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EntityQ764081· pop 33· linked from 495 articles

galaxy

Key facts

Constellation
Coma Berenices
Right ascension
12 49 38.958
Declination
+15 ° 09 ′ 55.76 ″
Redshift
0.00397 ± 0.00011
Heliocentric radial velocity
1,129 km/s
Distance
54.5 ± 3.6 Mly (16.7 ± 1.1 Mpc )
Type
S0a-S0/Sa
Apparent size v
3.0′ × 0.8′

via Wikipedia infobox

Wikidata facts

Distance from Earth
19.43
Image
NGC 4710 Hubble.jpg
Show 9 more facts
redshift
0.003753
Commons category
NGC 4710
catalog code
LEDA 43375
time of discovery or invention
1784-03-21
apparent magnitude
7.567
right ascension
192.412325
declination
15.1654889
radial velocity
1125
galaxy morphological type
S0a-S0/Sa
Sources (1)

via Wikidata · CC0

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Article

NGC 4710 is an edge-on lenticular galaxy in the northern constellation of Coma Berenices. It was discovered on March 21, 1784 by German-British astronomer William Herschel. This galaxy has a B-band visual magnitude of 11.60 and an angular size of 3.0′ × 0.8′. It is located at a distance of 54.5 ± 3.6 million light-years (16.7 ± 1.1 Mpc) from the Milky Way, and is receding with a heliocentric radial velocity of 1,129 km/s. This is a member of the Virgo Cluster, with a projected offset of ~6° from the cluster center and a cluster crossing time of around two billion years.

The morphological classification of NGC 4710 is S0 or SA(r)0, which indicates this is an unbarred lenticular galaxy (SA) with an inner ring structure (r). It is inclined at an angle of 86° to the plane of the sky, with the major axis aligned along a position angle of 207°. NGC 4710 has a relatively high gas abundance with a dusty nucleus. The stellar velocity distribution is characteristic of galaxies with a small bulge. Like the Milky Way, it has an X-shaped bulge which is a probable bar structure; hence it is likely a barred lenticular. The star formation rate is 0.11±0.02 M☉·yr. NGC 4710 possesses both thin and thick discs.

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