Messier 92 (also known M 92, or NGC 6341) (Boris US5WU)

Celestial hemisphere: Northern · Constellation: Hercules (Her) · Contains: M 92 · NGC 6341 · PGC 2208131 · PGC 2212174 · PGC 2220230 · PGC 2220717 · PGC 59931 · PGC 59938 · PGC 59984

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Messier 92 (also known M 92, or NGC 6341)

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Messier 92 (also known M 92, or NGC 6341)

Messier 92 (also known M 92, or NGC 6341) is a globular cluster of stars in the northern constellation of Hercules. It was discovered by Johann Elert Bode in 1777, then published in the Jahrbuch during 1779. It was inadvertently rediscovered by Charles Messier in 1781 and added as the 92nd entry in his catalogue. It is about 26,700 light-years away from the Solar System. It is one of the brighter of its sort in apparent magnitude in the northern hemisphere and in its absolute magnitude in the galaxy, but it is often overlooked by amateur astronomers due to angular proximity to bright cluster Messier 13, about 20% closer. It is visible to the naked eye under very good conditions.

This image taken in September 2021.

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Schmidt-Cassegrain Telescope (SCT) Imagers

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	Distinct awarded users	Total awarded images
Image of the day
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	Image of the day	Top pick	Top pick nominations	Total submitted
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Other
Unknown

The “AstroBin Image of the Day and Top Picks”, or IOTD/TP, is a long-running system to promote beautiful, interesting, peculiar, or otherwise amazing astrophotographs, with a focus on technical excellence. Learn more.

Submitted The date and time when you submitted this image for IOTD/TP consideration.	...
Views by Submitters (available since September 19th, 2023) Every image is assigned to 50% of available Submitters. In the event that at least 80% of them don't view the image before its time in the IOTD/TP process expires, it's assigned to the other 50% of Submitters and the process begins anew.
Promotions by Submitters When 3 distinct Submitters promote the image, it moves on to the next stage of the process: evaluation for Top Pick status. This requirement, in addition to anonymization of images and distribution to only a subset of them, prevents biases and ensures that the best images are selected.
Promotions by Reviewers When 3 distinct Reviewers promote the image, it moves on to the next stage of the process: evaluation for IOTD status.
Early dismissal Staff members have a lot of images to inspect on a daily basis, and they can dismiss images if they believe they don't meet the requirements for IOTD/TP selection. If an image is dismissed 5 times, it's removed from the process. This streamlines the process and ensures that any bias present in promotions could be overruled by other staff members.

Status	Advanced success
Started	...
Astrometry.net job	5699533
PixInsight job	C1ERPN43URGL01KN809AMZ4ZLUQT1OT5
PixInsight queue size	n/a
PixInsight stage	TASK_LOG

RA (center)	17h17m05s.52
RA (top/left)	17h19m07s.30
RA (top/right)	17h14m55s.93
RA (bottom/right)	17h15m03s.93
RA (bottom/left)	17h19m12s.44

Dec (center)	+43°08′11″.8
Dec (top/left)	+43°27′06″.7
Dec (top/right)	+43°25′40″.5
Dec (bottom/right)	+42°49′07″.6
Dec (bottom/left)	+42°50′41″.3

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Messier 92 (also known M 92, or NGC 6341)

Messier 92 (also known M 92, or NGC 6341)

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Image Index:

Contribution Index (beta):

Messier 92 (also known M 92, or NGC 6341)

Messier 92 (also known M 92, or NGC 6341)

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Description

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In these public groups

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