NGC 1293 explained

NGC 1293
Upright:1.15
Epoch:J2000
Type:E0[1]
Dist Ly:65.8Mpc
H Radial V:4173 km/s
Z:0.013920
Appmag V:14.50
Size V:1.0 x 1.0
Constellation Name:Perseus
Names:CGCG 540-116, MCG +07-07-075, PGC 012597
Size:~37.8kpc (estimated)

NGC 1293 is an elliptical galaxy[2] located about 215 million light-years away[3] in the constellation Perseus.[4] It was discovered by astronomer William Herschel on October 17, 1786.[5] NGC 1293 is a member of the Perseus Cluster.[6]

See also

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 1293 . 2018-07-07.
  2. Web site: Your NED Search Results. ned.ipac.caltech.edu. 2018-07-07.
  3. Web site: NED Query Results for NGC 1293. ned.ipac.caltech.edu. en-US. 2018-07-07.
  4. Web site: Revised NGC Data for NGC 1293. spider.seds.org. 2018-07-07.
  5. Web site: New General Catalog Objects: NGC 1250 - 1299. cseligman.com. en-US. 2018-06-15.
  6. Brunzendorf. J.. Meusinger. H.. October 1, 1999. The galaxy cluster Abell 426 (Perseus). A catalogue of 660 galaxy positions, isophotal magnitudes and morphological types. Astronomy and Astrophysics Supplement Series. en. 139. 1. 141–161. 10.1051/aas:1999111. 0365-0138. 1999A&AS..139..141B. free.