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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

Wikidata facts

Instance of
spiral galaxy
Constellation
Virgo
Distance from Earth
10.5
Image
NGC 4504 hst 09042 R814B450.png
Show 13 more facts
catalog code
Gaia DR2 3580325595969515776
galaxy morphological type
Sc
Commons category
NGC 4504
discoverer or inventor
William Herschel
time of discovery or invention
1789-03-20
apparent magnitude
9.498
right ascension
188.07260116347470
declination
-7.56359512891930
redshift
0.003336
radial velocity
809
epoch
J2000.0
right ascension component of proper motion
-2.852
declination component of proper motion
2.798

via Wikidata · CC0

~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.