Celestial hemisphere:  Northern  ·  Constellation: Cepheus (Cep)  ·  Contains:  B160  ·  B161  ·  B162  ·  B163  ·  B365  ·  B367  ·  B368  ·  Erakis  ·  Erakis (μ Cep)  ·  HD204231  ·  HD204613  ·  HD205196  ·  HD205510  ·  HD205948  ·  HD206081  ·  HD206183  ·  HD206267  ·  HD206482  ·  HD206773  ·  HD207086  ·  HD239671  ·  HD239710  ·  HD239712  ·  HD239724  ·  HD239725  ·  HD239727  ·  HD239729  ·  HD239748  ·  HD239767  ·  IC 1396  ·  And 43 more.
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IC1396 and vdB142 - Elephant Trunk - Foraxx and CFHT Palette, Massimo Marchini
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IC1396 and vdB142 - Elephant Trunk - Foraxx and CFHT Palette

Link to TIFF/FITS: https://flic.kr/p/2pm2C7V
Getting plate-solving status, please wait...
IC1396 and vdB142 - Elephant Trunk - Foraxx and CFHT Palette, Massimo Marchini
Powered byPixInsight

IC1396 and vdB142 - Elephant Trunk - Foraxx and CFHT Palette

Link to TIFF/FITS: https://flic.kr/p/2pm2C7V

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Acquisition details

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Description

The IC1396 nebula is an open cluster associated with a vast diffuse nebula in the constellation of Cepheus. Located approximately 3000 light-years from Earth, this H II region spans over 50 arcminutes in the night sky. Among its most notable features is the “Elephant’s Trunk” (vdB 142), a formation of interstellar gas and dust that stands out against the starry background. The nebula is illuminated by the young blue stars of the Cepheus OB2 association, whose ionizing radiation has created a ring of molecular gas. Within the nebula, there are numerous dark globules, dense regions of star formation.The image was captured using a Tecnosky AG70 astrograph and a monochrome ZWO ASI2600MM PRO camera. 54 narrowband frames of 600" for 9 hours total integration. Despite challenges from weather conditions and light pollution, careful selection allowed for the integration of the best images, discarding a greater number of shots than those used.The final processing was done with Pixinsight software. Two different palettes were selected:-          The Foraxx Palette, which is based on the contrast between the rust tones of S II and the blue tones of O III, while Ha is used to modulate the red and blue. This palette creates an image with vivid colors and fascinating details, using dynamic PixelMath expressions to combine the narrowband images.-          The CFHT Palette, which is named after the Canada-France-Hawaii Telescope, and which uses a different combination from the classic Hubble Palette, assigning S II to the green channel, O III to the blue channel, and H-alfa to the red channel. This palette creates an image with particular gold and purple tones, highlighting the different emission regions of the nebula.

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