IC 1296

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IC 1296
IC 1296 (crop).jpg
IC 1296, as seen by Spitzer
Observation data (J2000 epoch)
Constellation Lyra
Right ascension 18h 53m 18s
Declination +33° 03’ 59”
Redshift 0.017075
Heliocentric radial velocity 5,119 km/s
Distance 238 Mly (72.97 Mpc)
Surface brightness 23.63 mag/arcsec^2
Characteristics
Type SBbc
Size120,000 ly
Apparent size  (V)1.10' x 0.9'
Other designations
IC 1296, UGC 11374, PGC 62532, CGCG 201-040, MCG +06-41-022, 2MASX J18531883+3303596, 2MASS J18531884+3303599

IC 1296 is an extremely faint barred spiral galaxy of Hubble-type SBbc in the constellation Lyra in the northern sky. It is estimated to be 238 million light-years from the Milky Way and about 120,000 light-years in diameter. [1]

Contents

IC 1296 is only 4 arc minutes away from the well-known Ring Nebula in the night sky. [2] Planetary nebulae and galaxies are rarely observed together because planetary nebulae are galactic objects and are concentrated toward our galactic center, where extragalactic objects – such as distant galaxies – are rarely observed due to absorption by gas and dust.

The astronomical object was discovered on October 2, 1893, by Edward Emerson Barnard. In August 2013, supernova SN2013ev was discovered in the southern spiral arm of IC 1296. [3]

The Ring Nebula. IC 1296 is visible as the faint galaxy to the right. Messier 57 Ring Nebula and IC 1296 spiral galaxy.jpg
The Ring Nebula. IC 1296 is visible as the faint galaxy to the right.

See also

Related Research Articles

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<span class="mw-page-title-main">Planetary nebula</span> Type of emission nebula created by dying red giants

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<span class="mw-page-title-main">Hoag's Object</span> Unusual galaxy in the constellation Serpens

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<span class="mw-page-title-main">Ring Nebula</span> Planetary nebula in Lyra

The Ring Nebula is a planetary nebula in the northern constellation of Lyra.[C] Such a nebula is formed when a star, during the last stages of its evolution before becoming a white dwarf, expels a vast luminous envelope of ionized gas into the surrounding interstellar space.

<span class="mw-page-title-main">Astronomical object</span> Large natural physical entity in space

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<span class="mw-page-title-main">H II region</span> Large, low-density interstellar cloud of partially ionized gas

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

The Whirlpool Galaxy, also known as Messier 51a (M51a) or NGC 5194, is an interacting grand-design spiral galaxy with a Seyfert 2 active galactic nucleus. It lies in the constellation Canes Venatici, and was the first galaxy to be classified as a spiral galaxy. It is 7.22 megaparsecs away and 23.58 kiloparsecs (76,900 ly) in diameter.

<span class="mw-page-title-main">Small Sagittarius Star Cloud</span> Star cloud in Sagittarius

The Small Sagittarius Star Cloud is a star cloud in the constellation of Sagittarius approximately 600 light years wide, which was catalogued by Charles Messier in 1764. It should not be confused with the nearby Large Sagittarius Star Cloud which lies about 10° to the south.

<span class="mw-page-title-main">Messier 58</span> Galaxy in the constellation Virgo

Messier 58 is an intermediate barred spiral galaxy with a weak inner ring structure located within the constellation Virgo, approximately 68 million light-years away from Earth. It was discovered by Charles Messier on April 15, 1779 and is one of four barred spiral galaxies that appear in Messier's catalogue. M58 is one of the brightest galaxies in the Virgo Cluster. From 1779 it was arguably the farthest known astronomical object until the release of the New General Catalogue in the 1880s and even more so the publishing of redshift values in the 1920s.

<span class="mw-page-title-main">Little Dumbbell Nebula</span> Planetary nebula in the constellation Perseus

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<span class="mw-page-title-main">Messier 90</span> Galaxy in the constellation Virgo

Messier 90 is an intermediate spiral galaxy exhibiting a weak inner ring structure about 60 million light-years away[a] in the constellation Virgo. It was discovered by Charles Messier in 1781.

<span class="mw-page-title-main">Owl Nebula</span> Planetary nebula in the constellation Ursa Major

The Owl Nebula is a planetary nebula approximately 2,030 light years away in the constellation Ursa Major. Estimated to be about 8,000 years old, it is approximately circular in cross-section with a faint internal structure. It was formed from the outflow of material from the stellar wind of the central star as it evolved along the asymptotic giant branch. The nebula is arranged in three concentric shells, with the outermost shell being about 20–30% larger than the inner shell. The owl-like appearance of the nebula is the result of an inner shell that is not circularly symmetric, but instead forms a barrel-like structure aligned at an angle of 45° to the line of sight.

<span class="mw-page-title-main">Caldwell catalogue</span> Astronomical objects catalogued by Patrick Moore

The Caldwell catalogue is an astronomical catalogue of 109 star clusters, nebulae, and galaxies for observation by amateur astronomers. The list was compiled by Patrick Moore as a complement to the Messier catalogue.

<span class="mw-page-title-main">Abell 31</span> Astronomical object

Abell 31 is an ancient planetary nebula in the constellation of Cancer. It is estimated to be about 2,000 light years away. Although it is one of the largest planetary nebulae in the sky, it is not very bright. The central star of the planetary nebula is a white dwarf with a spectral type of DAO. The white dwarf is the dead remains of a star that existed but had died leaving behind Abell 31 and the white dwarf.

<span class="mw-page-title-main">Abell Catalog of Planetary Nebulae</span> Astronomical catalog

The Abell Catalog of Planetary Nebulae was created in 1966 by George O. Abell and was composed of 86 entries thought to be planetary nebulae.

<span class="mw-page-title-main">NGC 2242</span> Planetary nebula in the constellation Auriga

NGC 2242 is a planetary nebula in the constellation Auriga. It was discovered by Lewis A. Swift on November 24, 1886, and was thought to be a galaxy until a study published in 1987 showed it to be a planetary nebula. The nebula is located about 6,500 light-years away, and about 1,600 light-years above the galactic plane.

<span class="mw-page-title-main">IC 5332</span> Spiral Galaxy in the constellation Sculptor

IC 5332, also known as PGC 71775 is an intermediate spiral galaxy about 30 million light-years away in the constellation Sculptor. IC 5332 is not visible to the naked eye with an apparent magnitude of 10.72. Viewed from earth, it is nearly face on. It has a very small central bulge and open spiral arms accounting for its SABc classification. The galaxy lies in the direction of the galactic south pole.

<span class="mw-page-title-main">NGC 7013</span> Spiral or lenticular galaxy in the constellation Cygnus

NGC 7013 is a relatively nearby spiral or lenticular galaxy estimated to be around 37 to 41.4 million light-years away from Earth in the constellation of Cygnus. NGC 7013 was discovered by English astronomer William Herschel on July 17, 1784 and was also observed by his son, astronomer John Herschel on September 15, 1828.

<span class="mw-page-title-main">NGC 3313</span> Galaxy in the constellation Hydra

NGC 3313 is a large barred spiral galaxy located about 55 megaparsecs away in the constellation Hydra. It was discovered by astronomer Ormond Stone in 1886 and is an outlying member of the Hydra Cluster.

References

  1. "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-06-06.
  2. "Ring Nebula (Messier 57) | Deep⋆Sky Corner". deepskycorner.ch. Retrieved 2024-06-06.
  3. "Revised IC Data for IC 1296". spider.seds.org. Retrieved 2024-06-06.