M106 (Almos Balasi)

Celestial hemisphere: Northern · Constellation: Canes Venatici (CVn) · Contains: M 106 · NGC 4248 · NGC 4258

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M106

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M106

Messier 106 (also known as NGC 4258) is an intermediate spiral galaxy in the constellation Canes Venatici. It was discovered by Pierre Méchain in 1781. M106 is at a distance of about 22 to 25 million light-years away from Earth. M106 contains an active nucleus classified as a Type 2 Seyfert, and the presence of a central supermassive black hole has been demonstrated from radio-wavelength observations of the rotation of a disk of molecular gas orbiting within the inner light-year around the black hole. A Type II supernova was observed in M106 in May 2014.

Original
B
C
D
Final
E

B

Description: More color on the galaxy core

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C

Description: More details, slightly darker background

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D

Description: More details

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E

Description: Reprocessed with less contrast

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Schmidt-Cassegrain Telescope (SCT) Imagers
N.I.N.A. Users
ZWO ASIAIR PRO USERS
The OSC Club (One Shot Camera)
ASI 071 mcc

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Distribution of astrophotographers

This table shows the number of distinct astrophotographers who have been assigned and IOTD/TP award compared to the total number of images awarded.
	Distinct awarded users	Total awarded images
Image of the day
Top picks
Top pick nominations

Distribution of subject types

This table shows the distribution of awards per subject type, compared to the popularity of images of that subject type.
	Image of the day	Top pick	Top pick nominations	Total submitted
Deep sky
Solar system
Extremely wide field
Star trails
Northern lights
Noctilucent clouds
Landscape

Distribution of data sources

This table shows the distribution of awards per data source, compared to the popularity of images acquired from that data source.
	Image of the day	Top pick	Top pick nominations	Total submitted
Backyard
Traveller
Own remote observatory
Amateur hosting facility
Public amaeteur data
Professional, scientific grade data
Mix of multiple sources
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	4643723
PixInsight job	IKA559OZ8R515CXOP2NHZN3Q42I8ZQQ9
PixInsight queue size	n/a
PixInsight stage	n/a

RA (center)	12h18m59s.999
RA (top/left)	12h19m43s.626
RA (top/right)	12h21m12s.701
RA (bottom/right)	12h18m14s.789
RA (bottom/left)	12h16m47s.836

Dec (center)	+47°17′47″.77
Dec (top/left)	+46°50′58″.43
Dec (top/right)	+47°34′12″.28
Dec (bottom/right)	+47°44′36″.71
Dec (bottom/left)	+47°01′14″.23

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Contribution Index (beta):

M106

M106

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Image Index:

Contribution Index (beta):

M106

M106

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E

Sky plot

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