Astronomical data · SIMBAD
- Object type
- GiP
- Redshift
- z = 0.004503247880706773
- Morphology
- SB
- Coordinates
- RA 145.8001° · Dec 31.9287°
via SIMBAD · CDS Strasbourg
Key facts
- Constellation
- Leo
- Right ascension
- 09 43 12.0423
- Declination
- +31 ° 55 ′ 43.503 ″
- Redshift
- 0.005 132 ± 0.000 009 19
- Heliocentric radial velocity
- 1,539 ± 3 km/s
- Distance
- 45.69 ± 13.40 Mly (14.010 ± 4.107 Mpc )
- Group or cluster
- NGC 7329 group (LGG 462)
- Apparent magnitude v
- 12.9g
- Type
- SB C
- Size
- ~35,200 ly (10.78 kpc ) (estimated)
- Apparent size v
- 1.89′ × 1.30′
via Wikipedia infobox
Wikidata facts
- Distance from Earth
- 25.78
- Image
- NGC 2968 SDSS.jpg
Show 9 more facts
- redshift
- 0.00513
- catalog code
- LEDA 27800
- time of discovery or invention
- 1785-00-00
- galaxy morphological type
- SAB0
- apparent magnitude
- 8.431
- Commons category
- NGC 2968
- right ascension
- 145.80010678610760
- declination
- 31.92871071212900
- radial velocity
- 1534
Sources (1)
via Wikidata · CC0
~1 min read
Article
NGC 2968 is a barred spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 1,804±19 km/s, which corresponds to a Hubble distance of 86.8 ± 6.1 Mly (26.61 ± 1.88 Mpc). However, five non-redshift measurements give a much closer mean distance of 45.69 ± 13.40 Mly (14.010 ± 4.107 Mpc). It was discovered by German-British astronomer William Herschel on 7 December 1785.
NGC 2968 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
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via Wikidata sitelinks · CC0