NGC 1351 explained

NGC 1351
Epoch:J2000
Type:E-S0
Dist Ly:20.8 Mpc (67.8 Mly)
Z:0.00507
Appmag V:11.46
Size V:2.2 × 3.4
Constellation Name:Fornax
Names:ESO 358-12, PGC 13028, FCC 83, MCG -6-8-22
Absmag V:-20.07

NGC 1351 is a lenticular galaxy[1] in the constellation Fornax. It has a redshift of z=0.00505,[2] [3] and its distance from Earth can be estimated as 21 million parsecs (68 million light-years). It is elongated in shape, and was discovered by William Herschel on October 19, 1835.

The diameter of the galaxy is about 33 kpc, which makes it a medium-size galaxy, and smaller than the Milky Way. It is a member of the Fornax Cluster, a cluster of approximately 200 galaxies. The galaxy possesses a bright nucleus at its center.

It is currently receding from the solar system at a velocity of 1514 km/s, and 1410 km/s from the cosmic microwave background.

See also

Notes and References

  1. Web site: NGC 1351 - Elliptical/Spiral Galaxy in Fornax TheSkyLive.com . 2024-07-17 . theskylive.com.
  2. Web site: Astronomy . Go . NGC 1351 galaxy in Fornax New General Catalogue . 2024-07-17 . Go-Astronomy.com . en-US.
  3. Web site: By Name NASA/IPAC Extragalactic Database . 2024-07-17 . ned.ipac.caltech.edu.