Messier 85

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Messier 85
Messier85 - HST - Potw1905a.jpg
Galaxy Messier 85 by Hubble Space Telescope
Observation data (J2000 epoch)
Constellation Coma Berenices
Right ascension 12h 25m 24.0s [1]
Declination +18° 11′ 28″ [1]
Redshift 729 ± 2 km/s [1]
Distance 60 ± 4 Mly (18.5 ± 1.2 Mpc) [2]
Apparent magnitude  (V)9.1 [3]
Characteristics
Type SA(s)0+ pec [1] /E2 [4]
Apparent size  (V)7′.1 × 5′.5 [1]
Other designations
NGC 4382, UGC 7508, PGC 40515 [1]

Messier 85 (also known as M85 or NGC 4382 or PGC 40515 or ISD 0135852) is a lenticular galaxy, or elliptical galaxy for other authors, [4] in the Coma Berenices constellation. It is 60 million light-years away, and it is estimated to be 125,000 light-years across.

Contents

Pierre Méchain discovered M85 in 1781. It is within the outskirts of the Virgo cluster, and is relatively isolated. [5]

Properties

M85 is extremely poor in neutral hydrogen [6] and has a very complex outer structure with shells and ripples that are thought to have been caused by a merger with another galaxy that took place between 4 and 7 billion years ago, [6] as well as a relatively young (<3 billion years old) stellar population on its centermost region, some of it in a ring, that may have been created by a late starburst. [7] Like other massive, early-type galaxies, it has different populations of globular clusters. Aside from the typical "red" and "blue" populations, there is also a population with intermediate colors and an even redder population. [5] It is likely transitioning from being a lenticular galaxy into an elliptical galaxy. [5]

While indirect methods imply that Messier 85 should contain a central supermassive black hole of around 100 million solar masses, [8] velocity dispersion observations imply that the galaxy may entirely lack a central massive black hole. [9]

M85 is interacting with the nearby spiral galaxy NGC 4394, and a small elliptical galaxy called MCG 3-32-38. [10]

Compared to other early-type galaxies, M85 emits a relatively smaller proportion of X-rays. [5]

Novae and Supernovae

The type I supernova, SN 1960R was discovered in M85 on December 20, 1960 and reached an apparent magnitude of 11.7 (its effect in the telescope-resolvable sky to outshine most red dwarves a million times closer).

This galaxy has also been the host of the first luminous red nova identified as such, M85 OT2006-1. It was discovered on January 7 of 2006 and took place on the outskirts of this galaxy. [11]

On 25 June 2020, the ATLAS telescope in Hawaii spotted type Ia supernova SN 2020nlb in M85, which reached a peak magnitude of 12.0. [12] [13] [14]

Location of M85 M85map.png
Location of M85

See also

Related Research Articles

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An elliptical galaxy is a type of galaxy with an approximately ellipsoidal shape and a smooth, nearly featureless image. They are one of the four main classes of galaxy described by Edwin Hubble in his Hubble sequence and 1936 work The Realm of the Nebulae, along with spiral and lenticular galaxies. Elliptical (E) galaxies are, together with lenticular galaxies (S0) with their large-scale disks, and ES galaxies with their intermediate scale disks, a subset of the "early-type" galaxy population.

<span class="mw-page-title-main">Virgo Cluster</span> Galaxy cluster in the constellation Virgo

The Virgo Cluster is a large cluster of galaxies whose center is 53.8 ± 0.3 Mly away in the constellation Virgo. Comprising approximately 1,300 member galaxies, the cluster forms the heart of the larger Virgo Supercluster, of which the Local Group is a member. The Local Group actually experiences the mass of the Virgo Supercluster as the Virgocentric flow. It is estimated that the Virgo Cluster's mass is 1.2×1015M☉ out to 8 degrees of the cluster's center or a radius of about 2.2 Mpc.

<span class="mw-page-title-main">Lenticular galaxy</span> Class of galaxy between an elliptical galaxy and a spiral galaxy

A lenticular galaxy is a type of galaxy intermediate between an elliptical and a spiral galaxy in galaxy morphological classification schemes. It contains a large-scale disc but does not have large-scale spiral arms. Lenticular galaxies are disc galaxies that have used up or lost most of their interstellar matter and therefore have very little ongoing star formation. They may, however, retain significant dust in their disks. As a result, they consist mainly of aging stars. Despite the morphological differences, lenticular and elliptical galaxies share common properties like spectral features and scaling relations. Both can be considered early-type galaxies that are passively evolving, at least in the local part of the Universe. Connecting the E galaxies with the S0 galaxies are the ES galaxies with intermediate-scale discs.

<span class="mw-page-title-main">Messier 61</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">Centaurus A</span> Radio galaxy in the constellation Centaurus

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<span class="mw-page-title-main">NGC 5866</span> Galaxy in the constellation Draco

NGC 5866 is a lenticular galaxy in the constellation Draco. NGC 5866 was most likely discovered by Pierre Méchain or Charles Messier in 1781, and independently found by William Herschel in 1788. Measured orbital velocities of its globular cluster system imply that dark matter makes up only 34±45% of the mass within 5 effective radii, a notable paucity.

<span class="mw-page-title-main">Messier 49</span> Elliptical galaxy in the constellation Virgo

Messier 49 is a giant elliptical galaxy about 56 million light-years away in the equatorial constellation of Virgo. This galaxy was discovered by astronomer Charles Messier in 1777.

<span class="mw-page-title-main">Messier 59</span> Elliptical galaxy in the constellation Virgo

Messier 59 or M59, also known as NGC 4621, is an elliptical galaxy in the equatorial constellation of Virgo. It is a member of the Virgo Cluster, with the nearest fellow member 8′ away and around 5 magnitudes fainter. The nearest cluster member of comparable brightness is the lenticular galaxy NGC 4638, which is around 17′ away. It and the angularly nearby elliptical galaxy Messier 60 were both discovered by Johann Gottfried Koehler in April 1779 when observing comet seeming close by. Charles Messier listed both in the Messier Catalogue about three days after Koehler's discovery.

<span class="mw-page-title-main">Messier 60</span> Elliptical galaxy in the constellation Virgo

Messier 60 or M60, also known as NGC 4649, is an elliptical galaxy approximately 57 million light-years away in the equatorial constellation of Virgo. Together with NGC 4647, it forms a pair known as Arp 116. Messier 60 and nearby elliptical galaxy Messier 59 were discovered by Johann Gottfried Koehler in April 1779, observing a comet in the same part of the sky. Charles Messier added both to his catalogue about three days after this.

<span class="mw-page-title-main">Messier 84</span> Galaxy in the constellation Virgo

Messier 84 or M84, also known as NGC 4374, is a giant elliptical or lenticular galaxy in the constellation Virgo. Charles Messier discovered the object in 1781 in a systematic search for "nebulous objects" in the night sky. It is the 84th object in the Messier Catalogue and in the heavily populated core of the Virgo Cluster of galaxies, part of the local supercluster.

<span class="mw-page-title-main">Messier 86</span> Elliptical galaxy in the constellation Virgo

Messier 86 is an elliptical or lenticular galaxy in the constellation Virgo. It was discovered by Charles Messier in 1781. M86 lies in the heart of the Virgo Cluster of galaxies and forms a most conspicuous group with another large galaxy known as Messier 84. It displays the highest blue shift of all Messier objects, as it is, net of its other vectors of travel, approaching the Milky Way at 244 km/s. This is due to both galaxies falling roughly towards the center of the Virgo cluster from opposing ends.

<span class="mw-page-title-main">Messier 89</span> Elliptical galaxy in the constellation Virgo

Messier 89 is an elliptical galaxy in the constellation Virgo. It was discovered by Charles Messier on March 18, 1781. M89 is a member of the Virgo Cluster of galaxies.

<span class="mw-page-title-main">NGC 3115</span> Galaxy in the constellation Sextans

NGC 3115 is a field lenticular (S0) galaxy in the constellation Sextans. The galaxy was discovered by William Herschel on February 22, 1787. At about 32 million light-years away from Earth, it is several times bigger than the Milky Way. It is a lenticular (S0) galaxy because it contains a disk and a central bulge of stars, but without a detectable spiral pattern. NGC 3115 is seen almost exactly edge-on, but was nevertheless mis-classified as elliptical. There is some speculation that NGC 3115, in its youth, was a quasar.

<span class="mw-page-title-main">Messier 110</span> Satellite galaxy of the Andromeda Galaxy

Messier 110, or M110, also known as NGC 205, is a dwarf elliptical galaxy that is a satellite of the Andromeda Galaxy in the Local Group.

<span class="mw-page-title-main">NGC 1316</span> Lenticular radio galaxy in the constellation Fornax

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<span class="mw-page-title-main">NGC 4526</span> Lenticular galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 3585</span> Galaxy in the constellation Hydra

NGC 3585 is an elliptical or a lenticular galaxy located in the constellation Hydra. It is located at a distance of circa 60 million light-years from Earth, which, given its apparent dimensions, means that NGC 3585 is about 80,000 light years across. It was discovered by William Herschel on December 9, 1784.

<span class="mw-page-title-main">NGC 4278</span> Galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 4318</span> Galaxy in the constellation Virgo

NGC 4318 is a small lenticular galaxy located about 72 million light-years away in the constellation Virgo. It was discovered by astronomer John Herschel on January 18, 1828. NGC 4318 is a member of the Virgo W′ group, a group of galaxies in the background of the Virgo Cluster that is centered on the giant elliptical galaxy NGC 4365.

References

  1. 1 2 3 4 5 6 "NASA/IPAC Extragalactic Database". Results for Messier 85. Retrieved 18 November 2006.
  2. ↑ J. L. Tonry; A.Dressler; J. P. Blakeslee; E. A. Ajhar; et al. (2001). "The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances". Astrophysical Journal . 546 (2): 681–693. arXiv: astro-ph/0011223 . Bibcode:2001ApJ...546..681T. doi:10.1086/318301. S2CID   17628238.
  3. ↑ "Messier 85". SEDS Messier Catalog. Retrieved 30 April 2022.
  4. 1 2 Kormendy, John; Fisher, David B.; Cornell, Mark E.; Bender, Ralf (2009). "Structure and Formation of Elliptical and Spheroidal Galaxies". Astrophysical Journal Supplement . 182 (1): 216–309. arXiv: 0810.1681 . Bibcode:2009ApJS..182..216K. doi:10.1088/0067-0049/182/1/216. S2CID   119273143.
  5. 1 2 3 4 Escudero, Carlos G.; Cortesi, Arianna; Faifer, Favio R.; Sesto, Leandro A.; Smith Castelli, Analía V.; Johnston, Evelyn J.; Reynaldi, Victoria; Chies-Santos, Ana L.; Salinas, Ricardo; Menéndez-Delmestre, Karín; Gonçalves, Thiago S.; Grossi, Marco; Mendes De Oliveira, Claudia (2022). "The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster". Monthly Notices of the Royal Astronomical Society. 511 (1): 393–412. arXiv: 2201.01759 . Bibcode:2022MNRAS.511..393E. doi:10.1093/mnras/stac021.
  6. 1 2 Hibbard, J. E.; Sansom, A. E. (2003). "A Search for H I in Five Elliptical Galaxies with Fine Structure". The Astronomical Journal . 125 (2): 667–683. arXiv: astro-ph/0211003 . Bibcode:2003AJ....125..667H. doi:10.1086/345822. S2CID   14748737.
  7. ↑ Fisher, David; Franx, Marijn; Illingworth, Garth (1996). "Line Strengths and Line-Strength Gradients in S0 Galaxies". Astrophysical Journal . 459 (1): 110. Bibcode:1996ApJ...459..110F. doi:10.1086/176873.
  8. ↑ Kormendy, John; Bender, Ralf (2009). "Correlations between Supermassive Black Holes, Velocity Dispersions, and Mass Deficits in Elliptical Galaxies with Cores". Astrophysical Journal Letters . 691 (2): L142–L146. arXiv: 0901.3778 . Bibcode:2009ApJ...691L.142K. doi:10.1088/0004-637X/691/2/L142. S2CID   18919128.
  9. ↑ Gultekin, Kayhan; Richstone, Douglas O.; et al. (2011). "Is There a Black Hole in NGC 4382?". Astrophysical Journal . 741 (1): L142–L146. arXiv: 1108.1808 . Bibcode:2011ApJ...741...38G. doi:10.1088/0004-637X/741/1/38. S2CID   411264.
  10. ↑ "M85, Lenticular Galaxy". Messier's Nebulae and Star Clusters. Retrieved 29 March 2009.
  11. ↑ Kulkarni, S. R.; Ofek, E. O.; Rau, A.; Cenko, S. B.; et al. (2007). "An unusually brilliant transient in the galaxy M85". Nature . 447 (7143): 458–460. arXiv: 0705.3668 . Bibcode:2007Natur.447..458K. doi:10.1038/nature05822. PMID   17522679. S2CID   4300285.
  12. ↑ "AstroNote 2020-126". ATLAS20qoq (AT2020nlb): discovery of a candidate SN in MESSIER 85 (17 Mpc). Retrieved 26 June 2020.
  13. ↑ "Messier 85". SEDS: Galaxy M85. Retrieved 23 February 2010.[ permanent dead link ]
  14. ↑ "SN 2020nlb". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 23 February 2010.
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