Veil Nebula in Cygnus 3 x 2 Mosaic (Sigga)

Celestial hemisphere: Northern · Constellation: Cygnus (Cyg) · Contains: 32 Vul · 49 Cyg · 52 Cyg · 53 eps Cyg · BW Vul · Filamentary nebula · Gienah · IC 1340 · Lace-work nebula · NGC 6960 · NGC 6974 · NGC 6979 · NGC 6992 · NGC 6995 · Network nebula · Sh2-103 · T Vul · The star 32Vul · The star 49Cyg · The star 52Cyg · The star Gienah (εCyg) · Veil nebula

Powered byPixInsight

Veil Nebula in Cygnus 3 x 2 Mosaic

Powered byPixInsight

Veil Nebula in Cygnus 3 x 2 Mosaic

The Veil Nebula is a cloud of heated and ionized gas and dust in the constellation Cygnus

It constitutes the visible portions of the Cygnus Loop, a supernova remnant, many portions of which have acquired their own individual names and catalogue identifiers. The source supernova was a star 20 times more massive than the Sun, which exploded around 8,000 years ago. The remnants have since expanded to cover an area of the sky roughly 3 degrees in diameter (about 6 times the diameter, or 36 times the area, of the full Moon). The distance to the nebula is not precisely known, but Far Ultraviolet Spectroscopic Explorer (FUSE) data supports a distance of about 1,470 light-years.

The brighter segments of the nebula have the New General Catalogue designations NGC 6960, 6974, 6979, 6992, and 6995. The easiest segment to find is 6960, which runs behind the naked eye star 52 Cygni. NGC 6992/5 are also relatively easy objects on the eastern side of the loop. NGC 6974 and NGC 6979 are visible as knots in an area of nebulosity along the northern rim. Pickering's Triangle is much fainter, and has no NGC number (though 6979 is occasionally used to refer to it). It was discovered photographically in 1904 by Williamina Fleming (after the New General Catalogue was published), but credit went to Edward Charles Pickering (typical!!!).

--Wikipedia

3 x 2 mosaic in LRGB, each panel 4 x 300 seconds with 20% overlap calculated. Stitched in MSFT ICE. Frankly turned out way better than expect although maybe is better narrow band object?

"Nordish by nature"
Women Astrophotographers

Please note: The following tables are updated every 24 hours.

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	2685388
PixInsight job	V0HSJAXX2GGSSM2GNVIVGM6VPFCIP0JN
PixInsight queue size	n/a
PixInsight stage	n/a

RA (center)	20h49m17s.38
RA (top/left)	21h00m01s.50
RA (top/right)	20h59m06s.19
RA (bottom/right)	20h37m50s.70
RA (bottom/left)	20h40m09s.80

Dec (center)	+30°55′04″.3
Dec (top/left)	+27°39′53″.9
Dec (top/right)	+34°20′49″.2
Dec (bottom/right)	+34°06′15″.10
Dec (bottom/left)	+27°26′46″.7

Image Index:

Contribution Index (beta):

Veil Nebula in Cygnus 3 x 2 Mosaic

Veil Nebula in Cygnus 3 x 2 Mosaic

Equipment

Acquisition details

Description

Comments

Sky plot

Histogram

In these public groups

		...
You have no new notifications.

Image Index:

Contribution Index (beta):

Veil Nebula in Cygnus 3 x 2 Mosaic

Veil Nebula in Cygnus 3 x 2 Mosaic

Equipment

Acquisition details

Description

Comments

Sky plot

Histogram

In these public groups

Notifications

AstroBin is in READ ONLY mode

Sorry :-(

Sorry :-(

Sorry :-(

Are you really sure?

Warning!

Warning!

Are you sure?

Report abuse

Slideshow settings

IOTD/TP stats (last [x] days)

Distribution of astrophotographers

Distribution of subject types

Distribution of data sources

Sorry

Sorry

Share

Upload new revision

Upload uncompressed source (XISF/FITS/PSD/TIFF)

Delete image and all its revisions?

Delete original image?

Delete all other versions?

Delete all revisions?

IOTD/TP stats

The following people like this image

The following people bookmarked this image

Warning

Flag malfunctioning thumbnails

Contains

Remove yourself as a collaborator

Plate-solving information