
NGC 4395 · galaxy
NGC 4395
NGC 4395 is a nearby low surface brightness spiral galaxy located about 14 million light-years from Earth in the constellation Canes Venatici.
RA12h 25m 48sDec+33° 32' 48"
Identity & coordinates
Identification
- Primary designation
- NGC 4395
- All designations
- NGC 4395
- Object type
- Galaxy
- Constellation
- Canes Venatici
- Best viewing
- Spring
Coordinates & physical
- Right ascension (J2000)
- 12h 25m 48s
- Declination (J2000)
- +33° 32' 48"
- Apparent magnitude (V)
- —
- Distance
- —
- Redshift (z)
- 0.001064
Visibility tonight
The science
NGC 4395 is a nearby low surface brightness spiral galaxy located about 14 million light-years from Earth in the constellation Canes Venatici. It was discovered by German-British astronomer William Herschel on 2 January 1786. The nucleus of NGC 4395 is active and the galaxy is classified as a Seyfert Type I, known for its very low-mass supermassive black hole.
Summary adapted from Wikipedia · CC-BY-SA-4.0
References
- SIMBAD Not resolved
- NED Fetched May 8, 2026 View in NED ↗
- Wikipedia Fetched May 8, 2026 Read full article ↗
Wikipedia title resolved via id — the catalog designation was a Wikipedia article title directly.
1 merge conflict resolved
- coordinates: SIMBAD missing → NED used



