Messier 58
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Messier 58 (also known as ''M58'' and ''NGC 4579'') is an intermediate barred spiral galaxy with a weak inner ring structure located within the
constellation A constellation is an area on the celestial sphere in which a group of visible stars forms Asterism (astronomy), a perceived pattern or outline, typically representing an animal, mythological subject, or inanimate object. The first constellati ...
Virgo Virgo may refer to: Arts and entertainment * Virgo (film), a 1970 Egyptian film * Virgo (character), several Marvel Comics characters * Virgo Asmita, a character in the manga ''Saint Seiya: The Lost Canvas'' * ''Virgo'' (album), by Virgo Four, ...
, approximately 68 million
light-year A light-year, alternatively spelled light year (ly or lyr), is a unit of length used to express astronomical distances and is equal to exactly , which is approximately 9.46 trillion km or 5.88 trillion mi. As defined by the International Astr ...
s away from
Earth Earth is the third planet from the Sun and the only astronomical object known to Planetary habitability, harbor life. This is enabled by Earth being an ocean world, the only one in the Solar System sustaining liquid surface water. Almost all ...
. It was discovered by
Charles Messier Charles Messier (; 26 June 1730 – 12 April 1817) was a French astronomer. He published an astronomical catalogue consisting of 110 nebulae and star clusters, which came to be known as the ''Messier objects'', referred to with th ...
on April 15, 1779 and is one of four barred spiral galaxies that appear in Messier's catalogue.The other barred spiral galaxies in Messier's catalogue are Messier 91,
Messier 95 Messier 95, also known as M95 or NGC 3351, is a barred spiral galaxy about 33 million light-years away in the zodiac constellation Leo. It was discovered by Pierre Méchain in 1781, and catalogued by compatriot Charles Messier four days la ...
and
Messier 109 Messier 109 (also known as NGC 3992 or the Vacuum Cleaner Galaxy) is a barred spiral galaxy exhibiting a weak inner ring structure around the central bar approximately away in the northern constellation Ursa Major. M109 can be seen south-east of ...
M58 is one of the brightest galaxies in the
Virgo Cluster The Virgo Cluster is a cluster of galaxies whose center is 53.8 ± 0.3 Mly (16.5 ± 0.1 Mpc) away in the Virgo constellation. Comprising approximately 1,300 (and possibly up to 2,000) member galaxies, the cluster forms the heart of the larger ...
. From 1779 it was arguably (though unknown at that time) the farthest known astronomical object until the release of the
New General Catalogue The ''New General Catalogue of Nebulae and Clusters of Stars'' (abbreviated NGC) is an astronomical catalogue of deep-sky objects compiled by John Louis Emil Dreyer in 1888. The NGC contains 7,840 objects, including galaxy, galaxies, star cluste ...
in the 1880s and even more so the publishing of redshift values in the 1920s.


Early observations

Charles Messier discovered Messier 58, along with the
elliptical galaxies An elliptical galaxy is a type of galaxy with an approximately ellipsoidal shape and a smooth, nearly featureless image. They are one of the three main classes of galaxy described by Edwin Hubble in his Hubble sequence and 1936 work ''The Re ...
Messier 59 Messier 59 or M59, also known as NGC 4621, is an elliptical galaxy in the celestial equator, equatorial constellation of Virgo (constellation), Virgo. It is a member of the Virgo Cluster, with the nearest fellow member away and around 5 magnitud ...
and
Messier 60 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 ellipti ...
, on April 15, 1779. M58 was reported on the chart of the Comet of 1779 as it was almost on the same parallel as the star
Epsilon Virginis Epsilon Virginis (ε Virginis, abbreviated Epsilon Vir, ε Vir), formally named Vindemiatrix , is a star in the zodiac constellation of Virgo. The apparent visual magnitude of this star is +2.8, making it the third-brightest member of Vi ...
. Messier described M58 as a very faint
nebula A nebula (; or nebulas) is a distinct luminescent part of interstellar medium, which can consist of ionized, neutral, or molecular hydrogen and also cosmic dust. Nebulae are often star-forming regions, such as in the Pillars of Creation in ...
in Virgo which would disappear in the slightest amount of light he used to illuminate the
micrometer Micrometer can mean: * Micrometer (device), used for accurate measurements by means of a calibrated screw * Micrometre The micrometre (English in the Commonwealth of Nations, Commonwealth English as used by the International Bureau of Weights ...
wires. This description was later contradicted by John Herschel's observations in 1833 where he described it as a very bright galaxy, especially towards the middle. Herschel's observations were also similar to the descriptions of both
John Dreyer John Dreyer may refer to: *John Louis Emil Dreyer, Danish-Irish astronomer *John Dreyer (footballer) John Brian Dreyer (born 11 June 1963) is an English former professional footballer and manager who played in defence and midfield. Playing care ...
and
William Henry Smyth Admiral William Henry Smyth (21 January 1788 – 8 September 1865) was an English Royal Navy officer, hydrographer, astronomer and numismatist. He is noted for his involvement in the early history of a number of learned societies, for his hy ...
who said that M58 was a bright galaxy, mottled, irregularly round and very much brighter toward the middle.


Characteristics

Like many other spiral galaxies of the Virgo Cluster (e.g.
Messier 90 Messier 90 (also known as M90 and NGC 4569) is an intermediate spiral galaxy exhibiting a weak inner ring structure about 60 million light-years away in the constellation Virgo. It was discovered by Charles Messier in 1781. Membership of the ...
), Messier 58 is an
anemic galaxy An anemic galaxy is a type of spiral galaxy characterized by a low contrast between its spiral arms and its disk. Etymology The term was coined in 1976 by the Canadian astronomer Sidney van den Bergh to classify galaxies that are an intermed ...
with low
star formation Star formation is the process by which dense regions within molecular clouds in interstellar space—sometimes referred to as "stellar nurseries" or "star-forming regions"—Jeans instability, collapse and form stars. As a branch of astronomy, sta ...
activity concentrated within the galaxy's optical disk, and relatively little
neutral hydrogen The hydrogen line, 21 centimeter line, or H I line is a spectral line that is created by a change in the energy state of solitary, electrically neutral hydrogen atoms. It is produced by a spin-flip transition, which means the directio ...
, also located inside its disk, concentrated in clumps, compared with other galaxies of similar morphological type. This deficiency of gas is believed to be caused by interactions with Virgo's
intracluster medium In astronomy, the intracluster medium (ICM) is the superheated plasma (physics), plasma that permeates a galaxy cluster. The gas consists mainly of ionized hydrogen and helium and accounts for most of the baryonic material in galaxy clusters. The ...
. Messier 58 has a low-luminosity
active galactic nucleus An active galactic nucleus (AGN) is a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars. Such e ...
, where a
starburst MicroPro International Corporation was an American software company founded in 1978 in San Rafael, California. They are best known as the publisher of WordStar, a popular early word processor for personal computers. History Founding and early su ...
may be present as well as a
supermassive black hole A supermassive black hole (SMBH or sometimes SBH) is the largest type of black hole, with its mass being on the order of hundreds of thousands, or millions to billions, of times the mass of the Sun (). Black holes are a class of astronomical ...
with a mass of around 70 million
solar mass The solar mass () is a frequently used unit of mass in astronomy, equal to approximately . It is approximately equal to the mass of the Sun. It is often used to indicate the masses of other stars, as well as stellar clusters, nebulae, galaxie ...
es. It is also one of the very few galaxies known to possess a UCNR (''ultra-compact nuclear ring''), a series of star-forming regions located in a very small ring around the center of the galaxy. This led to its being dubbed the "ring bearer galaxy" by the
popular astronomy Amateur astronomy is a hobby where participants enjoy observing or imaging celestial objects in the sky using the unaided eye, binoculars, or telescopes. Even though scientific research may not be their primary goal, some amateur astronomers m ...
YouTube program "Deep Sky videos".


Supernovae

Two
supernova A supernova (: supernovae or supernovas) is a powerful and luminous explosion of a star. A supernova occurs during the last stellar evolution, evolutionary stages of a massive star, or when a white dwarf is triggered into runaway nuclear fusion ...
e have been observed in the M58 galaxy: * SN 1988A ( type II, mag. 13.5) was discovered by Kaoru Ikeya,
Robert Evans Robert Evans (born Robert J. Shapera; June 29, 1930 – October 26, 2019) was an American film producer who worked on ''Rosemary's Baby (film), Rosemary's Baby'' (1968), ''Love Story (1970 film), Love Story'' (1970), ''The Godfather'' (1972), ...
,
Christian Pollas Christian Pollas (b. 1947) is a French astronomer, known for the discovery and observation of minor planets and supernovae. Pollas is credited by the Minor Planet Center with the discovery of 26 asteroids, some co-discovered with Eric W. Elst, ...
and Shingo Horiguchi on January 18, 1988. It was found 40
arcseconds A minute of arc, arcminute (abbreviated as arcmin), arc minute, or minute arc, denoted by the symbol , is a unit of angular measurement equal to of a degree. Since one degree is of a turn, or complete rotation, one arcminute is of a tu ...
south of the galaxy center. * SN 1989M (
Type Ia A Type Ia supernova (read: "type one-A") is a type of supernova that occurs in binary systems (two stars orbiting one another) in which one of the stars is a white dwarf. The other star can be anything from a giant star to an even smaller white ...
, mag. 12.2) was discovered by Givi N. Kimeridze on 28 June 1989. It was found 33 arcseconds north and 44 arcseconds west of M58's nucleus.


See also

*
List of Messier objects The Messier objects are a set of 110 astronomical objects catalogued by the French astronomer Charles Messier in his ' (''Catalogue of Nebulae and Star Clusters''). Because Messier was interested only in finding comets, he created a list of th ...
* Messier 91 *
Messier 95 Messier 95, also known as M95 or NGC 3351, is a barred spiral galaxy about 33 million light-years away in the zodiac constellation Leo. It was discovered by Pierre Méchain in 1781, and catalogued by compatriot Charles Messier four days la ...
*
Messier 109 Messier 109 (also known as NGC 3992 or the Vacuum Cleaner Galaxy) is a barred spiral galaxy exhibiting a weak inner ring structure around the central bar approximately away in the northern constellation Ursa Major. M109 can be seen south-east of ...
* M100 *
NGC 4536 NGC 4536 is an intermediate spiral galaxy in the constellation Virgo. It was discovered by German-British astronomer William Herschel on 24 January 1784. NGC 4536 is located about 10° south of the midpoint of the Virgo cluster. However, it is ...


Notes


References


External links


SEDS Messier: M58Spitzer Space Telescope page on Messier 58
* {{DEFAULTSORT:Messier 58 Intermediate spiral galaxies Messier 058 Messier 058
058 58 may refer to: * 58 (number) * one of the years 58 BC, AD 58, 1958, 2058 * 58 (band), an American rock band * 58 (golf), a round of 58 in golf * "Fifty Eight", a song by Karma to Burn from the album ''Arch Stanton ''Arch Stanton'' is t ...
Messier 058 07796 42168 Astronomical objects discovered in 1779 Discoveries by Charles Messier