NGC 523

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NGC 523
NGC523 - SDSS DR14.jpg
NGC 523 as seen on SDSS
Observation data (J2000 [1] epoch)
Constellation Andromeda
Right ascension 01h 23.3m 00s [1]
Declination +34° 02′ 00″ [1]
Redshift 0.0159 [2]
Heliocentric radial velocity 4758 +/− 4 km/s [3]
Galactocentric velocity4904 +/− 7 km/s [3]
Distance 219 million light years away [2]
Apparent magnitude  (V)12.7 [2]
Apparent magnitude  (B)13.5 [1]
Characteristics
Type SBc/P [2]
Apparent size  (V)2.5 feet x 42 inches [2]
Other designations
NGC 537, 4ZW 45, Arp 158, CGCG 521-22, IRAS 01225+3345, MCG 6-4-18, PGC 5268, UGC 979, V V 783 [2]

NGC 523, also known as Arp 158, from the ARP catalog is a spiral galaxy located in the constellation Andromeda. [1] It was discovered separately by William Herschel on 13 September 1784, and by Heinrich d'Arrest on 13 August 1862. d'Arrest's discovery was listed as NGC 523, while Herschel's was listed as NGC 537; the two are one and the same. [4] John Dreyer noted in the New General Catalogue that NGC 523 is a double nebula. [1]

Contents

In September 2001 a type Ia supernova, SN 2001en was discovered in NGC 523. [5]

See also

Related Research Articles

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NGC 68 is a lenticular galaxy, and the central member of the NGC 68 group, in the constellation Andromeda. The galaxy was discovered on September 11, 1784, by William Herschel, who observed the NGC 68 group as a single object and described it as "extremely faint, large, 3 or 4 stars plus nebulosity". As such, his reported location is between NGC 68, NGC 70, and NGC 71. By the time Dreyer looked at the galaxies to add to the NGC catalog, however, he was able to tell that the single galaxy observed by Herschel was in fact 3 adjacent galaxies, and cataloged them as NGC 68, NGC 70, and NGC 71.

<span class="mw-page-title-main">NGC 71</span> Galaxy in the constellation Andromeda

NGC 71 is an elliptical galaxy located in the constellation Andromeda. It is in the NGC 68 group. The galaxy was discovered by R. J. Mitchell in 1855, and observed in 1865 by Heinrich d'Arrest, who described it as "extremely faint, very small, round". The galaxy is about 110,000-130,000 light years across, making it just slightly larger than the Milky Way. The galaxy is the second largest in the NGC 68 group, after spiral galaxy NGC 70.

<span class="mw-page-title-main">NGC 7003</span> Galaxy in the constellation Delphinus

NGC 7003 is a spiral galaxy around 220 million light-years from Earth in the constellation Delphinus. NGC 7003 has an estimated diameter of 80,800 light-years. The galaxy was discovered by German astronomer Heinrich Louis d'Arrest on August 26, 1864. There also has been at least one supernova observed in NGC 7003.

<span class="mw-page-title-main">NGC 507</span> Galaxy in the constellation Pisces

NGC 507, also known as Arp 229, CGCG 502-67, MCG 5-4-44, PGC 5098, UGC 938, and V V 207, is a lenticular galaxy in the constellation Pisces. It was described as being "very faint", "pretty large", "round", "brighter in the middle", and "south of NGC 508" by John Dreyer in the New General Catalogue. The two galaxies are a part of the Atlas of Peculiar Galaxies, where NGC 507 is described as "Circular or near circular rings of small density difference."

<span class="mw-page-title-main">NGC 7042</span> Galaxy in the constellation Pegasus

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<span class="mw-page-title-main">NGC 7051</span> Galaxy in the constellation Aquarius

NGC 7051 is a barred spiral galaxy located about 100 million light-years away in the constellation of Aquarius. It was discovered by astronomer John Herschel on July 30, 1827.

<span class="mw-page-title-main">NGC 4454</span> Galaxy in the constellation Virgo

NGC 4454 is a barred spiral galaxy located about 123 million light-years away in the constellation of Virgo. NGC 4454 was discovered by astronomer William Herschel on April 17, 1784.

<span class="mw-page-title-main">NGC 4907</span> Barred spiral galaxy in the constellation Coma Berenices

NGC 4907 is a barred spiral galaxy located about 270 million light-years away in the constellation of Coma Berenices. It is also classified as a LINER galaxy. NGC 4907 was discovered by astronomer Heinrich d'Arrest on May 5, 1864. The galaxy is a member of the Coma Cluster, located equidistant between NGC 4928 and NGC 4829.

<span class="mw-page-title-main">NGC 477</span> Galaxy in the constellation Andromeda

NGC 477 is a spiral galaxy in the constellation Andromeda. It is located approximately 250 million light-years from Earth and was discovered on October 18, 1786 by astronomer William Herschel.

<span class="mw-page-title-main">NGC 485</span> Spiral galaxy in the constellation Pisces

NGC 485, also commonly referred to as PGC 4921 or GC 270, is a spiral galaxy in the constellation Pisces. It is located approximately 86 million light-years from Earth and was discovered on January 8, 1828 by astronomer William Herschel. It was later also observed by Heinrich d'Arrest and Herman Schultz. When NGC 485 was originally categorized in the New General Catalogue by John Louis Eil Dreyer in 1888, it was incorrectly described as a "considerably faint, pretty large, round, 8th magnitude star 3 1/2 arcmin to southwest".

<span class="mw-page-title-main">NGC 495</span> Galaxy in the constellation Pisces

NGC 495, also occasionally referred to as PGC 5037, UGC 920 or GC 278, is a barred spiral galaxy in the constellation Pisces. It is located approximately 184 million light-years from the Solar System and was discovered on 12 September 1784 by astronomer William Herschel.

<span class="mw-page-title-main">NGC 4523</span> Spiral galaxy in the constellation Coma Berenices

NGC 4523 is a Magellanic spiral galaxy located about 35 to 50 million light-years away in the constellation Coma Berenices. It was discovered by astronomer Heinrich d'Arrest on April 19, 1865. NGC 4523 is a member of the Virgo Cluster. A distance of for NGC 4523 was derived from using yellow supergiants in the galaxy as standard candles.

<span class="mw-page-title-main">NGC 504</span> Lenticular galaxy in the constellation Pisces

NGC 504, also occasionally referred to as PGC 5084 or UGC 935, is a lenticular galaxy located approximately 189 million light-years from the Solar System in the constellation Pisces. It was discovered on 22 November 1827 by astronomer John Herschel. The object was listed twice in the General Catalogue, precursor of the New General Catalogue, as both GC 291 and GC 292.

<span class="mw-page-title-main">NGC 508</span> Galaxy in the constellation Pisces

NGC 508, also occasionally referred to as PGC 5099 or UGC 939, is an elliptical galaxy in the constellation Pisces. It is located approximately 247 million light-years from the Solar System and was discovered on 12 September 1784 by British astronomer William Herschel.

<span class="mw-page-title-main">NGC 512</span> Spiral galaxy in the constellation Andromeda

NGC 512, also occasionally referred to as PGC 5132 or UGC 944, is a spiral galaxy in the constellation Andromeda. It is located approximately 217 million light-years from the Solar System and was discovered on 17 November 1827 by astronomer John Herschel.

<span class="mw-page-title-main">NGC 513</span> Galaxy in the constellation Andromeda

NGC 513, also occasionally referred to as PGC 5174 or UGC 953, is a spiral galaxy in the constellation Andromeda. It is located approximately 262 million light-years from the Solar System and was discovered on 13 September 1784 by astronomer William Herschel.

<span class="mw-page-title-main">NGC 517</span> Lenticular galaxy in the constellation Pisces

NGC 517, also occasionally referred to as PGC 5214 or UGC 960, is a lenticular galaxy located approximately 188 million light-years from the Solar System in the constellation Pisces. It was discovered on 13 September 1784 by astronomer William Herschel.

<span class="mw-page-title-main">NGC 3336</span> Galaxy in the constellation Hydra

NGC 3336 is a barred spiral galaxy located about 190 million light-years away in the constellation Hydra. It was discovered by astronomer John Herschel on March 24, 1835. NGC 3336 is a member of the Hydra Cluster.

<span class="mw-page-title-main">NGC 1268</span> Spiral galaxy in the constellation Perseus

NGC 1268 is a spiral galaxy located about 140 million light-years away in the constellation Perseus. It was discovered by astronomer Heinrich d'Arrest on February 14, 1863. NGC 1268 is a member of the Perseus Cluster and appears to show signs of distortion in the form of bridges. These features may be the result of a strong interaction with NGC 1267.

<span class="mw-page-title-main">NGC 3873</span> Galaxy in the constellation Leo

NGC 3873 is an elliptical galaxy located about 300 million light-years away in the constellation Leo. The galaxy was discovered by astronomer Heinrich d'Arrest on May 8, 1864. NGC 3873 is a member of the Leo Cluster.

References

  1. 1 2 3 4 5 6 Frommert, Hartmut. "NGC 523". spider.seds.org.
  2. 1 2 3 4 5 6 Rojas, Sebastián García. "Galaxy NGC 523 · Deep Sky Objects Browser". DSO Browser.[ permanent dead link ]
  3. 1 2 "Your NED Search Results". ned.ipac.caltech.edu.
  4. ↑ "New General Catalog Objects: NGC 500 – 549". cseligman.com.
  5. ↑ Bishop, David. "Supernova 2001en in NGC 523". Rochester Astronomy.org. Retrieved 21 October 2018.


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