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EntityQ1112098· pop 29· linked from 656 articles

galaxy

Astronomical data · SIMBAD

Object type
EmG
Redshift
z = 0.003318129992532004
Morphology
Sa-Sc
Coordinates
RA 188.0726° · Dec -7.5636°
View on SIMBAD →

via SIMBAD · CDS Strasbourg

Key facts

Constellation
Virgo
Right ascension
12 32 17.4095
Declination
−07 ° 33 ′ 48.897 ″
Redshift
0.003329 ± 0.000002
Heliocentric radial velocity
998 ± 1 km/ s
Distance
55.6 ± 16.9 Mly (17.1 ± 5.2 Mpc )
Group or cluster
Virgo II Groups
Type
SA(s)cd
Size
~71,000 ly (21.7 kpc ) (estimated)
Apparent size v
4.4 ′ × 2.7 ′

via Wikipedia infobox

~1 min read

Encyclopedic overview

NGC 4504 is a spiral galaxy in the constellation Virgo. The galaxy lies about 55 million light years away from Earth, which means, given its apparent dimensions, that NGC 4504 is approximately 70,000 light years across. It was discovered by William Herschel on March 20, 1789.

NGC 4504 has a point source nucleus embedded in a highly elliptical bulge. It is possible there is a small bar in the bulge. The galaxy has very low surface brightness arms emerging from the bulge. HII regions are visible in the disk, the largest of which are more than 3 arcseconds across. The star formation rate is estimated to be 0.45 M☉ per year based on the H-alpha emission. The galaxy has a small bar 0.36 arcminutes long and a ring with a diameter 0.93 arcminutes. In the nucleus of the galaxy lies a nuclear star cluster which has a radius of 4 arcseconds.

Excerpted from Wikipedia’s “Q1112098” article, available under the CC BY-SA 4.0 licence.