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EntityQ1107105· pop 29· linked from 275 articles

galaxy

Astronomical data · SIMBAD

Object type
AG?
Redshift
z = 0.003173895686006123
Morphology
SA
Coordinates
RA 177.6623° · Dec 55.3539°
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via SIMBAD · CDS Strasbourg

Key facts

Constellation
Ursa Major
Right ascension
11 50 38.9222
Declination
+55 ° 21 ′ 13.942 ″
Heliocentric radial velocity
955 ± 1 km/s
Distance
27.06 ± 14.19 Mly (8.297 ± 4.352 Mpc )
Group or cluster
NGC 3631 Group (LGG 241)
Type
(R')SA(rs)d?
Size
~23,600 ly (7.24 kpc ) (estimated)
Apparent size v
2.6′ × 2.6′

via Wikipedia infobox

Wikidata facts

Instance of
spiral galaxy
Constellation
Ursa Major
Distance from Earth
19.8
Image
NGC 3913 hst 09042 606.png
Show 11 more facts
catalog code
LEDA 37024
Commons category
NGC 3913
time of discovery or invention
1789-00-00
discoverer or inventor
William Herschel
apparent magnitude
12.406
redshift
0.003182
galaxy morphological type
SAcd
right ascension
177.6622000
declination
55.3538667
radial velocity
949
epoch
J2000.0
Sources (1)

via Wikidata · CC0

~2 min read

Encyclopedic overview

NGC 3913 is a spiral galaxy in the constellation of Ursa Major. Its velocity with respect to the cosmic microwave background for is 1,124±12 km/s, which corresponds to a Hubble distance of 54.1 ± 3.8 Mly (16.58 ± 1.17 Mpc). However, three non redshift measurements give a much closer distance of 27.06 ± 14.19 Mly (8.297 ± 4.352 Mpc). It was discovered by German-British astronomer William Herschel on 14 April 1785. It was also observed by Lewis Swift on 8 May 1890, which resulted in the galaxy also being listed in the Index Catalogue as IC 740.

The SIMBAD database lists NGC 3913 as an Active Galaxy Nucleus Candidate, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.

Excerpted from Wikipedia’s “Q1107105” article, available under the CC BY-SA 4.0 licence.