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Astrophotography by Bob Franke

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IC 434 ( The Horsehead Nebula ) Hα Filtered


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Instrument

12.5" RCOS @  ~f/9 (2880 mm fl) 0.643 arcsec / pixel.  Zoomify image scale is 0.96 to 2.88 arcsec / pixel.

Mount

Paramount ME

Camera

SBIG STL-11000 w/ internal filter wheel, AstroDon 6nm Filter

Acquisition Data

11/01/2009 to 12/17/2009 Chino Valley, AZ... with CCDAutoPilot3 & CCDSoft.

Exposure

Hα  660 min (22 x 30 min, bin 1x1)

Software

  • CCDSoft, CCDStack, Photoshop CS w/ the Fits Liberator plugin and Noel Carboni's PhotoShop actions.

  • PixFix32 (pre-beta) to repair hot/cold pixels and column defects.

  • CCDStack to calibrate, register, normalize, data reject, & combine the sub exposures.

  • PhotoShop for on-linear stretching.

Comment

North is to the left.

At a distance of about 1500 light years, the Horsehead Nebula, in Orionis, is part of a large dark molecular cloud. Also known as Barnard 33, the unusual shape was first discovered on a photographic plate in the late 1800's. The background glow originates from hydrogen gas predominantly behind the nebula, ionized by the nearby bright star Sigma Orionis. The darkness of the Horsehead is caused mostly by thick dust, although the lower part of the Horsehead's neck casts a shadow to the left.

Source: NASA APOD