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Saturday, October 9, 2010

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:








NGC 300







NGC 300, the spiral galaxy in constellation Sculptor, distance is about 6 million light years.

 It's likely, that NGC300 and NGC55 forms a gravitationally bound pair.
I have shot NGC 55, an irregular galaxy, ealier and it can be found here:
http://astroanarchy.blogspot.com/2010/09/ngc-55-irregular-galaxy-in.html

Image of NGC 55
"NGC300 and NGC55 forms a gravitationally bound pair."

Surface brightness is lowish and this image gave me a hard time when processing the raw data. I tried to keep a "diffused" look of it. Active parts of this galaxy can be seen as a Blue and Red areas in a spiral arms.


A closeup


Technical details:

16" RCOS ja Apogee U9000 camera. 
LRGB combo. An Australian remote telescope
5x1200s for the Luminance and 2x600s / RGB-channel . Dark, Bias and Flat calibrated.
Raw data is shared by Petri Kehusmaa and J-P Metsavainio

Processing workflow:
Image acquisition, MaxiDL v4.xxx
Stacked and calibrated in CCDStack.
Deconvolution with a CCDSharp, 30 iterations, added at 50% weight.
Levels, curves and color combine in PS CS3.

Something extra in my image

A bright trail trough a single raw frame of NGC 300.

A closeup, there is odd looking pattern inside of trail.


Mystery was solved by a help from Bert Candusio, the administrator of Northern Galactic group.
Object seen in the image is a geocentric satellite COSMOS 1536.
Thank you Bert.