NGC 359 explained

NGC 359
Epoch:J2000
Ra:[1]
Constellation Name:Cetus
Z:0.017803
H Radial V:5,337 km/s
Dist Ly:238 Mly[2]
Upright:1.35
Type:E0[3]
Appmag V:14.3g
Size V:1.10' × 0.78'
Names:UGC 00662, CGCG 384-066, MCG +00-03-066, 2MASX J01041697-0045532, 2MASXi J0104169-004555, PGC 3817.

NGC 359 is an elliptical galaxy located approximately 238 million light-years from the Solar System[2] in the constellation Cetus. It was discovered on September 2, 1864, by Albert Marth. It was described by Dreyer as "extremely faint, very small."[4]

This elliptical galaxy has an extremely long tidal tail and shell structure, seen across several deep-sky surveys, indicating a likely-recent and possibly ongoing interaction with nearby galactic neighbor NGC 364.

See also

External links

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 0359 . September 2, 2016.
  2. An object's distance from Earth can be determined using Hubble's law: v=Ho is Hubble's constant (70±5 (km/s)/Mpc). The relative uncertainty Δd/d divided by the distance is equal to the sum of the relative uncertainties of the velocity and v=Ho
  3. NGC 359. January 1, 2017.
  4. Web site: New General Catalog Objects: NGC 350 - 399. Cseligman. November 19, 2016.