Observation data Epoch J2000.0 Equinox ICRS | |
---|---|
Constellation | Perseus [1] |
NGC 1276 | |
Right ascension | 03h 19m 51.2s [1] |
Declination | 41° 38′ 29″ [1] |
Apparent magnitude (V) | {{{appmag_v1}}} |
Pul -3 270349 | |
Right ascension | 03h 19m 50.5421584698s [2] |
Declination | 41° 38′ 31.367763313″ [2] |
Apparent magnitude (V) | {{{appmag_v2}}} |
Pul -3 270357 | |
Right ascension | 03h 19m 51.8974508403s [3] |
Declination | 41° 38′ 29.364043732″ [3] |
Apparent magnitude (V) | {{{appmag_v3}}} |
Astrometry | |
Pul -3 270349 | |
Proper motion (μ) | RA: 0.576 [2] mas/yr Dec.: -3.787 [2] mas/yr |
Parallax (π) | 0.8814 [2] ± 0.0323 [2] mas |
Distance | 1,134.5587 parsecs (3,700.436 ly) [2] ly |
Pul -3 270357 | |
Proper motion (μ) | RA: 2.389 [3] mas/yr Dec.: -4.469 [3] mas/yr |
Parallax (π) | 0.5635 [3] ± 0.0338 [3] mas |
Distance | 1,774.6229 parsecs (5,788.046 ly) [3] ly |
Characteristics | |
Apparent magnitude (B) | 15.6 (Pul -3 270349)/15.5 (Pul -3 270357) [4] |
Apparent magnitude (R [4] ) | 14.8 (Pul -3 270349) [4] /14.7 (Pul -3 270357) [4] |
Details | |
Pul -3 270349 | |
Radius | 1.09 [5] R☉ |
Luminosity | 0.838 [5] L☉ |
Temperature | 5299.00 [5] K |
Pul -3 270357 | |
Radius | 1.48 [5] R☉ |
Luminosity | 1.964 [5] L☉ |
Temperature | 5614.53 [5] K |
Other designations | |
Pul -3 270349: WISEA J031950.54+413831.4, 2MASS J03195054+4138313, GALEXASC J031950.58+413831.6, GALEXMSC J031950.52+413831.0, SSTSL2 J031950.52+413831.3, TIC 178110482, Gaia DR2 239424674200835712 [2] [6] | |
Pul -3 270357: WISEA J031951.89+413829.3, 2MASS J03195190+4138293, GALEXASC J031951.93+413829.8, GALEXMSC J031951.88+413829.5, SSTSL2 J031951.88+413829.3, TIC 178110483, Gaia DR2 239424669903392256 [3] [7] | |
Database references | |
SIMBAD | data |
Pul -3 270349 | |
Pul -3 270357 |
NGC 1276 is an optical [2] [3] double star system [1] [8] [9] [10] located in the constellation Perseus. [1] [8] [10] The system was discovered by astronomer John Dreyer [1] [10] [11] on December 12, 1876. [1] [11] The pair consists of two 15th magnitude stars [1] [4] known as Pul -3 270349 and Pul -3 270357 that are unrelated as they lie at different distances from each other. [4] [2] [3] Pul -3 270349 lies at a distance of 1,134.5587 parsecs (3,700.436 ly ) [2] and Pul -3 270357 lies at a distance of 1,774.6229 parsecs (5,788.046 ly ). [3]
The two stars are about the same size and luminosity as the Sun. [5]
NGC 4309 is a lenticular galaxy located about 55 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer Christian Peters in 1881 and is a member of the Virgo Cluster.
NGC 4500 is a barred spiral galaxy in the constellation Ursa Major. The galaxy was discovered on April 17, 1789 by William Herschel. It is a blue compact galaxy.
NGC 4492 is a spiral galaxy located about 90 million light-years away in the constellation Virgo. NGC 4492 was discovered by astronomer William Herschel on December 28, 1785. It was rediscovered by astronomer Arnold Schwassmann on January 23, 1900 and was listed as IC 3438. NGC 4492 lies in the direction of the Virgo Cluster. However, it is not considered to be a member of that cluster.
NGC 4598 is a barred lenticular galaxy located in the constellation Virgo. NGC 4598 was discovered by astronomer William Herschel on April 15, 1784.
NGC 3309 is a giant elliptical galaxy located about 200 million light-years away in the constellation Hydra. NGC 3309 was discovered by astronomer John Herschel on March 24, 1835. The galaxy forms a pair with NGC 3311 which lies about 72,000 ly (22 kpc) away. Both galaxies dominate the center of the Hydra Cluster.
NGC 6047 is an elliptical galaxy located about 430 million light-years away in the constellation Hercules. It was discovered by astronomer Lewis Swift on June 27, 1886. NGC 6047 is a member of the Hercules Cluster.
NGC 679 is an elliptical or a lenticular galaxy located 210 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 13, 1784 and is a member of Abell 262.
NGC 704 is a lenticular galaxy located 220 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 21, 1786 and is also a member of Abell 262.
NGC 705 is a lenticular galaxy located 240 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 21, 1786 and is also a member of Abell 262.
NGC 7199 is a barred spiral galaxy registered in the New General Catalogue. It is located in the direction of the Indus constellation. It was discovered by the English astronomer John Herschel in 1835 using a 47.5 cm reflector.
NGC 759 is an elliptical galaxy located 230 million light-years away in the constellation Andromeda. NGC 759 was discovered by astronomer by Heinrich d'Arrest on September 17, 1865. It is a member of Abell 262.
NGC 918 is a barred spiral galaxy in the constellation Aries about 67 million light years from the Milky Way. It was discovered by John Herschel on Jan 11, 1831.
NGC 970 is an interacting galaxy pair in the constellation Triangulum. It is estimated to be 471 million light-years from the Milky Way and has a diameter of approximately 100,000 ly. The object was discovered on September 14, 1850 by Bindon Blood Stoney.
NGC 913 is a lenticular galaxy located in the constellation Andromeda about 224 million light years from the Milky Way. It was discovered by French astronomer Édouard Stephan in 1878.
NGC 998 is a spiral galaxy in the constellation Cetus. It is estimated to be 294 million light years from the Milky Way and has a diameter of approximately 90,000 ly. Together with NGC 997, it forms a gravitationally bound pair of galaxies. NGC 998 was discovered by astronomer Albert Marth on 10 November 1863 using a 48-inch telescope.
NGC 991 is an intermediate spiral galaxy the constellation Cetus. This galaxy was discovered by astronomer William Herschel in 1785.
NGC 734 is a lenticular galaxy with a central bar in the constellation Cetus, which is about 538 million light years from the Milky Way. It was discovered on November 9, 1885 by the American astronomer Francis Preserved Leavenworth.
NGC 721 is a barred spiral galaxy located in the constellation Andromeda about 250 million light years from the Milky Way. It was discovered by the Prussian astronomer Heinrich d'Arrest in 1862.
NGC 713 is a spiral galaxy located in the constellation of Cetus about 234 million light years from the Milky Way. It was discovered by the American astronomer Francis Leavenworth in 1886.
NGC 3925 is a barred lenticular galaxy and a ring galaxy located about 370 million light-years away in the constellation Leo. It was discovered by astronomer Heinrich d'Arrest on February 19, 1863.