IC 4026 | |
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Observation data | |
Constellation | Coma Berenices |
Right ascension | 195.0 degrees |
Declination | 28.04 degrees |
Redshift | 0.02727 |
Heliocentric radial velocity | 8,196 km/s |
Distance | 315 Mly (96.5 Mpc) |
Group or cluster | Coma Cluster |
Apparent magnitude (V) | 14.63 |
Surface brightness | 11.99 mag/arcsec |
Characteristics | |
Type | SB0 |
Size | 70,000 ly |
Other designations | |
PGC 44749, CGCG 160-250, WBL 426-100, AGC 221386, UZC J130022.0+280250, NSA 104078, SDSS J130022.12+280249.2, 2MASX J13002215+2802495, [DZ2015] 703-29, MaNGA 01-456903, LEDA 44749 |
IC 4026 is a type S0 lenticular galaxy with a bar [1] located in Coma Berenices. [2] [3] It is located 315 million light-years away from the Solar System and has an approximate diameter of 70,000 light-years which is less the size of the Milky Way. [4] IC 4026 was discovered on May 11, 1896, by astronomer Hermann Kobold [5] and is a member of the Coma Cluster. [4] [6] [7] It has a surface brightness of 11.99 mag/arcsecs meaning it is a high surface brightness galaxy. [8]
LEDA 83677 is a lenticular galaxy located about 290 million light-years away in the constellation Coma Berenices. It is a member of the Coma cluster of galaxies. LEDA 83677 is also classified as a type 1 Seyfert galaxy. The core of the galaxy is emitting high-energy X-rays and ultraviolet light, probably caused by a massive black hole lurking in the core.
NGC 4477 is a barred lenticular galaxy located about 55 million light-years away in the constellation of Coma Berenices. NGC 4477 is classified as a type 2 Seyfert galaxy. The galaxy was discovered by astronomer William Herschel on April 8, 1784. NGC 4477 is a member of Markarian's Chain which forms part of the larger Virgo Cluster.
NGC 4489 is a dwarf elliptical galaxy located about 60 million light-years away in the constellation of Coma Berenices. It was discovered by astronomer William Herschel on March 21, 1784. NGC 4489 is a member of the Virgo Cluster.
NGC 4873 is a lenticular galaxy located about 270 million light-years away in the constellation of Coma Berenices. NGC 4873 was discovered by astronomer Heinrich d'Arrest on May 10, 1863. The galaxy is a member of the Coma Cluster.
NGC 4919 is a lenticular galaxy located about 340 million light-years away in the constellation of Coma Berenices. NGC 4919 was discovered by astronomer Heinrich d'Arrest on May 5, 1864. NGC 4919 is a member of the Coma Cluster.
NGC 4479 is a barred lenticular galaxy located about 60 million light-years away in the constellation of Coma Berenices. NGC 4479 was discovered by astronomer William Herschel on April 8, 1784. It is a member of the Virgo Cluster.
NGC 4474 is an edge-on lenticular galaxy located about 50 million light-years away in the constellation Coma Berenices. NGC 4474 was discovered by astronomer William Herschel on April 8, 1784. It is a member of the Virgo Cluster.
NGC 4515 is a lenticular galaxy located about 57 million light-years away in the constellation Coma Berenices. NGC 4515 was discovered by astronomer William Herschel on March 21, 1784. The galaxy is a member of the Virgo Cluster.
NGC 4540 is a spiral galaxy with type 1 Seyfert activity located about 64 million light-years away in the constellation Coma Berenices. NGC 4540 was discovered by astronomer William Herschel on March 21, 1784 and is a member of the Virgo Cluster.
NGC 4659 is a lenticular galaxy located about 54 million light-years away in the constellation Coma Berenices. NGC 4659 was discovered by astronomer William Herschel on April 12, 1784 and is a member of the Virgo Cluster.
NGC 4875 is a lenticular galaxy located about 350 million light-years away in the constellation Coma Berenices. NGC 4875 was discovered by astronomer Guillaume Bigourdan on May 16, 1885. The galaxy is a member of the Coma Cluster.
NGC 4883 is a barred lenticular galaxy located about 315 million light-years away in the constellation Coma Berenices. NGC 4883 was discovered by astronomer Heinrich d'Arrest on April 22, 1865. It is a member of the Coma Cluster.
NGC 4895 is a lenticular galaxy located 330 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer Heinrich d'Arrest on May 5, 1864 and is a member of the Coma Cluster.
NGC 646 is a large barred spiral galaxy located in the constellation Hydrus. Its speed relative to the cosmic microwave background is 8,145 ± 19 km/s, which corresponds to a Hubble distance of 120.1 ± 8.4 Mpc. NGC 646 was discovered by British astronomer John Herschel in 1834. It forms an interacting galaxy pair.
NGC 945 is a barred spiral galaxy in the constellation Cetus. It is located south of the celestial equator. It is estimated to be 200 million light-years from the Milky Way and about 135,000 light-years in diameter. Together with NGC 948, it forms a gravitationally bound pair of galaxies. In the same area of the sky there are, among other things: the galaxies NGC 942, NGC 943, NGC 950, IC 230. The Type Ib supernova SN 1998dt was observed here. The object was discovered by astronomer William Herschel on November 28, 1785. It is within close proximity to NGC 948.
IC 3528 is a Seyfert 1.5 type spiral galaxy with X-ray emission located 660 million light-years away in the constellation of Coma Berenices. It lies near to spiral galaxy NGC 4540, although the two of them are quite far. The object was discovered by Royal Harwood Frost on May 7, 1904. Although listed as a member in the Virgo Cluster Catalogue as VCC 1593, it is not a member of the Virgo cluster but a background galaxy.
NGC 2494 is a lenticular galaxy located in the Monoceros constellation. It is 183 million light-years away and about 58,000 light-years in diameter.
NGC 5008 is a massive barred spiral galaxy located in the Boötes constellation.
NGC 3750 is a lenticular galaxy with a bar located in the constellation of Leo. It is located 450 million light-years from the Solar System and was discovered by Ralph Copeland on February 9, 1874.
NGC 3748 is a lenticular galaxy with a bar located in the Leo constellation. It is located 440 million light-years away from the Solar System and was discovered by Ralph Copeland on April 5, 1874, but also observed by Hermann Kobold, Lawrence Parsons and John Louis Emil Dreyer.
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