NGC 665 explained

NGC 665
Epoch:J2000
Constellation Name:Pisces
Z:0.018079±0.000103
Dist Ly:236 Mly (72.3 Mpc)
Appmag V:12.2
Type:(R)S0^0
Size:100,000 ly
Size V:1.8 x 1.0
Notes:Small halo of gas visible at galactic center
Names:UGC 1223, PGC 6415, MCG+02-05-019

NGC 665 is a Lenticular galaxy 236 million light-years away in the constellation Pisces.[1] NGC 665 was discovered in 1786 by William Herschel, and is 100,000 light-years across. In the center of NGC 665, a small halo of dust and gas can be seen, indicating some small star-forming regions. NGC 665 is not known to have an active galactic nuclei, as seen in the SDSS image.[2]

Nearby and satellite galaxies

Like other galaxies, NGC 665 has a satellite galaxy (MCG 02-05-022),[3] a dwarf elliptical galaxy, as seen in the SDSS image of NGC 665. Its nearby cluster of stars is NGC 663.

Notes and References

  1. Web site: By Name NASA/IPAC Extragalactic Database . 2023-11-29 . ned.ipac.caltech.edu.
  2. Web site: NGC 665 - Lenticular Galaxy in Pisces TheSkyLive.com . 2023-11-29 . theskylive.com.
  3. Web site: NGC 665 - Galaxy - WIKISKY . 2023-11-29 . server6.wikisky.org.