Key facts
- Constellation
- Lepus
- Right ascension
- 06 01 07.963
- Declination
- −23 ° 40 ′ 20.35 ″
- Redshift
- 0.006148 ± 0.000017
- Heliocentric radial velocity
- 1,836 km/s
- Galactocentric velocity
- 1,649 km/s
- Distance
- 120.6 Mly (36.98 Mpc )
- Type
- SAB(rs)cd
- Number of stars
- 9.1 × 10 M ☉
- Apparent size v
- 2.40 ′ × 1.9 ′
- Notable features
- Bulgeless
via Wikipedia infobox
~2 min read
Encyclopedic overview
NGC 2139 is a barred spiral galaxy in the constellation of Lepus. It was discovered on November 17, 1784, by the German-English astronomer William Herschel. The galaxy is located at a distance of 120.6 million light-years (36.98 Mpc) from the Sun and is receding with a radial velocity of 1,836 km/s.
The overall form of this galaxy is irregular with spiral arms and the appearance of tidal features, suggesting a potential recent merger event. There is no central bulge of significance. The morphological classification is SAB(rs)cd, which indicates a barred spiral galaxy (SAB) with a transitional inner ring structure (rs) and loosely wound spiral arms (cd). It is a star forming galaxy with a formation rate of 3.8 M☉·yr. There is a plume extending to the south of the galaxy.
Excerpted from Wikipedia’s “Q1047119” article, available under the CC BY-SA 4.0 licence.
Available in 32 languages
- Français
- Deutsch
- 中文
- Русский
- Português
- Italiano
- العربية
- Azerbaijani
- Basque
- Belarusian
- Bosnian
- Chechen
- Croatian
- Egyptian Arabic
- Esperanto
- Greek
- Kazakh
- Luxembourgish
Show 13 more
via Wikidata sitelinks · CC0