File:Messier_26.jpg · Wikimedia Commons · See Wikimedia Commons
Messier 26 is a group of stars that are gravitationally bound together and located relatively close to each other in space, known as an open cluster. Astronomers study objects like this to better understand how stars form and evolve together over time.
AI-generated from the Wikipedia summary — may contain errors.
Wikidata facts
- Distance from Earth
- 1582
- Radius
- 22
- Image
- NGC 6694 PanS.jpg
Show 11 more facts
- Commons category
- Messier 26
- catalog code
- [KPS2012] MWSC 2987
- declination
- -9.3833
- time of discovery or invention
- 1764-07-20
- Commons gallery
- Messier 26
- apparent magnitude
- 8.0
- spectral class
- II
- right ascension
- 281.3250
- radial velocity
- 4.0
- right ascension component of proper motion
- -3.04
- declination component of proper motion
- -2.07
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via Wikidata · CC0
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Article
Messier 26, also known as NGC 6694, is an open cluster of stars in the southern constellation of Scutum. It was discovered by Charles Messier in 1764. This 8th magnitude cluster is a challenge to find in ideal skies with typical binoculars, where it can be, with any modern minimum 3-inch (76 mm) aperture device. It is south-southwest of the open cluster Messier 11 and is 14′ across. About 25 stars are visible in a telescope with a 150–200 mm (6–8 in) aperture.
M26 spans a linear size of 22 light years across with a tidal radius of 25 light-years, and is at a distance of 5,160 light years from the Earth. The brightest star is of magnitude 11 and the age of this cluster has been calculated to be 85.3 million years. It includes one known spectroscopic binary system.