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NGC 685

Coordinates:Sky map01h 47m 42.8593s, −52° 45′ 42.446″
From Wikipedia, the free encyclopedia
Galaxy in the constellation Eridanus
NGC 685
NGC 685 imaged by theHubble Space Telescope
Observation data (J2000epoch)
ConstellationEridanus
Right ascension01h 47m 42.8593s[1]
Declination−52° 45′ 42.446″[1]
Redshift0.004546 ± 0.000010[1]
Heliocentric radial velocity1,363 ± 3 km/s[1]
Distance50–58Mly (15.2-17.8Mpc)[1]
Apparent magnitude (V)11.2[2]
Characteristics
TypeSB(rs)d[1]
Size~74,300 ly (22.77 kpc) (estimated)[1]
Apparent size (V)3.7′ × 3.3′[1]
Other designations
ESO 152- G 024, AM 0145-530A,IRAS 01458-5300,PGC 6581[1]

NGC 685 is abarred spiral galaxy in the constellationEridanus. The galaxy lies about 55 millionlight years away from Earth, which means, given its apparent dimensions, that NGC 685 is approximately 74,000 light years across.[1] It was discovered byJohn Herschel on October 3, 1834.[3]

This galaxy is seen nearly face-on, at an inclination of 23°.[4] It is a barred spiral galaxy with its bright center bar and patchy, curvingarms. The arms have low surface brightness and emerge from the bar and complete three quarters of a revolution before fading.[5] The patches of bright blue along the galaxy’s arms arestar clusters, groups of stars held together by their mutual gravitational attraction. Wisps of dark red near the central bar depict interstellar gas and dust, the matter from which stars form.[6] The southeast edge of the galaxy features three brightHII regions, whichHalton Arp argued they are a companion galaxy.H-alpha emission is stronger at the southeastern half of the galaxy.[7] The totalstar formation rate of the galaxy is estimated to be 0.42M per year.[4]

The whole galaxy is about 74,000 light-years across – a little more than half the size of ourMilky Way.[6]In the centre of the galaxy is predicted to lie asupermassive black hole whose mass is estimated to be between 7.6 and 40 millionsolar masses, based on the spiral arm pitch angle.[8]

See also

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References

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  1. ^abcdefghij"Results for object NGC 0685".NASA/IPAC Extragalactic Database.NASA andCaltech. Retrieved1 February 2025.
  2. ^"Revised NGC Data for NGC 685".spider.seds.org. Retrieved30 March 2024.
  3. ^Seligman, Courtney."NGC 685 (= PGC 5619)".Celestial Atlas. Retrieved19 November 2018.
  4. ^abLee, Janice C.; et al. (1 January 2022)."The PHANGS-HST Survey: Physics at High Angular Resolution in Nearby Galaxies with the Hubble Space Telescope".The Astrophysical Journal Supplement Series.258 (1): 10.arXiv:2101.02855.doi:10.3847/1538-4365/ac1fe5.
  5. ^Eskridge, Paul B.; Frogel, Jay A.; Pogge, Richard W.; Quillen, Alice C.; Berlind, Andreas A.; Davies, Roger L.; DePoy, D. L.; Gilbert, Karoline M.; Houdashelt, Mark L.; Kuchinski, Leslie E.; Ramirez, Solange V.; Sellgren, K.; Stutz, Amelia; Terndrup, Donald M.; Tiede, Glenn P. (November 2002). "Near-Infrared and Optical Morphology of Spiral Galaxies".The Astrophysical Journal Supplement Series.143 (1):73–111.arXiv:astro-ph/0206320.doi:10.1086/342340.
  6. ^abPublic Domain This article incorporates text from this source, which is in thepublic domain."Hubble Examines Entrancing Galaxy in Eridanus - NASA Science".NASA. 7 October 2023. Retrieved1 February 2025.
  7. ^Arp, H. (May 1982). "Characteristics of companion galaxies".The Astrophysical Journal.256: 54.doi:10.1086/159883.
  8. ^Davis, Benjamin L.; Berrier, Joel C.; Johns, Lucas; Shields, Douglas W.; Hartley, Matthew T.; Kennefick, Daniel; Kennefick, Julia; Seigar, Marc S.; Lacy, Claud H. S. (20 June 2014). "The Black Hole Mass Function Derived from Local Spiral Galaxies".The Astrophysical Journal.789 (2): 124.arXiv:1405.5876.doi:10.1088/0004-637X/789/2/124.

External links

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