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IC 1805 in Cassiopeia widefield, Dan Kordella

IC 1805 in Cassiopeia widefield

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IC 1805 in Cassiopeia widefield, Dan Kordella

IC 1805 in Cassiopeia widefield

Equipment

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Acquisition details

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Description

Using the Askar FRA400 astrograph with the 0.7x f/3.9 reducer = tons of fun! Experimented with a range of different exposure times but in the end settled on 210 seconds. Glad I finished this when I could because with terrible weather it's getting late in the year to try to keep working on some of these "autumn" targets. 

From Wikipedia:The Heart NebulaIC 1805Sharpless 2-190, is some 7500 light years away from Earth and is located in the Perseus Arm of the Galaxy in the constellation Cassiopeia. It was discovered by William Herschel on 3 November 1787.[1] It is an emission nebula showing glowing ionized hydrogen gas and darker dust lanes.The brightest part of the nebula (a knot at its western edge) is separately classified as NGC 896, because it was the first part of the nebula to be discovered. The nebula's intense red output and its morphology are driven by the radiation emanating from a small group of stars near the nebula's center. This open cluster of stars, known as Collinder 26 or Melotte 15, contains a few bright stars nearly 50 times the mass of our Sun, and many more dim stars that are only a fraction of our Sun's mass.The Heart Nebula is also made up of ionised Oxygen and Sulfur gasses, responsible for the rich blue and orange colours seen in narrowband images. The shape of the nebula is driven by stellar winds from the hot stars in its core. The nebula also spans almost 2 degrees in the sky, covering an area four times that of the diameter of the full moon.

Comments

Revisions

  • IC 1805 in Cassiopeia widefield, Dan Kordella
    Original
  • IC 1805 in Cassiopeia widefield, Dan Kordella
    B
  • IC 1805 in Cassiopeia widefield, Dan Kordella
    C
  • Final
    IC 1805 in Cassiopeia widefield, Dan Kordella
    D

B

Description: Starless version of the luminance, only. Just because I thought it was really cool :)

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C

Description: This is the starless version of the luminance + chrominance layers. You can see a lot of the nebula structure that gets kind of lost when the stars getting added back in.

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D

Description: A variation on the processing used for the first version (which used a synthetic luminance layer). This version does not. I also did an additional noise reductive (TGCDenoise) pass, though it may have been too aggressive. This version is more contrasty, I think.

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Histogram

IC 1805 in Cassiopeia widefield, Dan Kordella

In these public groups

NOVAC