NGC 6566

Last updated
NGC 6566
Observation data (J2000 epoch)
Constellation Draco
Right ascension 18h 07m 00.65042s [1]
Declination +52° 15 36.6716 [1]
Redshift 0.01768 [2]
Heliocentric radial velocity 5252 km/s [2]
Distance 250.6 ± 17.7  Mly (76.84 ± 5.43  Mpc) [3]
Apparent magnitude  (B)15.47 [4]
Characteristics
Type cE [4]
Other designations
MCG +09-30-001, PGC 61418 [2]

NGC 6566 is a compact [4] elliptical galaxy [4] within the constellation Draco. It is located about 250 million light-years (80 Mpc) [3] away from the Sun. [3] It was discovered on October 27, 1861 by the astronomer Heinrich d'Arrest. [5]

Related Research Articles

<span class="mw-page-title-main">NGC 27</span> Galaxy in the constellation Andromeda

NGC 27 is a spiral galaxy located in the constellation Andromeda. It was discovered on 3 August 1884 by Lewis Swift. It forms a galaxy pair with the nearby UGC 95.

<span class="mw-page-title-main">NGC 4777</span> Galaxy in the constellation Virgo

NGC 4777 is an intermediate spiral ring galaxy. It is estimated to be about 180 million light-years away from the Sun. It was discovered on March 3, 1786 by the astronomer William Herschel.

<span class="mw-page-title-main">NGC 3260</span> Galaxy in the constellation Antlia

NGC 3260 is an elliptical galaxy in the constellation Antlia. It is a member of the Antlia Cluster, which lies about 40.7 megaparsecs away. It was discovered on May 2, 1834 by the astronomer John Herschel.

<span class="mw-page-title-main">NGC 321</span> Elliptical galaxy in the Cetus constellation

NGC 321 is an elliptical galaxy located in the constellation Cetus. It was discovered on September 27, 1864, by the astronomer Albert Marth. Measurements of its redshift put it at a distance of about 217.4 ± 15.4 megalight-years (66.67 ± 4.73 Mpc), assuming a Hubble constant of H0 = 67.8 km/sec/Mpc.

<span class="mw-page-title-main">NGC 62</span> Barred spiral galaxy in the constellation Cetus

NGC 62 is a barred spiral galaxy in the constellation Cetus. NGC 62 is its New General Catalogue designation. It has an apparent magnitude of 13.2.

<span class="mw-page-title-main">NGC 63</span> Galaxy in the constellation Pisces

NGC 63 is a spiral galaxy in the constellation Pisces. NGC 63 is its New General Catalogue designation. It has an apparent V-band magnitude of 12.70.

<span class="mw-page-title-main">UGC 9796</span> Lenticular and polar ring galaxy in the constellation Bootes

UGC 9796 is a lenticular and polar-ring galaxy in the constellation Boötes, and about 250 million light years distant from Earth. It is an object of great scientific interest as there have been very few polar ring galaxies discovered. UGC 9796 is a very gas-rich environment hosting as much 5×109 solar masses of neutral hydrogen. DSS and SDSS images show that it is very similar to polar ring galaxy NGC 660, the best-known of all the polar ring galaxies.

<span class="mw-page-title-main">NGC 66</span> Galaxy in the constellation Cetus

NGC 66 is a barred spiral galaxy discovered by Frank Muller in 1886, and is located in the Cetus constellation.

<span class="mw-page-title-main">NGC 69</span> Galaxy in the constellation Andromeda

NGC 69 is a barred lenticular galaxy located in the constellation Andromeda. It is a member of the NGC 68 group. It was discovered in 1855 by R. J. Mitchell, who described it as "extremely faint, very small, round."

<span class="mw-page-title-main">NGC 112</span> Galaxy in the constellation Andromeda

NGC 112 is a barred spiral galaxy located in the constellation Andromeda. It was discovered by American astronomer Lewis Swift on September 17, 1885. The galaxy lies approximately 295 million light-years from Earth, and is about 75,000 light-years in diameter.

<span class="mw-page-title-main">NGC 114</span> Galaxy in the constellation Cetus

NGC 114 is a barred lenticular galaxy located in the constellation Cetus. It was discovered by American astronomer Truman Henry Safford on September 23, 1867. The galaxy lies approximately 195 million light-years from Earth, and is about 55,000 light-years in diameter, nearly half the size of the Milky Way.

<span class="mw-page-title-main">NGC 119</span> Unbarred lenticular galaxy in Phoenix

NGC 119 is an unbarred lenticular galaxy with an apparent magnitude of 13.0 located in the constellation Phoenix. It was discovered on October 28, 1834, by the astronomer John Herschel.

<span class="mw-page-title-main">NGC 120</span> Galaxy in the constellation Cetus

NGC 120 is a lenticular galaxy of type SB0? pec? with an apparent magnitude of 13.4 located in the constellation Cetus. It was discovered on 27 September 1880 by Wilhelm Tempel.

<span class="mw-page-title-main">NGC 4500</span> Galaxy in the constellation Ursa Major

NGC 4500 is a barred spiral galaxy in the constellation Ursa Major. The galaxy was discovered on April 17, 1789 by William Herschel. It is a blue compact galaxy.

<span class="mw-page-title-main">NGC 471</span> Galaxy in the constellation Pisces

NGC 471 is a lenticular galaxy located about 168 million light-years away from Earth in the constellation Pisces. It was discovered by the German astronomer Albert Marth on November 3, 1864.

<span class="mw-page-title-main">NGC 2460</span> Galaxy in the constellation Camelopardalis

NGC 2460 is an unbarred spiral galaxy in the constellation Camelopardalis. It was discovered by German astronomer Wilhelm Tempel on August 11, 1882.

<span class="mw-page-title-main">NGC 999</span> Galaxy in the constellation Andromeda

NGC 999 is an intermediate spiral galaxy located in the constellation Andromeda about 195 million light-years from the Milky Way. It was discovered by French astronomer Edouard Stephan on 8 December 1871.

<span class="mw-page-title-main">NGC 970</span> Pair of interacting galaxies in the constellation Triangulum

NGC 970 is an interacting galaxy pair in the constellation Triangulum. It is estimated to be 471 million light-years from the Milky Way and has a diameter of approximately 100,000 ly. The object was discovered on September 14, 1850, by Bindon Blood Stoney.

<span class="mw-page-title-main">NGC 995</span> Galaxy in the constellation Andromeda

NGC 995 is a lenticular galaxy located in the constellation Andromeda about 178 million light years from the Milky Way. It was discovered by the French astronomer Édouard Stephan on 8 December 1871.

<span class="mw-page-title-main">NGC 823</span> Galaxy in the constellation Fornax

NGC 823, also known as IC 1782, is an unbarred lenticular galaxy in the constellation Fornax. It is estimated to be 194 million light-years from the Milky Way and has a diameter of approximately 100,000 light years. NGC 823 was discovered on October 14, 1830, by astronomer John Herschel.

References

  1. 1 2 Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics . 616. A1. arXiv: 1804.09365 . Bibcode: 2018A&A...616A...1G . doi: 10.1051/0004-6361/201833051 .
  2. 1 2 3 "NGC 6566". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2021-02-03.
  3. 1 2 3 "Results for object NGC 6566 (NGC 6566)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2021-02-03.
  4. 1 2 3 4 "Search specification: NGC 6566". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-02-03.
  5. "New General Catalog Objects: NGC 6550 - 6599". cseligman.com. Retrieved 2018-11-05.