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EntityQ1147221· pop 31· linked from 453 articles

open cluster in Aquila

Key facts

Right ascension
18 51 20. 6
Declination
+10 ° 20 ′ 0 2 ″
Distance
3,510 ly (1,075 pc )
Apparent dimensions v
13'
Radius
26 ly (tidal)
Estimated age
141 Myr
Other designations
NGC 6709, Cr 392
Constellation
Aquila

via Wikipedia infobox

Wikidata facts

Instance of
open cluster
Part of
Milky Way
Constellation
Aquila
Distance from Earth
1075
Image
NGC 6709 PanS.jpg
Show 11 more facts
epoch
J2000.0
radial velocity
-7.8
time of discovery or invention
1827-07-29
Commons category
NGC 6709
discoverer or inventor
John Frederick William Herschel
catalog code
[KPS2012] MWSC 3009
apparent magnitude
6.7
right ascension
282.8250
declination
10.3183
right ascension component of proper motion
1.17
declination component of proper motion
-3.13
Sources (1)

via Wikidata · CC0

~1 min read

Encyclopedic overview

NGC 6709 is an open cluster of stars in the equatorial constellation of Aquila, some 5° to the southwest of the star Zeta Aquilae. It is situated toward the center of the galaxy at a distance of 3,510 light-years.

This cluster has a Trumpler class of IV 2 m, and is considered moderately rich with 305 member stars. It is around 141 million years old; about the same as the Pleiades. The core radius of NGC 6709 is 2.2 ly (0.68 pc) and the tidal radius 26.4 ly (8.08 pc). It contains two Be stars and one of them is a shell star. There is one candidate red giant member.

Excerpted from Wikipedia’s “Q1147221” article, available under the CC BY-SA 4.0 licence.