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EntityQ942187· pop 36· linked from 522 articles

Also known as Eye of Sauron

spiral galaxy in the constellation Canes Venatici

Key facts

Constellation
Canes Venatici
Right ascension
12 10 32.6
Declination
+39 ° 24 ′ 21 ″
Redshift
0.003262 , 995 ± 3 km/ s
Distance
15.8 ± 0.4 Mpc (51.5 × 10 ^ ± 1.3 × 10 ^ ly)
Type
(R') SAB (rs)ab, Sy1
Size
~54,300 ly (16.66 kpc ) (estimated)
Apparent size v
6.4 ′ × 5.5 ′

via Wikipedia infobox

Wikidata facts

Constellation
Canes Venatici
Distance from Earth
3.9
Image
NGC 4151.jpg
Show 13 more facts
declination
39.40584936870090
Commons category
NGC 4151
catalog code
Gaia DR2 1535808699355081728
galaxy morphological type
SABa
discoverer or inventor
William Herschel
time of discovery or invention
1787-03-17
apparent magnitude
10.448
right ascension
182.63573822822210
redshift
0.003262
radial velocity
976
epoch
J2000.0
right ascension component of proper motion
-1.172
declination component of proper motion
0.252
Sources (3)

via Wikidata · CC0

~3 min read

Encyclopedic overview

NGC 4151 is an intermediate spiral Seyfert galaxy with weak inner ring structure located 15.8 megaparsecs (52 million light-years) from Earth in the constellation Canes Venatici. The galaxy was first mentioned by William Herschel on March 17, 1787. It was one of the six galaxies described in Carl Seyfert's original paper which defined such systems. It is one of the nearest galaxies to Earth to contain an actively growing supermassive black hole. The black hole would have a mass on the order of 2.5 million to 30 million solar masses. It was speculated that the nucleus may host a binary black hole, with about 40 million and about 10 million solar masses respectively, orbiting with a 15.8-year period. This is, however, still a matter of active debate.

Some astronomers nickname it the "Eye of Sauron" from its appearance.

Excerpted from Wikipedia’s “Q942187” article, available under the CC BY-SA 4.0 licence.