Messier 100

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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.[1] It is one of the brightest and largest galaxies in the Virgo Cluster and is approximately 55 million light-years[2] from our galaxy, about 166,000 light-years in diameter. It was discovered by Pierre Méchain in 1781Template:Efn and 29 days later seen again and entered by Charles Messier in his catalogue "of nebulae and star clusters".[3][4] It was one of the first spiral galaxies to be discovered,[4] 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.[5][6]

Early observations

File:Widefield View of M100.png
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[4] to recognize the nebula because of its faintness. William Herschel was able to identify a bright cluster of stars[4] 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[4] 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[7] 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[8] – where star formation has been taking place for at least 500 million years in separate bursts.[9]

As usual on spiral galaxies of the Virgo Cluster, in the rest of the disk both star formation[10] and neutral hydrogen, of which M100 is deficient compared to isolated spiral galaxies of similar Hubble type,[11] are truncated within the galaxy's disk, which is caused by interactions with the intracluster medium of Virgo.

Supernovae

File:Noirlab2019b.jpg
Supernova SN 2019ehk in M100 (Hubble)

Seven supernovae have been identified in M100:[1]

  • On 17 March 1901 Heber Curtis discovered SN 1901B (Type I, mag. 15.6),[12][1][13] at 110"W and 4"N from the galaxy's nucleus.[14]
  • Heber Curtis discovered SN 1914A (type unknown, mag. 15.7)[1][15] on 2 March 1914, at 24"E and 111"S from the galaxy's nucleus.[12][14]
  • Milton Humason, with observations from early to mid 1960,Template:Efn discovered SN 1959E (Type I, mag. 17.5),[1][16] located 58"E and 21"S from the galaxy's nucleus.[17]
  • 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.[1][18][19]
  • 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.[1][20][21][22]
  • Jaroslaw Grzegorzek discovered SN 2019ehk ([[Type Ib and Ic supernovae|TypeTemplate:NbspIb]], mag. 16.5) on 29 April 2019. The supernova reached a peak magnitude of approximately 15.8.[23]
  • SN 2020oi ([[Type Ib and Ic supernovae|TypeTemplate:NbspIc]], mag. 17.28) was discovered by Automatic Learning for the Rapid Classification of Events (ALeRCE) on 7 January 2020.[1][24][25]

See also

References and footnotes

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External links

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