071
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* 3074
* 3075
* 3076
* 3077
* 3078
* 3079
* 3080
* 3081
* 3082
* 3083
* 3084
* 3085
* 3086
* 3087
* 3088
* 3089
* 3090
* 3091
* 3092
* 3093
* 3094
* 3095
* 3096
* 3097
* 3098
* 3099
* 3100
* 3101
* 3102
* 3103
* 3104
* 3105
* 3106
* 3107
* 3108
* 3109
* 3110
* 3111
* 3112
* 3113
* 3114
* 3115
* 3116
* 3117
* 3118
* 3119
* 3120
* 3121
* 3122
* 3123
* 3124
* 3125
* 3126
* 3127
* 3128
* 3129
* 3130
* 3131
* 3132
* 3133
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* 3135
* 3136
* 3137
* 3138
* 3139
* 3140
* 3141
* 3142
* 3143
* 3144
* 3145
* 3146
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* 3148
* 3149
* 3150
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* 3160
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* 3197
* 3198
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* 3200
* 3201
* 3202
* 3203
* 3204
* 3205
* 3206
* 3207
* 3208
* 3209
* 3210
* 3211
* 3212
* 3213
* 3214
* 3215
* 3216
* 3217
* 3218
* 3219
* 3220
* 3221
* 3222
* 3223
* 3224
* 3225
* 3226
* 3227
* 3228
* 3229
* 3230
* 3231
* 3232
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* 3260
* 3261
* 3262
* 3263
* 3264
* 3265
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* 3268
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* 3277
* 3278
* 3279
* 3280
* 3281
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* 3297
* 3298
* 3299
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* 3310
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* 3321
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* 3325
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* 3328
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* 3330
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* 3340
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* 3350
* 3351
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* 3353
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* 3357
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* 3359
* 3360
* 3361
* 3362
* 3363
* 3364
* 3365
* 3366
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* 3370
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* 3377
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* 3380
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* 3398
* 3399
* 3400
* 3401
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* 3403
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* 3408
* 3409
* 3410
* 3411
* 3412
* 3413
* 3414
* 3415
* 3416
* 3417
* 3418
* 3419
* 3420
* 3421
* 3422
* 3423
* 3424
* 3425
* 3426
* 3427
* 3428
* 3429
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* 3433
* 3434
* 3435
* 3436
* 3437
* 3438
* 3439
* 3440
* 3441
* 3442
* 3443
* 3444
* 3445
* 3446
* 3447
* 3448
* 3449
* 3450
* 3451
* 3452
* 3453
* 3454
* 3455
* 3456
* 3457
* 3458
* 3459
* 3460
* 3461
* 3462
* 3463
* 3464
* 3465
* 3466
* 3467
* 3468
* 3469
* 3470
* 3471
* 3472
* 3473
* 3474
* 3475
* 3476
* 3477
* 3478
* 3479
* 3480
* 3481
* 3482
* 3483
* 3484
* 3485
* 3486
* 3487
* 3488
* 3489
* 3490
* 3491
* 3492
* 3493
* 3494
* 3495
* 3496
* 3497
* 3498
* 3499

* Astronomical catalog
* List of NGC objects

Coordinates:  09h 55m 33.1730s, +69° 03′ 55.060″

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Original source: https://en.wikipedia.org/wiki/Messier 81. Read more

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