Astronomical data · SIMBAD
- Object type
- GiG
- Redshift
- z = 0.02401
- Morphology
- S0a
- Coordinates
- RA 49.9961° · Dec 41.4796°
View on SIMBAD →
via SIMBAD · CDS Strasbourg
Key facts
- Constellation
- Perseus
- Right ascension
- 3 19 59.1
- Declination
- 41 ° 28 ′ 46 ″
- Heliocentric radial velocity
- 7285 km/s
- Distance
- 317 Mly (97.1 Mpc )
- Group or cluster
- Perseus Cluster
- Type
- S/S0?
- Size
- ~113,400 ly (34.77 kpc ) (estimated)
- Apparent size v
- 0.587 x 0.329
via Wikipedia infobox
~1 min read
Encyclopedic overview
NGC 1279 is a lenticular galaxy estimated to be 324 million light-years away from the Milky Way in the constellation Perseus. It has diameter of about 110,000 ly, and is a member of the Perseus Cluster.
It was discovered on December 12, 1876, by astronomer John Louis Emil Dreyer.
Excerpted from Wikipedia’s “Q571080” article, available under the CC BY-SA 4.0 licence.