Celestial hemisphere:  Southern  ·  Constellation: Capricornus (Cap)  ·  Contains:  41 Cap  ·  M 30  ·  NGC 7099  ·  The star 41Cap
M30 (The Complete Data Set for this Image is Available For Download at Remoteskies.net), Dustin Williams
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M30 (The Complete Data Set for this Image is Available For Download at Remoteskies.net)

M30 (The Complete Data Set for this Image is Available For Download at Remoteskies.net), Dustin Williams
Powered byPixInsight

M30 (The Complete Data Set for this Image is Available For Download at Remoteskies.net)

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Description

Messier 30 (also known as M30 or NGC 7099) is a globular cluster of stars in the southern constellation of Capricornus. It was discovered by the French astronomer Charles Messier in 1764, who described it as a circular nebula without a star. In the New General Catalogue, compiled during the 1880s, it was described as a "remarkable globular, bright, large, slightly oval." This cluster can be easily viewed with a pair of 10×50 binoculars, forming a patch of hazy light some 4 arcminutes wide that is slightly elongated along the east–west axis. With a larger instrument, individual stars can be resolved and the cluster will cover an angle of up to 12 arcminutes across with a compressed core one arcminute wide. It is best observed around August.

M30 is located at a distance of about 27,100 light-years from Earth, and is about 93 light-years across. The estimated age is roughly 12.93 billion years and it has a combined mass of about 160,000 times the mass of the Sun. The cluster is following a retrograde orbit through the inner galactic halo, suggesting that it was acquired from a satellite galaxy rather than forming within the Milky Way. It is currently located at a distance of about 22.2 kly (6.8 kpc) from the center of the galaxy, compared to an estimated 26 kly (8.0 kpc) for the Sun.

The M30 cluster has passed through a dynamic process called core collapse and now has a concentration of mass at its core of about a million times the Sun's mass per cubic parsec. This makes it one of the highest density regions in the Milky Way galaxy. Stars in such close proximity will experience a high rate of interactions that can create binary star systems, as well as a type of star called a blue straggler that is formed by mass transfer. A process of mass segregation may have caused the central region to gain a greater proportion of higher mass stars, creating a color gradient with increasing blueness toward the middle of the cluster. (Wikipedia)

L 20 X 30s

R 20 X 30s

G 20 X 30s

B 20 X 30s

(The Complete Data Set for this Image is Available For Download at Remoteskies.net)

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  • M30 (The Complete Data Set for this Image is Available For Download at Remoteskies.net), Dustin Williams
    Original
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    M30 (The Complete Data Set for this Image is Available For Download at Remoteskies.net), Dustin Williams
    B

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M30 (The Complete Data Set for this Image is Available For Download at Remoteskies.net), Dustin Williams