Astronomical data · SIMBAD
- Object type
- Sy1
- Distance
- 1,229 light-years
- Redshift
- z = 0.0032776351913594848
- Morphology
- SA_B
- Coordinates
- RA 190.7182° · Dec 13.2574°
via SIMBAD · CDS Strasbourg
Key facts
- Constellation
- Virgo
- Right ascension
- 12 42 52.37814
- Declination
- +13 ° 15 ′ 26.7129 ″
- Heliocentric radial velocity
- 989 km/s
- Distance
- 72.02 ± 0.23 Mly (22.08 ± 0.07 Mpc )
- Group or cluster
- Virgo Cluster
- Type
- SAB(rs)bc
- Apparent size v
- 2′.8 × 1′.9
- Notable features
- Seyfert type 1
via Wikipedia infobox
Wikidata facts
- Distance from Earth
- 20
- Image
- NGC 4639.jpg
Show 9 more facts
- catalog code
- LEDA 42741
- Commons category
- NGC 4639
- time of discovery or invention
- 1784-04-12
- apparent magnitude
- 8.805
- galaxy morphological type
- Sb
- right ascension
- 190.71824224840790
- declination
- 13.25742025813510
- radial velocity
- 1089
- redshift
- 0.00364
Sources (1)
via Wikidata · CC0
~2 min read
Article
NGC 4639 is a barred spiral galaxy located in the equatorial constellation of Virgo. It was discovered by German-born astronomer William Herschel on 12 April 1784. John L. E. Dreyer described it as "pretty bright, small, extended, mottled but not resolved, 12th magnitude star 1 arcmin to southeast". This is a relatively nearby galaxy, lying approximately 72 million light-years away from the Milky Way. It is a companion to NGC 4654, and the two appear to have interacted roughly 500 million years ago. NGC 4639 is a member of the Virgo Cluster.
The morphological classification of this galaxy is SAB(rs)bc, indicating a spiral galaxy with a weak bar (SAB), an incomplete ring around the bar (rs), and moderate to loosely-wound spiral arms (bc). NGC 4639 has a mildly active galactic nucleus of the Seyfert type 1; one of the weakest known. The compact central source has been detected by its X-ray emission, and is variable on timescales of months to years. There is a supermassive black hole at the core with an estimated mass of 7.9×10 M☉.
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via Wikidata sitelinks · CC0