NGC 298 explained

NGC 298
Upright:1.25
Epoch:J2000
Ra:[1]
Constellation Name:Cetus
Z:0.005847
H Radial V:1,753 km/s
Type:Scd
Appmag V:14.52
Size V:1.7' × 0.4'
Names:MCG -01-03-033, 2MASX J00550234-0719591, IRAS F00525-0736, 6dF J0055024-071959, PGC 3055.

NGC 298 is a spiral galaxy in the constellation Cetus. It was discovered on September 27, 1864, by Albert Marth.[2] NGC 298 is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in certain times of the year. Given its B magnitude of 14.7, NGC 298 is visible with the help of a telescope having an aperture of 20 inches (500 millimetre) or more.[3]

One supernova has been observed in NGC 298: SN 1986K (type II, mag. 16.5).[4]

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 0298 . September 2, 2016.
  2. Web site: New General Catalog Objects: NGC 250 - 299. Cseligman. October 17, 2016.
  3. Web site: NGC 298 - Spiral Galaxy TheSkyLive.com. 2020-07-23. theskylive.com.
  4. https://www.wis-tns.org/object/1986K Transient Name Server entry for SN 1986K.