Malin 1

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Malin 1
Malin1-HLA (cropped).jpg
Malin 1 by the Hubble Space Telescope
Observation data (J2000.0[1] epoch)
ConstellationComa Berenices[2]
Right ascension 12h 36m 59.34697s[1]
Declination+14° 19′ 49.1585″ [1]
Redshift0.082557±0.000033[3]
Helio radial velocity24750±10 km/s[3]
Galactocentric velocity24707±10 km/s[3]
Distance1.19 Gly (366 Mpc) h−1
0.73
[3]
Apparent magnitude (V)15.809±0.009[3]
Absolute magnitude (V)−22.01±0.50[3]
Characteristics
TypeSB0a [1]
Mass~1012[4] M
Size650 kly (200 kpc) [5][6][7]
Apparent size (V)0.219 × 0.204′ [2]
Other designations
PGC 42102, LEDA 42102, VPC 1091, 2MASX J12365934+1419494, Gaia DR2 3932516418935413504[1]
See also: Galaxy, List of galaxies

Malin 1 is a giant low surface brightness (LSB) spiral galaxy.[1][8] It is located 1.19 billion light-years (366 Mpc) away in the constellation Coma Berenices, near the North Galactic Pole. As of February 2015, it is arguably the largest known spiral galaxy, with an approximate diameter of 650,000 light-years (200,000 pc),[5][6][7] thus over three times the diameter of our Milky Way. It was discovered by astronomer David Malin in 1986 and is the first LSB galaxy verified to exist.[8][7][5] Its high surface brightness central spiral is 30,000 light-years (9,200 pc) across, with a bulge of 10,000 light-years (3,100 pc).[5] The central spiral is a SB0a type barred-spiral.[5]

Malin 1 is peculiar in several ways: its diameter alone would make it the largest barred spiral galaxy ever to have been observed.[4]

Malin 1 was found later to be interacting with two other galaxies, Malin 1B and SDSS J123708.91+142253.2. Malin 1B is located 46,000 light-years (14,000 pc) away from the high surface brightness central spiral of Malin 1, which may be responsible for the formation of the galaxy's central bar. Meanwhile, SDSS J123708.91+142253.2 is located within the huge, faint halo of Malin 1 and might have caused the formation of the extended low surface brightness disc through tidal stripping.

Observations by Galaz et al. in April 2014 revealed a detailed view of the spiral structure of Malin 1 in optical bands. The galaxy exhibits giant and very faint spiral arms, with a thickness of up to one-third the diameter of the Milky Way. Other details, such as possible stellar streams and formation regions, are revealed as well.[9]

Gallery[edit]

Processed image of Malin 1 by Giuseppe Donatiello showing its weak spiral arms

See also[edit]

References[edit]

  1. ^ a b c d e f "2MASX J12365934+1419494". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 27 October 2010.
  2. ^ a b "PGC 42102". WikiSky. Retrieved 27 October 2010.
  3. ^ a b c d e f "Detailed Information for Object Malin 1". NASA/IPAC Extragalactic Database. Retrieved April 18, 2012.
  4. ^ a b Barth, Aaron J. (March 2007). "A Normal Stellar Disk in the Galaxy Malin 1". The Astronomical Journal. 133 (3): 1085–1091. arXiv:astro-ph/0701018. Bibcode:2007AJ....133.1085B. doi:10.1086/511180.
  5. ^ a b c d e Crosswell, Ken (22 January 2007). "Malin 1: A Bizarre Galaxy Gets Slightly Less So". KenCroswell.com.
  6. ^ a b Dorminey, Bruce (22 December 2013). "Astronomers Still Puzzle Over 'Low Surface Brightness' Galaxies". Forbes. Retrieved 30 December 2014.
  7. ^ a b c Glenday, Craig, ed. (2011). Guinness World Records 2011. New York: Random House. p. 3. ISBN 978-0-440-42310-2.
  8. ^ a b Bothun, Gregory D. (February 1997). "The Ghostliest Galaxies". Scientific American. 276 (2): 56–61. Bibcode:1997SciAm.276b..40B. doi:10.1038/scientificamerican0297-56. JSTOR 24993608.
  9. ^ Galaz, Gaspar; et al. (December 2015). "Deep Optical Images of Malin 1 Reveal New Features". The Astrophysical Journal Letters. 815 (2). L29. arXiv:1512.01095. Bibcode:2015ApJ...815L..29G. doi:10.1088/2041-8205/815/2/L29.

External links[edit]

Media related to Malin 1 at Wikimedia Commons