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EntityQ1120021· pop 32· linked from 478 articles

globular cluster

Key facts

Class
XII
Constellation
Boötes
Right ascension
14 05 27.29
Declination
+28 ° 32 ′ 04.0 ″
Distance
52.2 ± 1.3 kly (16.0 ± 0.4 kpc )
Apparent dimensions v
9.0′
Absolute magnitude
−6.98
Mass
1.79 × 10 M ☉
Tidal radius
238.0 ly (72.98 pc)
Metallicity
[ Fe/H ] = –1.95 ± 0.02 dex
Estimated age
12.15 ± 0.11 Gyr
Notable features
Tidal stream
Other designations
NGC 5466, C 1403+287, GCl 27, GC 3776, h 1746, H 6

via Wikipedia infobox

Wikidata facts

Instance of
globular cluster
Part of
Milky Way
Constellation
Boötes
Distance from Earth
52192
Image
NGC 5466 Hubble WikiSky.jpg
Show 13 more facts
epoch
J2000.0
discoverer or inventor
William Herschel
Commons category
NGC 5466
catalog code
[KPS2012] MWSC 2198
time of discovery or invention
1784-05-17
right ascension component of proper motion
-3.55
apparent magnitude
9.413
radial velocity
107.7
absolute magnitude
-6.98
metallicity
-2.31
right ascension
211.363708
declination
28.534444
declination component of proper motion
-1.97
Sources (2)

via Wikidata · CC0

~4 min read

Encyclopedic overview

NGC 5466 is a globular cluster of stars in the constellation Boötes. It was discovered by German-British astronomer William Herschel on May 17, 1784, and catalogued as H VI.9. This large, dim cluster has an apparent visual magnitude of 9.2 and spans an angular size of 9.0′. It is relatively distant from the Sun, about 52 thousand light-years (16.0 kpc) away, and 53 thousand light-years (16.3 kpc) from the Galactic Center.

Observations

Excerpted from Wikipedia’s “Q1120021” article, available under the CC BY-SA 4.0 licence.