NGC 4889

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Coma A
NGC 4889.jpg
The NGC 4889 galaxy
Credit: Sloan Digital Sky Survey, Spitzer Space Telescope
Observation data
Epoch J2000.0
Constellation Coma Berenices
Right ascension 13h 00m 08.1s[1]
Declination +27° 58′ 37″[1]
Apparent dimension (V) 2.9' × 1.9'[1]
Apparent magnitude (V) 12.9[1]
Characteristics
Type cD; E4; Dd[1]
Astrometry
Heliocentric radial velocity 6495[1] ± 13[1]km/s
Redshift 0.21665[1]
Galactocentric velocity 6509[1] ± 13[1] km/s
Other designations
Coma A, NGC 4884, UGC 8110, MCG 5-31-77, PGC 44715, ZWG 160.241, DRCG 27-148[3]
Database references
SIMBAD data
See also: Galaxy, List of galaxies

NGC 4889 (also known as Caldwell 35, Coma A) a class-4 supergiant elliptical galaxy.[4] It was discovered in 1785 by the British astronomer Frederick William Herschel I, who catalogued it as a bright patch of nebulous feature. The brightest galaxy within the northern Coma Cluster, it is located at a distance of 94 megaparsecs (Mpc; 308 million light years) from Earth. Unlike a flattened, disc-shaped spiral galaxy like the Milky Way, NGC 4889 has no visible dust lanes or spiral arms and has a smooth, featureless, egg-shaped profile that diminishes in luminosity with distance from the center. At the core of the galaxy is a giant supermassive black hole that continously heats up the intracluster medium through the action of friction from infalling gases and dust. The X-ray emission from the galaxy extends out to several million light years of the cluster.

As with other similar elliptical galaxies, only a fraction of the mass of NGC 4889 is in the form of stars. They have a flattened, unequal distribution that bulges within its edge. In addition it also has a diffuse stellar halo that extends out to 1 million light years in diameter. Orbiting the galaxy is a massive population of tens of thousands of globular clusters, compared to 200 for the Milky Way. NGC 4889 is also a strong source of soft X-ray, ultraviolet, and radio frequency radiation.

As the largest and the most massive galaxy easily visible to Earth, NGC 4889 has played an important role in different subsequent studies in astronomy, both amateur and professional astronomy, and became an important prototype in the study of other similar, supergiant elliptical galaxies in the more distant universe. NGC 4889 is itself very massive, very large, yet so easy to observe that it demonstrates the dynamical evolution of such elliptical galaxies.

Observation[edit]

Wide-field image of the Coma Cluster. NGC 4889 is the bright galaxy to the left. The galaxy at the right is NGC 4874, while the star above it is HD 112887 which is a foreground star and is completely unrelated to the cluster.

Despite being an intrinistically bright object, NGC 4889 was not included by the French astronomer Charles Messier in his famous Messier catalogue despite being relatively close to some Messier objects. The first known observation of NGC 4889 was that of Frederick William Herschel I, together with his sister and assistant collaborator, Caroline Lucretia Herschel, in 1785, which included it in the Catalogue of Nebulae and Clusters of Stars which is published a year later. In 1864, Herschel's son, John Frederick William Herschel, published the General Catalogue of Nebulae and Clusters of Stars. He included the objects catalogued by his father, including the later to be called NGC 4889, plus other objects he found that were somehow missed by his father. In 1888 the Danish-Irish astronomer John Louis Emil Dreyer published the New General Catalogue of Nebulae and Clusters of Stars (NGC), with a total of 7,840 objects, but he erroneously duplicated the galaxy in two designations, NGC 4884 and NGC 4889. Within the following century, several projects aimed to revise the NGC catalogue were conducted, such as The NGC/IC Project, Revised New General Catalogue of Nebulae and Clusters of Stars, and the NGC 2000.0 projects, discovered the duplication. It was then decided that the object to be called by its latter designation, NGC 4889, which is in use today.

In December 1995, Patrick Caldwell Moore compiled the Caldwell catalogue, a list of 109 persistent, bright objects that were somehow missed by Messier in his catalogue. The list also includes NGC 4889, which is given the designation Caldwell 35.

Properties[edit]

The location of NGC 4889 (circled) in Coma Berenices
Cercle rouge 100%.svg
The location of NGC 4889 (circled) in Coma Berenices

NGC 4889 is located along the high declination region of Coma Berenices, south of the constellation Canes Venatici. It can be traced by following the line from Beta Comae Berenices to Gamma Comae Berenices. With an apparent magnitude of 11.4, it can be seen by telescopes with 12 inch aperture, but its visibility is greatly affected by light pollution due to glare of the light from Beta Comae Berenices. However, under very dark, moonless skies, it can be seen by small telescopes as a faint smudge, but larger telescopes are needed in order to see tbe galaxy's halo.

In the updated Hubble sequence galaxy morphological classification scheme by the French astronomer Gérard de Vaucouleurs in 1959, NGC 4889 is classified as an E4 type galaxy, which means it has a featureless, egg-shaped profile that diminishes in luminosity with distance from its center. It is also classified as a cD galaxy, a giant type of D galaxy, a classification devised by the American astronomer William Wilson Morgan in 1958 for galaxies with an elliptical-shaped nucleus surrounded by an immense, diffuse, dustless, extended halo.

NGC 4889 is far enough that its distance can be measured using redshift. With the redshift of 0.0266 as derived from the Sloan Digital Sky Survey, and the Hubble constant as determined in 2013 by the ESA COBRAS/SAMBA/Planck Surveyor translates its distance of 94 Mpc (308 million light years) from Earth.

NGC 4889 is probably the largest and the most massive galaxy out to the radius of 100 Mpc (326 million light years) of the Milky Way. The galaxy spans at 2.9 arcminutes of the sky, translating it to the diameter of 239,000 light years, about the size of the Andromeda Galaxy. For comparison, the nearby supergiant elliptical Messier 87 is only a third of that size, and other Virgo Cluster galaxies are only a fourth of it, making NGC 4889 an extraordinary galaxy in astronomical terms.

As for its large size, NGC 4889 may also be extremely massive. If we took Milky Way as the standard of mass, it may be close to 8 trillion solar masses. However, as NGC 4889 is a spheroid, and not a flat spiral, it has a three-dimensional profile, so it may be as high as 15 trillion solar masses. However, as for elliptical galaxies, only a small fraction of the mass of NGC 4889 is in the form of stars that radiate energy. Assuming a mass to light ratio of 6.5 as with other elliptical galaxies, NGC 4889 may be a thousand times more massive than the Milky Way.

Components[edit]

In addition to its 300,000 light year stellar halo, NGC 4889 also has an extended halo out to 750,000 light years. In addition it has a very large population of globular clusters, possibly as high as 35,000, compared to 200 for the Milky Way, seen as faint blue and greenish spots in the infobox image. It also has a giant X-ray halo that continuously heats up the cluster. Orbiting NGC 4889 are many dwarf galaxies, which are currently being bound to the massive gravity of NGC 4889.

Supermassive black hole[edit]

On December 5, 2011, astronomers measured the velocity dispersion of the central regions of two massive galaxies, NGC 4889, and the other being NGC 3842 in the Leo Cluster. According to the data of the study, they found out the central black hole of NGC 4889 is 5,200 times more massive than the central black hole of the Milky Way, or equivalent to 2.1×1010 (21 billion) solar masses (best fit of data; possible range is from 6 billion to 37 billion solar masses).[5] This makes it one of the most massive black holes on record. The diameter of the black hole's immense event horizon is about 124 billion kilometers, 12 times the diameter of Pluto's orbit. The ionized medium detected around the black hole suggests that NGC 4889 may have been a quasar in the past.

Environment[edit]

NGC 4889 lies at the center of the component A of the Coma Cluster, a giant cluster of 20,000 galaxies which it shares with NGC 4874, although NGC 4889 is sometimes referred as the cluster center, and it has been called by its other designation A1656-BCG.

The Coma Cluster is located at exactly the center of the Coma Supercluster, which is one of the nearest superclusters to the Laniakea Supercluster. The Coma Supercluster itself is within the CfA Homunculus, the center of the CfA2 Great Wall, the nearest galaxy filament to Earth and one of the largest structures in the known universe.

See also[edit]

Notes[edit]

  1. ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for 3C 147. Retrieved 2010-05-02. 
  2. ^ "Distance Results for NGC 4889". NASA/IPAC Extragalactic Database. Retrieved 2015-01-04. 
  3. ^ Revised NGC Data for NGC 4889
  4. ^ Jacobsen, Den (2006). "Abell 1656, NGC 4889, NGC 4874". astrophoto.net. Retrieved 2008-08-09. 
  5. ^ McConnell, Nicholas J. (2011-12-08). "Two ten-billion-solar-mass black holes at the centres of giant elliptical galaxies". Nature. Archived from the original on 2011-12-06. Retrieved 2011-12-06. 

References[edit]

  • Pasachoff, Jay M. (2000). "Atlas of the Sky". Stars and Planets. New York, NY: Peterson Field Guides. ISBN 0-395-93432-X. 
  • Eicher, David J. (1988). The Universe from Your Backyard: A Guide to Deep-Sky Objects from Astronomy Magazine. AstroMedia (Kalmbach Publishing Company). ISBN 0-521-36299-7. 

External links[edit]