File:NGC_3368_ESO.jpg · Wikimedia Commons · See Wikimedia Commons
AI overview
Messier 96 is a spiral galaxy located about 35 million light-years away in the constellation Leo. It's notable as one of the brighter galaxies visible through telescopes and serves as an important object for astronomers studying galaxy structure and evolution.
AI-generated from the Wikipedia summary — may contain errors.
Key facts
- Constellation
- Leo
- Right ascension
- 10 46 45.6847
- Declination
- +11 ° 49 ′ 12.003 ″
- Redshift
- 0.002 962 ± 0.000 002
- Heliocentric radial velocity
- 888 ± 1 km/s
- Distance
- 31 ± 3 Mly (9.6 ± 1.0 Mpc )
- Type
- SAB(rs)ab
- Size
- ~78,000 ly (23.93 kpc ) (estimated)
- Apparent size v
- 7.6′ × 5.2′
via Wikipedia infobox
Wikidata facts
- Instance of
- galaxy group
- Constellation
- Leo
- Distance from Earth
- 14
- Radius
- 50000
- Image
- Taking a third look (potw2534a).jpg
Show 13 more facts
- galaxy morphological type
- SBa
- Commons category
- Messier 96
- catalog code
- LEDA 32192
- Commons gallery
- Messier 96
- time of discovery or invention
- 1781-03-20
- discoverer or inventor
- Pierre Méchain
- apparent magnitude
- 6.320
- redshift
- 0.002992
- absolute magnitude
- -21.1
- right ascension
- 161.6906000
- declination
- 11.8199389
- radial velocity
- 902
- epoch
- J2000.0
via Wikidata · CC0
~3 min read
Encyclopedic overview
Messier 96 (also known as M96 or NGC 3368) is an intermediate spiral galaxy about 31 million light-years away in the constellation Leo.
Observational history and appearance
Excerpted from Wikipedia’s “Messier 96” article, available under the CC BY-SA 4.0 licence.