Messier 73

Messier 73 (M73, also known as NGC 6994) is an asterism of four stars in the constellation of Aquarius several arcminutes east of M72, a globular cluster. An asterism mainly refers to any bright stars as viewed from Earth appearing to form a reasonably sized, normally published, imagined shape in the sky but is used here in the sense of a loose optical double: gravitationally unconnected stars that appear close in the sky.

Messier 73
Messier 073 2MASS.jpg
Observation data (J2000 epoch)
ConstellationAquarius
Right ascension20h 58m 54s[1][2]
Declination−12° 38′[1][2]
DistanceMean distance star approx. 2,500 ly[2] (approx. 770 pc)
Apparent magnitude (V)9.0m[1][2]
Apparent dimensions (V)2.8′[2]
Physical characteristics
Radiusly
Estimated agemillion yrs[citation needed]
Other designationsM 73, NGC 6994,[1][2] Cr 426
See also: Open cluster, List of open clusters

HistoryEdit

M73 was discovered by Charles Messier in 1780[a] who originally described the object as a cluster of four stars with some nebulosity. Much later observations by John Herschel could not find any nebulosity. Moreover, Herschel noted that the designation of M73 as a cluster was questionable. Nonetheless, Herschel included M73 in his General Catalogue of clusters, nebulaæ, and galaxies, and John Dreyer included M73 when he compiled the New General Catalogue.[3]

Scientific research: asterism or open cluster?Edit

M73 was once treated as a potential sparsely populated open cluster, which consists of stars that are physically associated in space as well as on the sky. The question of whether the stars were an asterism or an open cluster generated a small, interesting debate.

In 2000, L. P. Bassino, S. Waldhausen, and R. E. Martinez published an analysis of the colors and luminosities of the stars in and around M73. They concluded that the four bright central stars and some other nearby stars followed the color-luminosity relation that is also followed by stars in open clusters (as seen in a Hertzsprung-Russell diagram). Their conclusion was that M73 was an old open cluster that was 9  wide.[4] However, G. Carraro, published results in 2000 based on a similar analysis and concluded that the stars did not follow any color-luminosity relation. Carraro's conclusion was that M73 was an asterism.[5] Adding to the controversy, E. Bica and collaborators concluded that the chance alignment of the four bright stars seen in the center of M73 as well as one other nearby star was highly unlikely, so M73 was probably a sparse open cluster.[6] The controversy was solved in 2002, when M. Odenkirchen and C. Soubiran published an analysis of the high resolution spectra of the six brightest stars within 6  of the centre point. They demonstrated that the distances from the Earth to the six stars were very different from each other, and the stars were moving in different directions. Therefore, they concluded that the stars were only an asterism.[7]

Although M73 was determined to be only a chance alignment of stars, further analysis of asterisms is still important for the identification of sparsely populated open clusters. A full study of very many such clusters would demonstrate how, how often, and to what degree open clusters are ripped apart by the gravitational forces in the Milky Way and reveal more of the sources of these forces.

LocationEdit

 
These stars appear in the same space as a typical star cluster in the southwest of the very mildly southern constellation of Aquarius

See alsoEdit

Notes and referencesEdit

  1. ^ on October 4
  1. ^ a b c d "M 73". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2006-12-21.
  2. ^ a b c d e f "Messier 73". SEDS Messier pages. Retrieved 2010-02-28.
  3. ^ K. G. Jones (1991). Messier's Nebulae and Star Clusters (2nd ed.). Cambridge University Press. ISBN 978-0-521-37079-0.
  4. ^ L. P. Bassino; S. Waldhausen & R. E. Martinez (2000). "CCD photometry in the region of NGC 6994: The remains of an old open cluster". Astronomy & Astrophysics. 355: 138–144. arXiv:astro-ph/0001238. Bibcode:2000A&A...355..138B.
  5. ^ G. Carraro (2000). "NGC 6994: An open cluster which is not an open cluster". Astronomy & Astrophysics. 357: 145–148. arXiv:astro-ph/0003372. Bibcode:2000A&A...357..145C.
  6. ^ E. Bica; B. X. Santiago; C. M. Dutra; H. Dottori; M. R. de Oliveira & D. Pavani (2001). "Dissolving star cluster candidates". Astronomy & Astrophysics. 366 (3): 827–833. arXiv:astro-ph/0011280. Bibcode:2001A&A...366..827B. doi:10.1051/0004-6361:20000248.
  7. ^ M. Odenkirchen & C. Soubiran (2002). "NGC 6994: Clearly not a physical stellar ensemble". Astronomy & Astrophysics. 383 (1): 163–170. arXiv:astro-ph/0111601. Bibcode:2002A&A...383..163O. doi:10.1051/0004-6361:20011730.

External linksEdit

Coordinates:   20h 58m 54s, −12° 38′ 00″