IC 348, Barnard 3, 4, and 5 (Brandon Tackett)

Celestial hemisphere: Northern · Constellation: Perseus (Per) · Contains: 38 Per) · 38 omi Per · Alatik (ο Per · Ati · Atik · B3 · B4 · B5 · HD22781 · HD22963 · HD23478 · HD23626 · HD23699 · HD23802 · HD278879 · HD278882 · HD278936 · HD278937 · HD278939 · HD278940 · HD278942 · HD278996 · HD278998 · HD281156 · HD281157 · HD281159 · HD281162 · HD281217 · HD281218 · HD281224 · And 11 more.

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IC 348, Barnard 3, 4, and 5

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IC 348, Barnard 3, 4, and 5

Another beautiful dark and dusty nebula within the Perseus. So many wonderful components of the image. Barnard 3 is a finely detail dark nebula with surrounding emission nebula and reflection nebula in the left hand portion of the image. Even more, the central portion while somewhat distracted by the trinary stars system seen as the bright star Atik, has gorgeous reflection nebula with dark nebula in and surrounding the star forming region IC 348. Finally, the top right left and bottom right have rivulet Barnard 5 dark nebula as it travels off the frame.

The Atik system comprises three stars approximately 1,100 light years from earth. The closely orbiting binary stars of the system are B class stars that have an orbital period of 4.4 days per wikipedia. These two stars are a mere 33 solar radii from each other. While in the near vicinity from our vantage point, IC 438 is separate from the system. IC 438 is a star forming area and open cluster with approximately 400 stars.

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Status	Advanced success
Started	...
Astrometry.net job	9003844
PixInsight job	L4I1IZAET14TVW0O3V2PGOY1738ZIVBQ
PixInsight queue size	n/a
PixInsight stage	TASK_LOG

RA (center)	03h43m40s.10
RA (top/left)	03h38m03s.83
RA (top/right)	03h49m01s.75
RA (bottom/right)	03h49m23s.20
RA (bottom/left)	03h38m12s.60

Dec (center)	+32°11′24″.4
Dec (top/left)	+31°18′29″.1
Dec (top/right)	+31°14′28″.10
Dec (bottom/right)	+33°03′26″.6
Dec (bottom/left)	+33°07′26″.1

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IC 348, Barnard 3, 4, and 5

IC 348, Barnard 3, 4, and 5

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IC 348, Barnard 3, 4, and 5

IC 348, Barnard 3, 4, and 5

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