Celestial hemisphere:  Southern  ·  Constellation: Capricornus (Cap)  ·  Contains:  M 30  ·  NGC 7099
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Globular Cluster, M 30 (NGC 7099), Paul Lloyd
Globular Cluster, M 30 (NGC 7099)
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Globular Cluster, M 30 (NGC 7099)

Getting plate-solving status, please wait...
Globular Cluster, M 30 (NGC 7099), Paul Lloyd
Globular Cluster, M 30 (NGC 7099)
Powered byPixInsight

Globular Cluster, M 30 (NGC 7099)

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Description

M 30 was first discovered by Charles Messier in 1764 and became the 30th entry in his catalogue of
comet-like objects. It can be seen as a hazy patch in good binoculars in the south-east corner of the
constellation, Capricornus. Larger apertures are needed to resolve stars. It lies approx. 27,000 ly away
and has been measured at 93 ly in diameter. Its age has been determined at 12.9  Gy (billion years).

The central core of this cluster is believed to be one of the most concentrated in our galaxy. Also, the
orbital rotation of this cluster around our galaxy's centre is retrograde, i.e. opposite to most other parts
of our galaxy. This has led astronomers to speculate that it was captured from a satelite galaxy, rather
than being generated from within our Milky Way.


Telescope: William Optics FLT110 refractor + 2.0x Barlow, f=1540mm
Camera:    ZWO ASI294MC Pro, 34 x 300 sec, no filter
                   Bortle 3-4 sky, moonless
Field of View: approx. 0º 30’ x 0º 20’
Image processed and prepared in PixInsight and Photoshop Elements

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Globular Cluster, M 30 (NGC 7099), Paul Lloyd