Astronomy:Messier 100

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Messier 100
Galaxy Messier 100 imaged by ESO, revealing complex spiral arm structure
Observation data (J2000 epoch)
ConstellationComa Berenices[1]
Right ascension 12h 22m 54.8616s[2]
Declination+15° 49′ 17.886″[2]
Redshift0.005240[2]
Helio radial velocity1,571±1 km/s[2]
Distance55 Mly[3]
Group or clusterVirgo Cluster
Apparent magnitude (V)9.3[4]
Characteristics
TypeSAB(s)bc[2]
Size~166,100 ly (50.93 kpc) (estimated)[2]
Apparent size (V)7.4′ × 6.3′[2]
Other designations
HOLM 387A, IRAS 12204+1605, NGC 4321, UGC 7450, MCG+03-32-015, PGC 40153

Messier 100 (also known as NGC 4321 or the Mirror Galaxy) is a grand design intermediate spiral galaxy in the southern part of the mildly northern Coma Berenices.[5] It is one of the brightest and largest galaxies in the Virgo Cluster and is approximately 55 million light-years[3] from our galaxy, about 166,000 light-years in diameter. It was discovered by Pierre Méchain in 1781[lower-alpha 1] and 29 days later seen again and entered by Charles Messier in his catalogue "of nebulae and star clusters".[6][7] It was one of the first spiral galaxies to be discovered,[7] and was listed as one of fourteen spiral nebulae by Lord William Parsons of Rosse in 1850. NGC 4323 and NGC 4328 are satellite galaxies of M100; the former is connected with it by a bridge of luminous matter.[8][9]

Early observations

This is a widefield view of the galaxy, M100, directly left of the center of the picture - captured with an amateur telescope in 2025.

After the discovery of M100 by Méchain, Charles Messier made observations of the galaxy depicting it as a nebula without a star. He pointed out that it was difficult[7] to recognize the nebula because of its faintness. William Herschel was able to identify a bright cluster of stars[7] within the "nebula" during his observations. His son John expanded the findings in 1833. With the advent of better telescopes, John Herschel was able to see a round, brighter galaxy; however, he also mentioned that it was barely visible through clouds. William Henry Smyth[7] extended the studies of M100, detailing it as a pearly white nebula and pointing out diffuse spots.

Star formation

Messier 100 is considered a starburst galaxy[10] with the strongest star formation activity concentrated in its center, within a ring – actually two tightly wound spiral arms attached to a small nuclear bar of radius: one thousand parsecs[11] – where star formation has been taking place for at least 500 million years in separate bursts.[12]

As usual on spiral galaxies of the Virgo Cluster, in the rest of the disk both star formation[13] and neutral hydrogen, of which M100 is deficient compared to isolated spiral galaxies of similar Hubble type,[14] are truncated within the galaxy's disk, which is caused by interactions with the intracluster medium of Virgo.

Supernovae

Supernova SN 2019ehk in M100 (Hubble)

Seven supernovae have been identified in M100:[5]

  • On 17 March 1901 Heber Curtis discovered SN 1901B (Type I, mag. 15.6),[15][5][16] at 110"W and 4"N from the galaxy's nucleus.[17]
  • Heber Curtis discovered SN 1914A (type unknown, mag. 15.7)[5][18] on 2 March 1914, at 24"E and 111"S from the galaxy's nucleus.[15][17]
  • Milton Humason, with observations from early to mid 1960,[lower-alpha 2] discovered SN 1959E (Type I, mag. 17.5),[5][19] located 58"E and 21"S from the galaxy's nucleus.[20]
  • On 15 April 1979, amateur astronomer Gus Johnson discovered SN 1979C, the first Type II supernova found in the M100 galaxy. However, the star faded quickly, and later observations from x-ray to radio wavelengths revealed its remnant.[5][21][22]
  • SN 2006X (Type Ia, mag. 15.3) was discovered by Shoji Suzuki and Marco Migliardi on 7 February 2006, two weeks before fading to magnitude 17.[5][23][24][25]
  • Jaroslaw Grzegorzek discovered SN 2019ehk (Type Ib, mag. 16.5) on 29 April 2019. The supernova reached a peak magnitude of approximately 15.8.[26]
  • SN 2020oi (Type Ic, mag. 17.28) was discovered by Automatic Learning for the Rapid Classification of Events (ALeRCE) on 7 January 2020.[5][27][28]

See also

References and footnotes

  1. ↑ R. W. Sinnott, ed (1988). The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer. Sky Publishing Corporation/Cambridge University Press. ISBN 978-0-933346-51-2. 
  2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 "Results for object MESSIER 100". NASA and Caltech. https://ned.ipac.caltech.edu/byname?objname=MESSIER+100. 
  3. ↑ 3.0 3.1 "Messier 100". Hearst Observatory. http://www.hearstobservatory.com/messier_100.html. 
  4. ↑ "Messier 100". https://messier.seds.org/m/m100.html. 
  5. ↑ 5.0 5.1 5.2 5.3 5.4 5.5 5.6 5.7 "Messier 100". SEDS: Spiral Galaxy M100 (NGC 4321), type Sc, in Coma Berenices. http://messier.seds.org/m/m100.html. 
  6. ↑ "Catalog of Nebulae and Star Clusters". SEDS. http://messier.seds.org/xtra/history/m-cat.html#M100. 
  7. ↑ 7.0 7.1 7.2 7.3 7.4 "Messier 100". SEDS: Observations and Descriptions. http://messier.seds.org/Mdes/dm100.html. 
  8. ↑ S. di Serego Alighieri (2007). "The HI content of Early-Type Galaxies from the ALFALFA survey I. Catalogued HI sources in the Virgo cluster". Astronomy and Astrophysics 474 (3): 851–855. doi:10.1051/0004-6361:20078205. Bibcode: 2007A&A...474..851D. 
  9. ↑ "NGC 4323". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+4323. 
  10. ↑ Wozniak, H.; Friedli, D.; Martinet, L.; Pfenniger, D. (1999). "Double-barred starburst galaxies viewed by ISOCAM". The Universe as Seen by ISO. 427: 989. Bibcode: 1999ESASP.427..989W. 
  11. ↑ Sakamoto, Kazushi; Okumura, Sachiko; Minezaki, Takeo; Kobayashi, Yukiyasu et al. (1995). "Bar-Driven Gas Structure and Star Formation in the Center of M100". The Astronomical Journal 110 (3): 2075. doi:10.1086/117670. Bibcode: 1995AJ....110.2075S. 
  12. ↑ Allard, E. L.; Knapen, J. H.; Peletier, R. F.; Sarzi, M. (2006). "The star formation history and evolution of the circumnuclear region of M100". Monthly Notices of the Royal Astronomical Society 371 (3): 1087–1105. doi:10.1111/j.1365-2966.2006.10751.x. Bibcode: 2006MNRAS.371.1087A. 
  13. ↑ R. A. Koopmann; J. D. P. Kenney (2004). "Hα Morphologies and Environmental Effects in Virgo Cluster Spiral Galaxies". Astrophysical Journal 613 (2): 866–885. doi:10.1086/423191. Bibcode: 2004ApJ...613..866K. 
  14. ↑ Chung, A.; Van Gorkom, J.H.; Kenney, J.F.P.; Crowl, Hugh et al. (2009). "VLA Imaging of Virgo Spirals in Atomic Gas (VIVA). I. The Atlas and the H I Properties". The Astronomical Journal 138 (6): 1741–1816. doi:10.1088/0004-6256/138/6/1741. Bibcode: 2009AJ....138.1741C. 
  15. ↑ 15.0 15.1 Pickering, E. C. (1917). "Ritchie's Nova". Harvard College Observatory Bulletin 642: 1. Bibcode: 1917BHarO.642....1P. 
  16. ↑ "SN 1901B". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=SN+1901B. 
  17. ↑ 17.0 17.1 Curtis, Heber Doust (1917). "Three novae in spiral nebulae". Lick Observatory Bulletin 300: 108. doi:10.5479/ADS/bib/1917LicOB.9.108C. Bibcode: 1917LicOB...9..108C. 
  18. ↑ "SN 1914A". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=SN+1914A. 
  19. ↑ "SN 1959E". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=SN+1959E. 
  20. ↑ Humason, M. L.; Gomes, Alercio M.; Kearns, C. E. (1961). "The 1960 Palomar Supernova Search". Publications of the Astronomical Society of the Pacific 73 (432): 175. doi:10.1086/127650. Bibcode: 1961PASP...73..175H. 
  21. ↑ "SN 1979C". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=SN+1979C. 
  22. ↑ International Astronomical Union (1979). "IAU Circular 3348". International Astronomical Union Circulars 3348 (3348): 1. Bibcode: 1979IAUC.3348....1M. https://www.cbat.eps.harvard.edu/iauc/03300/03348.html. Retrieved 2024-11-25. 
  23. ↑ "SN 2006X". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=SN+2006X. 
  24. ↑ Ponticello, N. J.; Burket, J.; Li, W.; Chen, Y. -T.; Yang, M.; Lin, C. -S.; Soma, M.; Migliardi, M. et al. (2006). "Supernovae 2006U, 2006V, 2006W, 2006X. (Lick Observatory Supernova Search)". International Astronomical Union Circular (8667): 1. Bibcode: 2006IAUC.8667....1P. http://www.cbat.eps.harvard.edu/iauc/08600/08667.html. 
  25. ↑ "SN 2006X". IAU. https://www.wis-tns.org/object/2006X. 
  26. ↑ "SN 2019ehk". IAU. https://www.wis-tns.org/object/2019ehk. 
  27. ↑ "SN 2020oi". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=SN+2020oi. 
  28. ↑ "SN 2020oi". IAU. https://www.wis-tns.org/object/2020oi. 
  1. ↑ On March 15
  2. ↑ February 21 to June 17

Template:NGC objects:4000-4499

Coordinates: Sky map 12h 22m 54.8616s, +15° 49′ 17.886″



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