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Q942160

File:NGC514_-_SDSS_DR14.jpg · Wikimedia Commons · See Wikimedia Commons

EntityQ942160· pop 40· linked from 892 articles

galaxy

Key facts

Constellation
Pisces
Right ascension
01 24 03.89603
Declination
+12 ° 55 ′ 02.8476 ″
Redshift
0.008246 ± 0.000010
Heliocentric radial velocity
2,472 km/s
Distance
82.8 Mly (25.4 Mpc )
Type
SAB(rs)c
Apparent size v
3.5 ′ × 2.8 ′

via Wikipedia infobox

Wikidata facts

Constellation
Pisces
Distance from Earth
23
Image
NGC514 - SDSS DR14.jpg
Show 13 more facts
discoverer or inventor
William Herschel
Commons category
NGC 514
galaxy morphological type
SAB(rs)c
catalog code
LEDA 5139
time of discovery or invention
1784-10-16
apparent magnitude
9.144
redshift
0.008246
right ascension
21.01623346583410
declination
12.91745767885910
radial velocity
2541
epoch
J2000.0
right ascension component of proper motion
0.182
declination component of proper motion
-0.476
Sources (2)

via Wikidata · CC0

~1 min read

Encyclopedic overview

NGC 514 is a low-luminosity, intermediate spiral galaxy in the equatorial constellation of Pisces, located at a distance of approximately 83 million light-years from the Milky Way. It was discovered on 16 October 1784 by astronomer William Herschel. The general form of the galaxy is specified by its morphological classification of SAB(rs)c, which indicates it has a weak bar system at the core (SAB), an incomplete ring formation around the bar (rs), and somewhat loosely-wound spiral arms (c). This galaxy has an H II nucleus with an extended region that displays weak emission lines in the optical range, but not in the near infrared. The suspected supermassive black hole at the core has an estimated mass of 3.2×10 M☉.

Supernova

Excerpted from Wikipedia’s “Q942160” article, available under the CC BY-SA 4.0 licence.