NGC 5308

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NGC 5308
NGC 5308.png
NGC 5308 imaged by the Hubble Space Telescope, along with LEDA 2802348 (right)
Observation data (J2000 epoch)
Constellation Ursa Major
Right ascension 13h 47m 00.392s [1]
Declination +60° 58 22.94 [1]
Redshift 0.006665 [2]
Heliocentric radial velocity 1998 km/s [2]
Distance 95.48 ± 16.78  Mly (29.275 ± 5.144  Mpc) [2]
Group or cluster NGC 5322 group (LGG 360) [3]
Apparent magnitude  (B)12.5 [4]
Characteristics
Type S0 [2]
Size103,200  ly (31,640  pc) [2]
Apparent size  (V)3.7 × 0.7 [2]
Other designations
UGC 8722, PGC 48860, CGCG 295-012 [4]

NGC 5308 is an edge-on lenticular galaxy in the constellation of Ursa Major. It was discovered on 19 March 1790 by William Herschel. [5] It was described by John Louis Emil Dreyer as "bright, pretty large" when he compiled the New General Catalogue. [6] A small, irregular galaxy near NGC 5308 has been given the designation LEDA 2802348. [7]

Contents

NGC 5308 was imaged by the Hubble Space Telescope in 2016. The galaxy appears to be a flat, smooth disk, typical of most lenticular galaxies. Many large globular clusters orbit the galaxy; these are visible as tiny dots surrounding the galaxy, and are mostly made of old, aging stars similar to the galaxy itself. [8]

NGC 5322 Group

According to A.M. Garcia, the galaxy NGC 5308 is a member of the NGC 5322 group (also known as LGG 360), which contains at least 10 other galaxies, inclulding NGC 5322, NGC 5342, NGC 5372, NGC 5376, NGC 5379, NGC 5389, UGC 8684, UGC 8714, and UGC 8716. [9]

Supernova

One supernova has been observed in NGC 5308: SN 1996bk (type Ia, mag. 14.5) was discovered by Piero Mazza and Stefano Pesci on 12 October 1996, located 10.5" south and 17.9" west of center of the galaxy. [10] [11]

See also

Related Research Articles

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<span class="mw-page-title-main">NGC 3550</span> Galaxy in the constellation Ursa Major

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<span class="mw-page-title-main">NGC 5679 Group</span> Triplet of galaxies in the constellation Virgo

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<span class="mw-page-title-main">NGC 7499</span> Galaxy in the constellation Pisces

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<span class="mw-page-title-main">NGC 2748</span> Galaxy in the constellation Camelopardalis

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−3.6
×107 M
, or 44 million times the mass of the Sun.

<span class="mw-page-title-main">NGC 1222</span> Lenticular galaxy in the constellation Eridanus

NGC 1222 is an early-type lenticular galaxy located in the constellation of Eridanus. The galaxy was discovered on 5 December 1883 by the French astronomer Édouard Stephan. John Louis Emil Dreyer, the compiler of the New General Catalogue, described it as a "pretty faint, small, round nebula" and noted the presence of a "very faint star" superposed on the galaxy.

<span class="mw-page-title-main">NGC 5011</span> Galaxy in the constellation Centaurus

NGC 5011 is an elliptical galaxy in the constellation of Centaurus. It was discovered on 3 June 1834 by John Herschel. It was described as "pretty bright, considerably small, round, among 4 stars" by John Louis Emil Dreyer, the compiler of the New General Catalogue.

<span class="mw-page-title-main">NGC 5559</span> Galaxy in the constellation Boötes

NGC 5559 is a barred spiral galaxy, located 240 million light-years away in the constellation of Boötes. It was discovered on April 10, 1785, by the astronomer William Herschel.

<span class="mw-page-title-main">NGC 515</span> Galaxy in the constellation Pisces

NGC 515, also occasionally referred to as PGC 5201 or UGC 956, is a lenticular galaxy located approximately 228 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 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 521</span> Spiral galaxy in the constellation Cetus

NGC 521, also occasionally referred to as PGC 5190 or UGC 962, is a barred spiral galaxy located approximately 224 million light-years from the Solar System in the constellation Cetus. It was discovered on 8 October 1785 by astronomer William Herschel.

<span class="mw-page-title-main">NGC 525</span> Galaxy in the constellation Pisces

NGC 525, also occasionally referred to as PGC 5232 or UGC 972, is a lenticular galaxy located approximately 95.6 million light-years from the Solar System in the constellation Pisces. It was discovered on 25 September 1862 by astronomer Heinrich d'Arrest.

<span class="mw-page-title-main">NGC 4242</span> Galaxy in constellation Canes Venatici

NGC 4242 is a spiral galaxy in the northern constellation of Canes Venatici. The galaxy is about 18 million light years away. It was discovered on 10 April 1788 by William Herschel, and it was described as "very faint, considerably large, irregular, round, very gradually brighter in the middle, resolvable" by John Louis Emil Dreyer, the compiler of the New General Catalogue.

<span class="mw-page-title-main">NGC 2300</span> Galaxy in the constellation Cepheus

NGC 2300 is a lenticular galaxy in the constellation Cepheus. Its velocity with respect to the cosmic microwave background is 1876 ± 7 km/s, which corresponds to a Hubble distance of 90.2 ± 6.3 Mly (27.67 ± 1.94 Mpc). However, 11 non redshift measurements give a distance of 131.98 ± 21.75 Mly (40.464 ± 6.668 Mpc). The galaxy was discovered in 1871 by French astronomer Alphonse Borrelly using an 18 cm telescope.

<span class="mw-page-title-main">NGC 2227</span> Galaxy in the constellation Canis Major

NGC 2227 is a barred spiral galaxy with a morphological type of SB(rs)c located in the direction of the Canis Major constellation. It was discovered on January 27, 1835, by John Herschel.

<span class="mw-page-title-main">NGC 996</span> Galaxy in the constellation Andromeda

NGC 996 is an elliptical galaxy of the Hubble type E0 in the constellation Andromeda. It is estimated to be 210 million light years from the Milky Way and has a diameter of approximately 75,000 ly. It was discovered on December 7, 1871 by astronomer Édouard Stephan.

<span class="mw-page-title-main">NGC 2801</span> Galaxy in the constellation Cancer

NGC 2801 is a spiral galaxy in the constellation Cancer. Its velocity with respect to the cosmic microwave background is 8011 ± 20 km/s, which corresponds to a Hubble distance of 385.4 ± 27.0 Mly (118.16 ± 8.28 Mpc). It was discovered February 17, 1865, by Albert Marth.

<span class="mw-page-title-main">NGC 3254</span> Spiral galaxy in the constellation Leo Minor

NGC 3254 is a spiral galaxy in the constellation Leo Minor. It was discovered on March 13, 1785, by the astronomer William Herschel. It is a member of the NGC 3254 Group of galaxies, which is a member of the Leo II Groups, a series of galaxies and galaxy clusters strung out from the right edge of the Virgo Supercluster.

<span class="mw-page-title-main">NGC 1819</span> Lenticular galaxy in the Orion constellation

NGC 1819 is a lenticular galaxy in the constellation of Orion. It was discovered on December 26, 1885, by American astronomer Lewis A. Swift. This galaxy is located at a distance of 197.4 million light-years (60.53 Mpc) from the Milky Way, and is receding with a heliocentric radial velocity of 4,483 km/s.

References

  1. 1 2 Cutri, Roc M.; Skrutskie, Michael F.; Van Dyk, Schuyler D.; Beichman, Charles A.; Carpenter, John M.; Chester, Thomas; Cambresy, Laurent; Evans, Tracey E.; Fowler, John W.; Gizis, John E.; Howard, Elizabeth V.; Huchra, John P.; Jarrett, Thomas H.; Kopan, Eugene L.; Kirkpatrick, J. Davy; Light, Robert M.; Marsh, Kenneth A.; McCallon, Howard L.; Schneider, Stephen E.; Stiening, Rae; Sykes, Matthew J.; Weinberg, Martin D.; Wheaton, William A.; Wheelock, Sherry L.; Zacarias, N. (2003). "VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)". CDS/ADC Collection of Electronic Catalogues. 2246: II/246. Bibcode:2003yCat.2246....0C.
  2. 1 2 3 4 5 6 "NED results for object NGC 5308". National Aeronautics and Space Administration / Infrared Processing and Analysis Center . Retrieved 21 February 2017.
  3. "NGC 5322". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 21 February 2017.
  4. 1 2 "NGC 5308". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 21 February 2017.
  5. Seligman, Courtney. "New General Catalogue objects: NGC 5300 – 5349". cseligman.com. Retrieved 21 February 2017.
  6. "NGC 5308 – SEDS". seds.org. Retrieved 21 February 2017.
  7. "LEDA 2802348". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 21 February 2017.
  8. "Busy bees | ESA/Hubble". spacetelescope.org. 2016. Retrieved 21 February 2017.
  9. Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G.
  10. Mazza, P.; et al. (1996). "Supernova 1996bk in NGC 5308". IAU Circ. 6491: 1. Bibcode:1996IAUC.6491....1M.
  11. "SN 1996bk". Transient Name Server. IAU . Retrieved 9 December 2024.