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EntityQ745029· pop 36· linked from 437 articles

globular cluster in the constellation Delphinus

Key facts

Class
VIII
Constellation
Delphinus
Right ascension
20 34 11.37
Declination
+07 ° 24 ′ 16.1 ″
Distance
52 kly (16 kpc )
Apparent dimensions v
1.20 ′
Absolute magnitude
−7.65
Mass
2.95 × 10 M ☉
Metallicity
[ Fe/H ] = –1.47 dex
Other designations
Caldwell 47, NGC 6934

via Wikipedia infobox

Wikidata facts

Instance of
globular cluster
Part of
Milky Way
Constellation
Delphinus
Distance from Earth
0.016
Image
NGC 6934 Hubble WikiSky.jpg
Show 11 more facts
catalog code
[KPS2012] MWSC 3369
Commons category
NGC 6934
discoverer or inventor
William Herschel
time of discovery or invention
1785-09-24
apparent magnitude
8.572
right ascension
308.547375
declination
7.404472
epoch
J2000.0
radial velocity
-411.4
right ascension component of proper motion
-2.93
declination component of proper motion
-4.20
Sources (1)

via Wikidata · CC0

~1 min read

Encyclopedic overview

NGC 6934 (also known as Caldwell 47) is a globular cluster of stars in the northern constellation of Delphinus, about 52 kilolight-years distant from the Sun. It was discovered by the German-born astronomer William Herschel on 24 September 1785. The cluster is following a highly eccentric orbit (with an eccentricity of 0.81) through the Milky Way along an orbital plane that is inclined by 73° to the galactic plane. It may share a common dynamic origin with NGC 5466. As of 2018, it has been poorly studied.

This appears to be a Oosterhoff type I cluster with an intermediate metallicity. It has an Shapley–Sawyer Concentration Class of VIII, with a core radius of 15″ and a half-light radius of 36″. The estimated mass is 295,000 times the mass of the Sun. The cluster displays photometric anomalies, with a split subgiant branch on the HR diagram. Searches for variable stars have discovered 85 in the cluster field, of which 79 are of the RR Lyrae class and one is a SX Phe variable. There is some evidence for a tidal tail.

Excerpted from Wikipedia’s “NGC 6934” article, available under the CC BY-SA 4.0 licence.