Bulgeless Galaxy Hides Black Hole

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"

Image: NASA/JPL-Caltech. Source: JPL via images.nasa.gov.

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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
III

Visibility tonight

V

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

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References

Wikipedia title resolved via id — the catalog designation was a Wikipedia article title directly.

1 merge conflict resolved
  • coordinates: SIMBAD missing → NED used