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Messier 94
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Messier 94 is a spiral galaxy located in the constellation Canes Venatici that can be observed from Earth. It is notable as one of the brightest galaxies visible through telescopes and serves as an important object for astronomical study and observation.
AI-generated from the Wikipedia summary — may contain errors.
Wikidata facts
- Constellation
- Canes Venatici
- Parent body
- M94 Group
- Distance from Earth
- 5.1
- Image
- Messier 94.jpg
Show 12 more facts
- redshift
- 0.001027
- catalog code
- [NKB95] N4736
- Commons category
- Messier 94
- Commons gallery
- Messier 94
- time of discovery or invention
- 1781-03-22
- discoverer or inventor
- Pierre Méchain
- apparent magnitude
- 5.106
- galaxy morphological type
- SAB0/a
- right ascension
- 192.7214500
- declination
- 41.1201528
- radial velocity
- 300
- epoch
- J2000.0
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Encyclopedic overview
Messier 94 (also known as NGC 4736, Cat's Eye Galaxy, Crocodile Eye Galaxy, or Croc's Eye Galaxy) is a spiral galaxy in the mid-northern constellation Canes Venatici. It was discovered by Pierre Méchain in 1781, and catalogued by Charles Messier two days later. Although some references describe M94 as a barred spiral galaxy, the "bar" structure appears to be more oval-shaped. The galaxy has two ring structures.
Structure
Excerpted from Wikipedia’s “Messier 94” article, available under the CC BY-SA 4.0 licence.