A reprocess of the SeaHorse nebula / Barnard 150 (mosaic) (Anthony Brunet-Bessette)

Celestial hemisphere: Northern · Constellation: Cepheus (Cep) · Contains: B148 · B149 · B150 · Fireworks Galaxy · HD196085 · HD197373 · HD197734 · HD198300 · HD198662 · HD199306 · LDN 1076 · LDN 1082 · MASIV J2030+5957 · MQ J203019.09+592825.2 · MQ J203246.34+594214.2 · MQ J203307.76+601551.5 · MQ J203400.31+595919.6 · MQ J203416.27+600631.9 · MQ J203431.37+600216.8 · MQ J203439.58+592716.2 · MQ J203446.58+600245.2 · MQ J203451.02+600756.6 · MQ J203456.65+600827.4 · MQ J203521.47+601914.7 · MQ J203533.30+602152.6 · MQ J203602.43+601325.5 · MQ J203629.68+592816.0 · MQ J203631.96+602328.6 · MQ J203653.58+601035.5 · NGC 6939 · And 43 more.

Powered byPixInsight

A reprocess of the SeaHorse nebula / Barnard 150 (mosaic)

Powered byPixInsight

A reprocess of the SeaHorse nebula / Barnard 150 (mosaic)

Hi everyone,
here is a reprocess of the SeaHorse nebula (mosaic) aka Barnard 150.

Description of the object :Barnard 150, also known as Seahorse Nebula, is a dark molecular cloud of dust in Cepheus constellation, so thick, that it absorbs all the light that comes from the stars behind it. This molecular cloud is part of our Milky Way galaxy, one of the 182 objects cataloged by astronomer Edward E. Barnard and it lies at about 1200 Light Years away. Cloud location on the Milky Way's plane, makes it stand out on the background completely filled with colorful stars of any age and size. Due to all of the light emitted from these stars, the distinctive, serpent like shape of this molecular cloud can be observed. And with rotation of the image by 90 degrees, one can easily recognize why this cloud inherent a second name of "Seahorse Nebula". This nebula is about 1 degree in size, width of two Moons. What is also interesting about this cloud, as it have 3 highly dense dust cores, which actually is a star formation regions. They were cataloged by Lynds and named LDN 1082 A, B and C, which are marked on annotated image. Source : myastroscience

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	6883425
PixInsight job	RY2YB2NMPK8ESPQPTAIBGPU4C0ZOPIA7
PixInsight queue size	n/a
PixInsight stage	TASK_LOG

RA (center)	20h43m28s.27
RA (top/left)	20h29m35s.79
RA (top/right)	20h54m46s.93
RA (bottom/right)	20h58m03s.14
RA (bottom/left)	20h31m17s.70

Dec (center)	+60°14′53″.9
Dec (top/left)	+59°26′27″.7
Dec (top/right)	+58°57′29″.9
Dec (bottom/right)	+60°57′43″.8
Dec (bottom/left)	+61°27′58″.7

Image Index:

Contribution Index (beta):

A reprocess of the SeaHorse nebula / Barnard 150 (mosaic)

A reprocess of the SeaHorse nebula / Barnard 150 (mosaic)

Equipment

Acquisition details

Description

Comments

Sky plot

Histogram

		...
You have no new notifications.

Image Index:

Contribution Index (beta):

A reprocess of the SeaHorse nebula / Barnard 150 (mosaic)

A reprocess of the SeaHorse nebula / Barnard 150 (mosaic)

Equipment

Acquisition details

Description

Comments

Sky plot

Histogram

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