The Pickering's Triangle, Metsavainio

Equipment

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Acquisition details

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Description

Image is in mapped colors, from the emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen.

This combination is generally called to HST-palette. It's used originally by the Hubble Space Telescope.

I managed to shoot enough data for the S-II channel, to build a three channel color image, last night.

It was very windy and i had hard time with guiding. There was some serious technical difficulties with my gears. After spending ten busy hours up in the observatory, I had only four 20 min. S-II frames, duh...

Pickering's Triangle, Simeis 3-188, is a small part of the Veil Nebula supernova remnant in constellation Cygnus.

Veil Nebula is a cloud of ionized gas and dust, leftovers from an exploded star. The star went off some 5000-8000 years ago at distance of about 1470 light years. This, relatively faint target, is difficult to image due to the large angular diameter, about three degrees, and a dense star field.

More info behind the link.

Comments

Revisions

  • The Pickering's Triangle, Metsavainio
    Original
  • Final
    The Pickering's Triangle, Metsavainio
    B

Histogram

The Pickering's Triangle, Metsavainio