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Sunday, June 5, 2011

Messier 76, the "Little Dumbbell Nebula", apparent scale in the sky





I have shot many targets with several focal lengths. 
Due that, I will publish some of my material as an image sets, with different field of view and detail levels.
The fractal nature of our universe stands out nicely by this way and it will make the orientation more easy.

Many times, it's difficult to understand the image scale of astronomical images.
Due that, I will add a Moon circle in some of the images to show the angular scale in a sky. 
The full Moon has an angular size of ~30 arc minutes, that's equal to ~0,5 degrees.



M76, the "Little Dumbbell Nebula"
In constellation Perseus.

NOTE. The size of the full Moon (0,5 degrees) is marked as a gray circle in all of the images.
Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. 
This composition is very close to a visual spectrum.

One image of M76 is used to make this image series,
original image and technical details can be found here:


Messier 27, the "Dumbbell Nebula", apparent scale in the sky





I have shot many targets with several focal lengths. 
Due that, I will publish some of my material as an image sets, with different field of view and detail levels.
The fractal nature of our universe stands out nicely by this way and it will make the orientation more easy.

Many times, it's difficult to understand the image scale of astronomical images.
Due that, I will add a Moon circle in some of the images to show the angular scale in a sky. 
The full Moon has an angular size of ~30 arc minutes, that's equal to ~0,5 degrees.



Messier 27, the "Dumbbell Nebula"

Ra 19h 59m 36.340s Dec +22° 43′ 16.09″



NOTE. The size of the full Moon (0,5 degrees) is marked as a gray circle in all of the images.
Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. Star colors are mixed from the NB channels, Red=H-a, G=O-III and B= 85%O-III + 15%H-a.This composition is very close to a visual spectrum.


One image of M27 is used to make this image series.
Original image and technical details can be found here:




Deep deep space, an anaglyph Red/Cyan 3D movie




NOTE!
You'll need Red/Cyan Eyeglasses to be able to see the movie as 3D.
If you have a Red and Blue filters, you can use them! Red goes to Left eye.



A ten minute still motion movie from a collection of my experimental 3D-astronomical objects.




Please note, there is a HD-selector, at lower Right corner of the window, set to 360p.
If you like to see the movie in higher resolution, use this selector. Maximum resolution of the movie is 1080p.
Double click the movie window to see it in full screen!

3D-images used in the movie and more can be found, in different 3D-formats, from my portfolio.

All the material in this movie have been imaged and converted by me. Original 2D-images used for the movie, can be found here: http://astroanarchy.zenfolio.com/



Saturday, June 4, 2011

IC1848, the "Soul Nebula", apparent scale in the sky





I have shot many targets with several focal lengths. 
Due that, I will publish some of my material as an image sets, with different field of view and detail levels.
The fractal nature of our universe stands out nicely by this way and it will make the orientation more easy.

Many times, it's difficult to understand the image scale of astronomical images.
Due that, I will add a Moon circle in some of the images to show the angular scale in a sky. 
The full Moon has an angular size of ~30 arc minutes, that's equal to ~0,5 degrees.



IC 1848 zoom in
In constellation Cassiopeia




Image is in HST-palette from the emission of ionized elements, R=Sulfur,
 G=Hydrogen and B=Oxygen. NOTE. The size of the full Moon (0,5 degrees) is marked as a gray circle in all of the images.


IC 1848, second zoom in


NOTE. The size of the full Moon (0,5 degrees) is marked as a gray circle in all of the images.
Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. Star colors are mixed from the NB channels, Red=H-a, G=O-III and B= 85%O-III + 15%H-a.This composition is very close to a visual spectrum.


Images used in the series above from top to bottom



  1. A wide field image of the area, covering about 5 degrees, ~300', of the sky. (Ten full Moons side by side)
    IC 1805, the "Heart Nebula", locates at upper Right and  IC 1848 can be seen at lower Left. Image is shot with a Canon EF 200mm f1.8 camera lens and a QHY9, a cooled astronomical camera.
    Baader narrowband filter set, total exposure time was ~1,5 hours (A very fast lens was used!).
  2. A medium wide field image is shot with a Tokina AT-X 300mm f2.8 camera lens and a QHY9, a cooled astronomical camera. Baader narrowband filter set, total exposure time was ~5 hours .
  3. Last image was shot with a Meade LX200 GPS 12" telescope @ f0.5 and a QHY9, a cooled astronomical camera.Baader narrowband filter set, total exposure time was ~2,5 hours. 
Links to the original images, used in series, from top to bottom

A panorama mosaic from the IC1396 to Sharpless 129




While making scale studies from various objects, I did make some new panoramas from archived images.
I will publish some of them as an individual images, comments and suggestions are welcome.


Panorama, from IC 1396, the "Elephant's Trunk Nebula" to the Sh2-129 
In constellation Cepheus

Image is in HST-palette from an emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen.




Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. Star colors are mixed from the NB channels, Red=H-a, G=O-III and B= 85%O-III + 15%H-a.This composition is very close to a visual spectrum.



There are two individual images used to make this panoramic image:

  1. IC 1396, http://astroanarchy.blogspot.com/2011/01/ic-1396-reprocessed.html
  2. Sharpless 129, http://astroanarchy.blogspot.com/2008/03/sh2-129.html 
  3. some data from newer image of Sh2-129, http://astroanarchy.blogspot.com/2011/01/sh2-129-reprocessed.html
Technical details for the images above

Sh2-129 Imaging data:
  Optics: Canon FD 200mm f2.8 lens with full aperature
- Camera: QHY8
- Platform and guiding: LX200 GPS 12" with QHY5 guider and PHD-guiding
- Exposures: 6 x 1800s H-alpha +4 x 600s RGB + Flats and Bias frames, no darks
- Filter: Baader 7nm H-alp + IDAS LP for RGB

IC 1396  Imaging data:
 Camera, QHY8
Filters, Baader 7nm H-alpha, Baader 8,5nm O-III and Baader 8nm S-II
-Optics, Tokina AT-X 300mm @ f2.8
-Exposures, 7X 1200s H-alpha, 8 X 1200 O-III and 3X1200s S-II + flats and bias
Guiding, LX200 GPS 12" + PHD-guiding and Lodestar



Friday, June 3, 2011

Panoramic mosaic from the M52 & Bubble to Wizard Nebula





While making scale studies from various objects, I did make some new panoramas from archived images.
I will publish some of them as an individual images, comments and suggestions are welcome.


Panorama, from M52, Bubble Nebula & Sh2-157 to the Wizard Nebula 
In constellation Cassiopeia


A panorama from the M52 to the Wizard Nebula in constellation Cassiopeia.
Image is in HST-palette from an emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen.



Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. Star colors are mixed from the NB channels, Red=H-a, G=O-III and B= 85%O-III + 15%H-a.This composition is very close to a visual spectrum.
Note. Size of the full Moon is marked as a gray circle, at lower Left corner, for a scale.

There are two individual images used to make this panoramic image:

  1. Sharpless 157, http://astroanarchy.blogspot.com/2011/03/sh2-157-reprocessed.html
  2. Wizard Nebula, http://astroanarchy.blogspot.com/2011/02/sh2-142-wizard-nebula-wide-field.html

Technical details for the images above

Sh2-157 Imaging data:
 Camera, QHY8 - 
Filters, Baader 7nm H-alpha, Baader 8,5nm O-III and Baader 8nm S-II - 
Optics, Tokina AT-X 300mm @ f2.8 - 
Exposures, 5X 1200s H-alpha, 2 X 1200 O-III and 2X1200s S-II + flats and bias - 
Guiding, LX200 GPS 12" + PHD-guiding and Lodestar

Wizard Nebula, Sharpless 142, NGC7380  Imaging data:
 Camera, QHY8 - 
Filters, Baader 7nm H-alpha, Baader 8,5nm O-III and Baader 8nm S-II - 
Optics, Tokina AT-X 300mm @ f2.8 - 
Exposures, 10X 1200s H-alpha, 2 X 1200 O-III and 2X1200s S-II + flats and bias - 
Guiding, LX200 GPS 12" + PHD-guiding and QHY5

Labeled version










Thursday, June 2, 2011

A panorama from the Sharpless 221 to 216




While making scale studies from various objects, I did make some new panoramas from archived images.
I will publish some of them as an individual images, comments and suggestions are welcome.


Sharpless panorama, Sh2-216, 217, 219, 221 and BFS44 
East of constellation Camelopardalis


Image is in HST-palette from an emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen.


There are two individual images used to make this panoramic view:



  1. Left side, http://astroanarchy.blogspot.com/2011/01/two-ways-to-end-life-planetary-nebula.html
  2. Right side, http://astroanarchy.blogspot.com/2011/02/sh2-216-project-finalized.html

This image covers over six degrees of sky horizontally, that's 12 full Moons side by side. Here is a "scale study out of this target, the Moon is marked as a gray circle:



A natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. Star colors are mixed from the NB channels, Red=H-a, G=O-III and B= 85%O-III + 15%H-a.This composition is very close to a visual spectrum.
Note. Size of the full Moon is marked as a gray circle, at lower Right corner, for a scale.


An annotated image shows objects in the field


There are very little information out of objects in the image and there is very few images from them generally.
I think, this must be the first three band narrowband image out of this field.

Objects in this image are spread out over wide range of distances. They are not forming a single complex, like the Cassiopeia arc west of Camelopardalis. The largest objects in a field are Sharpless 221 and 216.

First from the Left is a supernova remnant, SNR 160.4+02.8 (Sh 2-221) , the distance is unknown. 
The Planetary Nebula,  PK 158+00 1 (Sh 2-216) , at Right end of an image, distance of only 120 parsecs (~390 light years) makes this to a one of the oldes and largest planetary nebula known.

Smaller objects in a field are Sh2-217, 4100 solar mass molecular cloud at distance of 5200 parsecs (0ver 16.000 light years) and Sh2-219, an HII region at distance of 4200 parsecs (Over 13.000 light years)
Last object BFS44, at bottom center, located at distance of 6100 parsecs (over 19.000 light years), almost nothing has been published from this object.

Source for information above, galaxymap.org, http://galaxymap.org/drupal/node/44








Wednesday, June 1, 2011

Panorama from the Butterfly to Crescent





While making scale studies from various objects, I did make some new panoramas from archived images.
I will publish some of them as an individual images, comments and suggestions are welcome.


Cygnus panorama

A panorama from the Butterfly to the Crescent Nebula in constellation Cygnus.
Image is in HST-palette from an emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen.
Note. Size of the full Moon is marked as a gray circle, at lower Right corner, for a scale.

There are two individual images used to make this panoramic image:

  1. Butterfly Nebula, http://astroanarchy.blogspot.com/2011/01/butterfly-nebula-reprocessed.html
  2. Crescent Nebula, http://astroanarchy.blogspot.com/2011/01/ngc-6888-crescent-nebula-wide-field.html

Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. Star colors are mixed from the NB channels, Red=H-a, G=O-III and B= 85%O-III + 15%H-a.This composition is very close to a visual spectrum.


There is a third overlapping image from the same area, the "Tulip Nebula". I have a panoramic image containing it as well. I like this panorama but it's so long, that image gets very small, so I didn't place it as a main image in this post.

A long and narrow version, with the "Tulip Nebula"




Tulip Nebula, the original image:
http://astroanarchy.blogspot.com/2011/01/tulip-nebula-sh2-101-wide-field-closeup.html


All images in this page have been part of an older mosaic, the "Cygnus Trio"
It was my very first APOD (Astronomy Picture Of  Day) published  by NASA.
http://astroanarchy.blogspot.com/2008/11/apod.html








M57, the "Ring Nebula", apparent scale in the sky




I have shot many targets with several focal lengths. 
Due that, I will publish some of my material as an image sets, with different field of view and detail levels.
The fractal nature of our universe stands out nicely by this way and it will make the orientation more easy.

Many times, it's difficult to understand the image scale of astronomical images.
Due that, I will add a Moon circle in some of the images to show the angular scale in a sky. 
The full Moon has an angular size of ~30 arc minutes, that's equal to ~0,5 degrees.


M57, A planetary Nebula
In constellation Lyra

NOTE. The size of the full Moon (0,5 degrees) is marked as a gray circle in all of the images.
Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. Star colors are mixed from the NB channels, Red=H-a, G=O-III and B= 85%O-III + 15%H-a.This composition is very close to a visual spectrum.

This is generally a difficult target, due the small angular size and an extreme dim outer ring structure versus bright core. 

One image of M57 is used to make this image series.
Original image and technical details can be found here:





Tuesday, May 31, 2011

Apparent scale study of a rarely imaged planetary, Sharpless 216





I have shot many targets with several focal lengths. 
Due that, I will publish some of my material as an image sets, with different field of view and detail levels.
The fractal nature of our universe stands out nicely by this way and it will make the orientation more easy.

Many times, it's difficult to understand the image scale of astronomical images.
Due that, I will add a Moon circle in some of the images to show the angular scale in a sky. 
The full Moon has an angular size of ~30 arc minutes, that's equal to ~0,5 degrees.


Sh2-216, A planetary Nebula in Perseus, the closest PN to Earth ever discovered
Ra 04h 45m 35s Dec +46° 48′ 30"

Image is in HST-palette from the emission of ionized elements, R=Sulfur,
 G=Hydrogen and B=Oxygen.
NOTE. The size of the full Moon (0,5 degrees) is marked as a gray circle in all of the images.
This is a very large and dim object.

Images used in the series above from top to bottom



  1. Large field of view image shows an extremely dim supernova remnant at Left. Imaged with a Canon EF 200mm f1.8 camera lens at full aperture 
  2. A zoomed in version from the previous image 
  3. A closeup image of Sh2-216 with Tokina AT-X 300mm f2.8 camera lens
  4. A zoomed in version from the previous image 
Links to the original images, used in series, from top to bottom

NGC2264, the "Cone Nebula", apparent scale in the sky





I have shot many targets with several focal lengths. 
Due that, I will publish some of my material as an image sets, with different field of view and detail levels.
The fractal nature of our universe stands out nicely by this way and it will make the orientation more easy.

Many times, it's difficult to understand the image scale of astronomical images.
Due that, I will add a Moon circle in some of the images to show the angular scale in a sky. 
The full Moon has an angular size of ~30 arc minutes, that's equal to ~0,5 degrees.


NGC 2264, the "Cone Nebula"
In constellation Orion

Image is in HST-palette from the emission of ionized elements, R=Sulfur,
 G=Hydrogen and B=Oxygen.
NOTE. The size of the full Moon (0,5 degrees) is marked as a gray circle in all of the images.

Images used in the series above from top to bottom


  1. Two panel mosaic of Cone and Rosette Nebulae. Shot with a Canon EF 200mm f1.8 lens, Baader NB-filters and QHY9 cooled astronomical camera.
  2. The Cone Nebula half of the mosaic image.
  3. Zoomed in version from the previous image 
  4. A close up of the Cone Nebula imaged with a Meade LX200 GPS 12" telescope, focal lenght ~2000mm.
Links to the original images, used in series, from top to bottom

Monday, May 30, 2011

NGC7380, the "Wizard Nebula", apparent scale in the sky





I have shot many targets with several focal lengths. 
Due that, I will publish some of my material as an image sets, with different field of view and detail levels.
The fractal nature of our universe stands out nicely by this way and it will make the orientation more easy.

Many times, it's difficult to understand the image scale of astronomical images.
Due that, I will add a Moon circle in some of the images to show the angular scale in a sky. 
The full Moon has an angular size of ~30 arc minutes, that's equal to ~0,5 degrees.


NGC 7380, Sharpless 142 (Sh2-142)
In connstellation Cepheus


Sh2-142 alias NGC 7380, in HST-palette from the emission of ionized elements, R=Sulfur,
 G=Hydrogen and B=Oxygen.
NOTE. The size of the full Moon (0,5 degrees) is marked as a gray circle in all of the images.


Images used in the series above from top to bottom

  1. A wide field mosaic from the Bubble and Sharpless 157 to the Wizard Nebula at Right. Images are taken with a Tokina AT-X 300mm camera lens. 
  2. A Sh2-142, the Wizard Nebula part of the mosaic, Tokina AT-X 300mm 
  3. Zoomed in version from the previous image 
  4. A close up of the Nebula imaged with a Meade LX200 GPS 12" telescope, focal lenght ~2000mm.A zoomed 
Links to the original images, used in series, from top to bottom