NGC 1192

Last updated
NGC 1192
NGC1190 NGC1191 NGC1192 - SDSS DR14.png
NGC 1192 (on the left) (SDSS)
Observation data (J2000.0 epoch)
Constellation Eridanus
Right ascension 03h 03m 34.63s [1]
Declination −15° 40′ 43.80″ [1]
Redshift 0.032059 [1]
Helio radial velocity 9611 ± 14 km/s [1]
Distance 417 Mly
Apparent magnitude  (V)14.80 [2]
Apparent magnitude  (B)15.80 [2]
Characteristics
Type E5 [1]
Apparent size  (V)0.7 x 0.3 [1]
Other designations
PGC 11519, MCG -3-8-65, HCG 22E

NGC 1192 is a lenticular galaxy approximately 417 million light-years away from Earth in the constellation of Eridanus. [1] It was discovered by American astronomer Francis Leavenworth on December 2, 1885 with the 26" refractor at Leander McCormick Observatory. [3]

Contents

Together with NGC 1189, NGC 1190, NGC 1191 and NGC 1199 it forms Hickson Compact Group 22 (HCG 22) galaxy group. [4] Although they are considered members of this group, NGC 1191 and NGC 1192 are in fact background objects, since they are much further away compared to the other members of this group. [5]

See also

Related Research Articles

<span class="mw-page-title-main">Seyfert's Sextet</span> Group of galaxies in the constellation Serpens

Seyfert's Sextet is a group of galaxies about 190 million light-years away in the constellation Serpens. The group appears to contain six members, but one of the galaxies, NGC 6027d, is a background object and another "galaxy," NGC 6027e, is actually a part of the tail from galaxy NGC 6027. The gravitational interaction among these galaxies should continue for hundreds of millions of years. Ultimately, the galaxies will merge to form a single giant elliptical galaxy.

<span class="mw-page-title-main">NGC 201</span> Spiral galaxy in the constellation Cetus

NGC 201 is a spiral galaxy in the constellation of Cetus. It is one of the group members of HCG 7, with the other group members NGC 192, NGC 196, and NGC 197. It was discovered on December 28, 1790 by William Herschel.

<span class="mw-page-title-main">NGC 1741</span> Distant pair of interacting galaxies in the constellation Eridanus

NGC 1741 is a distant pair of interacting galaxies in the Eridanus constellation. It was discovered on 6 January 1878 by French astronomer Édouard Stephan. As a result of the collision, the galaxies are in a rapid starbust phase. The galaxies are classed as Wolf–Rayet galaxies due to their high content of rare Wolf–Rayet stars.

<span class="mw-page-title-main">NGC 4503</span> Barred lenticular galaxy in the constellation of Virgo

NGC 4503 is a barred lenticular galaxy located around 41 to 74 million light-years away in the constellation Virgo. NGC 4503 was discovered by astronomer William Herschel on March 15, 1784. NGC 4503 is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 1510</span> Galaxy in the constellation Horologium

NGC 1510 is a dwarf lenticular galaxy approximately 38 million light-years away from Earth in the constellation of Horologium. It was discovered by John Herschel on December 4, 1836.

<span class="mw-page-title-main">NGC 505</span> Lenticular galaxy in the constellation Pisces

NGC 505 is a lenticular galaxy approximately 234 million light-years away from Earth in the constellation of Pisces. It was discovered by German astronomer Albert Marth on October 1, 1864.

<span class="mw-page-title-main">NGC 509</span> Lenticular galaxy in the constellation Pisces

NGC 509 is a lenticular galaxy approximately 87 million light-years away from Earth in the constellation of Pisces. It was discovered by German astronomer Albert Marth on October 1, 1864.

<span class="mw-page-title-main">NGC 805</span> Lenticular galaxy in the constellation Triangulum

NGC 805 is a lenticular galaxy approximately 194 million light-years away from Earth in the constellation of Triangulum. It was discovered by German astronomer Heinrich Louis d'Arrest on September 26, 1864, with the 11-inch refractor at Copenhagen.

<span class="mw-page-title-main">NGC 966</span> Lenticular galaxy in the constellation Cetus

NGC 966 is an unbarred lenticular galaxy approximately 440 million light-years away from Earth in the constellation of Cetus. It was discovered by American astronomer Francis Preserved Leavenworth in 1886.

<span class="mw-page-title-main">NGC 1426</span> Elliptical galaxy in the constellation Eridanus

NGC 1426 is an elliptical galaxy approximately 59 million light-years away from Earth in the constellation of Eridanus. It was discovered by William Herschel in December 9, 1784.

<span class="mw-page-title-main">NGC 1060</span> Galaxy in the constellation Triangulum

NGC 1060 is a lenticular galaxy approximately 256 million light-years away from Earth in the constellation of Triangulum. It was discovered by William Herschel on September 12, 1784.

<span class="mw-page-title-main">NGC 1190</span> Galaxy in the constellation Eridanus

NGC 1190 is a lenticular galaxy approximately 109 million light-years away from Earth in the constellation of Eridanus. It was discovered by American astronomer Francis Leavenworth on December 2, 1885 with the 26" refractor at Leander McCormick Observatory.

<span class="mw-page-title-main">NGC 1189</span> Galaxy in the constellation Eridanus

NGC 1189 is a barred spiral galaxy approximately 105 million light-years away from Earth in the constellation of Eridanus. It was discovered by American astronomer Francis Leavenworth on December 2, 1885 with the 26" refractor at Leander McCormick Observatory.

<span class="mw-page-title-main">NGC 1191</span> Galaxy in the constellation Eridanus

NGC 1191 is a lenticular galaxy approximately 406 million light-years away from Earth in the constellation of Eridanus. It was discovered by American astronomer Francis Leavenworth on December 2, 1885 with the 26" refractor at Leander McCormick Observatory.

<span class="mw-page-title-main">NGC 1199</span> Galaxy in the constellation Eridanus

NGC 1199 is an elliptical galaxy approximately 107 million light-years away from Earth in the constellation of Eridanus. It was discovered by William Herschel on December 30, 1785.

<span class="mw-page-title-main">NGC 1436</span> Barred spiral galaxy in the constellation Eridanus

NGC 1436 is a barred spiral galaxy approximately 58 million light-years away from Earth in the constellation of Eridanus. It is a member of the Fornax I cluster.

<span class="mw-page-title-main">NGC 1262</span> Galaxy in the constellation of Eridanus

NGC 1262 is a barred spiral galaxy located in the constellation Eridanus. NGC 1262 is the most distant object in the New General Catalogue lying about 1.5 billion light-years away from Earth. NGC 1262 is also a large galaxy with a diameter of about 380,000 light-years making it nearly four times larger than the Milky Way. It was discovered by astronomer Francis Leavenworth on November 12, 1885.

<span class="mw-page-title-main">NGC 4551</span> Elliptical galaxy in the constellation Virgo

NGC 4551 is an elliptical galaxy located about 70 million light-years away in the constellation Virgo. It was discovered by astronomer William Herschel on April 17, 1784. NGC 4551 appears to lie close to the lenticular galaxy NGC 4550. However, both galaxies show no sign of interaction and have different red shifts. Both galaxies are also members of the Virgo Cluster.

<span class="mw-page-title-main">NGC 542</span> Spiral galaxy in the constellation Andromeda

NGC 542 is a spiral galaxy in the constellation Andromeda, which is approximately 215 million light years from the Milky Way. Together with the galaxies NGC 529, NGC 531, and NGC 536, it forms the Hickson Compact Group 10, abbreviated HCG 10. It was discovered by Irish astronomer R.J. Mitchell in 1885.

<span class="mw-page-title-main">NGC 5910</span> Elliptical galaxy in the constellation of Serpens

NGC 5910 is an elliptical galaxy located about 540 million light-years away in the constellation Serpens. It was discovered by astronomer William Hershel on April 13, 1785. NGC 5910 is also a strong radio source with a conspicuous nuclear jet.

References

  1. 1 2 3 4 5 6 7 "NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved December 9, 2017.
  2. 1 2 "Revised NGC Data for NGC 1192". spider.seds.org. Retrieved December 9, 2017.
  3. ↑ "Data for NGC 1192". www.astronomy-mall.com. Retrieved December 9, 2017.
  4. ↑ "A members-only galaxy club". www.spacetelescope.org. Retrieved December 9, 2017.
  5. ↑ Johnson, Kelsey E.; et al. (2007). "The Infrared Properties of Hickson Compact Groups". The Astronomical Journal . 134 (4): 1522–1543. arXiv: 0706.4461 . Bibcode:2007AJ....134.1522J. doi:10.1086/520921. S2CID   38349471.


This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.