Focal Pointe Observatory
Astrophotography by Bob Franke

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NGC 663 & Others

 

Click the image for a 57% size view. (2100 x 1500 - 1.56 MB)

Instrument

Takahashi FSQ-106ED @ f/5.0 (530 mm F.L.) Captured at 2.1 arcsec/pixel.  Shown at 3.32 and 9.28 arcsec/pixel.

Mount

Losmandy G11 with Gemini L4 v1.0

Camera

SBIG STF-8300M Self Guiding Package w/ mono ST-i, using Baader RGB filters.

Acquisition Data

11/3/2015 to 11/8/2015  Chino Valley, AZ with CCD Commander & CCDSoft. 

Exposure

Red

168 min. (24 x 7 min. each)   Binned 1x1

Green

217 min. (31 x 7 min. each)         "

Blue

273 min. (39 x 7 min. each)         "

 RGB combine ratios are 1.00, 1.35, 1.54

Software & Processing Notes

  • CCDSoft, CCDStack, PixInsight, Photoshop CS6

  • eXcalibrator v6.0 for (g:r), (b:r) color balancing, using 61 stars from the Pan-STARRS database.

  • PixInsight processing includes calibration, registering, stacking, RGB creation, gradient removal, non-linear stretching with HistogramTransformation.

  • PhotoShop for JPEG creation.

  • Annotation by Astrometry.net

Comment

North is to the right.

This group of clusters is located in the constellation Cassiopeia.  From left to right, in the bottom half of the image, are NGC 659, 663 and 654. The respective distances are 8,200, 6,850 and 7,830 light years. All three are very young clusters with respective ages of 20, 25 and 14 million years.

At the upper right, is the open cluster IC 166. With an intermediate age of 1 to 1.25 million years, it is at a distance of 13 to 15,000 light years. With its greater distance and line of sight near a dark nebula, the color of the cluster is greatly reddened.

Perhaps the most interesting object is the nonexistent nebula, IC 155. Charles Joseph Etienne Wolf published his discovery of this nebula on December 30, 1893. This is thought to be one of the earliest examples of a photographic plate defect being mistaken for a nebula. Also, it may have been an internal reflection in Wolf's telescope.