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NGC 1261

Globular cluster · C87 · NGC 1261

NGC 1261

Globular cluster in Horologium

Photo: Lithopsian · CC BY-SA 4.0 · Wikimedia Commons

NGC 1261 is a globular cluster of stars in the southern constellation of Horologium, first discovered by Scottish astronomer James Dunlop in 1826. The cluster is located at a distance of 53 kilolight-years from the Sun, and 59 kilolight-years from the Galactic Center. It is about 10.24 billion years old with 341,000 times the mass of the Sun. The cluster does not display the normal indications of core collapse, but evidence suggests it may have instead passed through a post core-collapse bounce state within the past two billion years. The central luminosity density is 2.22 L☉·pc−3, which is low for a globular cluster. Despite this, it has a Shapley–Sawyer Concentration Class of II, indicating a dense central concentration.

Description from Wikipedia (CC BY-SA 4.0).

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Key facts

Distance

~55,500 light-years

Apparent mag.

+8.4

Apparent size

5.1′

Best seen with

Binoculars

Catalogue

C87 · NGC 1261

Did you know

In HorologiumRead more on Wikipedia

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