IC 4026 | |
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![]() Sloan Digital Sky Survey image of IC 4026 | |
Observation data (J2000 epoch) | |
Constellation | Coma Berenices |
Right ascension | 13h 00m 22.136s |
Declination | +28d 02m 49.24s |
Redshift | 0.027269 |
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 lenticular galaxy located in Coma Berenices. [1] 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. [2] IC 4026 was discovered on May 11, 1896, by astronomer Hermann Kobold [3] and is a member of the Coma Cluster. [2] [4] [5] It has a surface brightness of 11.99 mag/arcsecs meaning it is a high surface brightness galaxy. [6]
IC 4026 shows a bar, indicating it might a barred lenticular galaxy of S0 morphology. [7] [8] [9] It has a central budge and an outer disc structure. [10]
To date, six redshift measurements give IC 4026 a distance of 92.483 ± 18.339 Megaparsecs or equivalent to (~ 302 Mly). This value is outside the Hubble Distance values. [11]
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NGC 7020 is a barred lenticular galaxy located about 140 million light-years away in the constellation Pavo. NGC 7020 was discovered by astronomer John Herschel on August 31, 1836.
NGC 4026 is an edge-on lenticular galaxy in the constellation Ursa Major. It is located at a distance of circa 50 million light years from Earth, which, given its apparent dimensions, means that NGC 4026 is about 80,000 light years across. It was discovered by William Herschel on April 12, 1789.
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NGC 708 is an elliptical galaxy located 240 million light-years away in the constellation Andromeda and was discovered by astronomer William Herschel on September 21, 1786. It is classified as a cD galaxy and is the brightest member of Abell 262. NGC 708 is a weak FR I radio galaxy and is also classified as a type 2 Seyfert galaxy.
NGC 4060 is a lenticular galaxy located 320 million light-years away in the constellation Coma Berenices. It was discovered by astronomer Albert Marth on March 18, 1865 and is a member of the NGC 4065 Group which is part of the Coma Supercluster.
NGC 4065 is an elliptical galaxy located 300 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer William Herschel on April 27, 1785. It was then rediscovered by John Herschel on April 29, 1832 and was listed as NGC 4057. NGC 4065 is the brightest member of the NGC 4065 Group.
NGC 4072 is a lenticular galaxy located 300 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer Ralph Copeland on April 3, 1872 and is a member of the NGC 4065 Group.
NGC 4074 is a peculiar lenticular galaxy located 310 million light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on April 27, 1785 and is a member of the NGC 4065 Group.
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NGC 1369 is a barred lenticular galaxy located 59 millon light years away in constellation of Eridanus. The galaxy was discovered by astronomer Julius Schmidt on January 19, 1865, and is a member of the Fornax Cluster. NGC 1369 is a host to a supermassive black hole with an estimated mass of 1.8 millon solar masses.
NGC 1428 is a peculiar galaxy of an uncertain morphology; either an elliptical or lenticular galaxy located approximately 65 million light-years away from Earth.
NGC 4324 is a lenticular galaxy located about 85 million light-years away in the constellation Virgo. It was discovered by astronomer Heinrich d'Arrest on March 4, 1862. NGC 4324 has a stellar mass of 5.62 × 1010M☉, and a baryonic mass of 5.88 × 1010M☉. The galaxy's total mass is around 5.25 × 1011M☉. NGC 4324 is notable for having a ring of star formation surrounding its nucleus. It was considered a member of the Virgo II Groups until 1999, when its distance was recalculated and it was placed in the Virgo W Group.
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