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Saturday, October 9, 2010

M57 as a 3D-stereo pair






Parallel vision



Cross vision

Other 3D-formats can be found here:

Original 2D-image and details:


NOTE! This 3D-study is a personal vision about forms and shapes, based on some known facts and an artistic impression.



M57 as an anaglyph Red/Cyan 3D






Other 3D-formats can be found here:

Original 2D-image and details:



NOTE! This 3D-study is a personal vision about forms and shapes, based on some known facts and an artistic impression.

Thursday, October 7, 2010

M57, the "Ring Nebula", project finalized







A narrow band and broad band luminance mix image of the M57 as a bi color, H-alpha & O-III, composition.Not too commonly imaged outer halo structure can be seen in an image. There is least two layers of it, outer one is faintly seen in this image. A clear O-III signal is visible in a first layer of outer halo.
The halo was clear in H-alpha channel and there was some hints of it in luminance one.

Ring Nebula, M57, NGC 6822, locates in constellation Lyra, near a very bright star Vega. This planetary nebula lays about 2300 light years away from the Earth and has a diameter of 1,3 light years.
The small angular diameter, 230" x 230", makes this target difficult to image. The central white dwarf of planetary nebula nucleus is seen in an image as a Bluish dim star, visual magnitude is 15,75. Star was visible only in O-III channel and luminance channel.

A closeup



Less compressed image in my Portfolio:
http://astroanarchy.zenfolio.com/p1072219942/h2becaeff#h2becaeff

Technical details:

Processing work flow:
Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack.
Deconvolution with a CCDSharp, 30 iterations.
Levels, curves and color combine in PS CS3.

Telescope, Meade LX200 GPS 12" @ f5
Camera, QHY9 Guiding, SXV-AO @ 8,5Hz
Image Scale, 0,75 arcseconds/pixel
Exposures H-alpha 9x1200s, binned 1x1
O-III 3x1200s, binned 1x1
Luminance, IDAS LP-filter 9 x 600s, binned 1x1


Wednesday, October 6, 2010

3D-study of NGC 300 galaxy



An experiment with the NGC 300. All the stars from our milky way are removed and the original 2D-galaxy image is the projected to a 3D-surface. The resulting 3D-model is animated to a movie file. The purpose is to show the actual shape of the galaxy, now distorted by a perspective.


Original 2D-image and the technical data: