Tuesday, March 31, 2015
IC 1795 in the Heart Nebula
I spent hours in two nights by shooting this busy area in IC 1805, the Heart nebula, at 13. and 15. March.
IC 1795
Click for a large image
A closeup
Click for a large image
INFO
IC 1795 is also known as a Fish Head Nebula. It's a star forming region in the northern constellation Cassiopeia at distance of about 6000 light years. My image shows about a square degree of sky, the actual size of the imaged area is around 130 light years. IC 1795 is a part of the large nebula complex known as IC 1805, the Heart Nebula.
Image in visual spectrum
Click for a large image
Image in emission of an ionized hydrogen only (H-alpha)
A two frame mosaic
Click for a large image
This photo of IC 1805 was partly overlapping with my previous image from the same area.
I made a small two frame mosaic out of them. I have shot more frames after this imaging project and now I'm able to make a high resolution mosaic of the whole IC 1805 area. I'll publish that later.
Orientation in IC 1805, the Heart Nebula
Click for a large image
Technical details
Processing work flow
Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack2.
Deconvolution with a CCDStack2 Positive Constraint, 33 iterations, added at 50% weight
Color combine in PS CS3
Levels and curves in PS CS3.
Imaging optics
Celestron Edge HD 1100 @ f7 with 0,7 focal reducer for Edge HD 1100 telescope
Mount
10-micron 1000
Mount
10-micron 1000
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x2 and SXV-AOL
Astrodon filter, 5nm H-alpha
Astrodon filter, 3nm O-III
Astrodon filter, 3nm S-II
Exposure times
H-alpha, 15 x 1200s = 5h
O-III, 3 x 1200s = 1h min.
S-II, 3 x 1200s = 1h min.
Total 7h
A single un cropped, calibrated and stretched 20 min. H-alpha frame as it comes from the camera
Optikfestival in Skara, Sweden
I had a pleasure to be invited as one of the speakers in "Optikfestival Skara", Sweden. The happening was organized by a Astrosweden, a largest optics retailer in Sweden. They are specialized to Astronomy, nature photography, hunting and microscopy. I was really impressed by the passion and knowledge they have about the the optics!
The owner, Christer Kjellner, has a personal interest to the subject and the sales team are experienced users of the products they are selling. That's not too common now a days! No matter if you are just entering in the subject or professional user they will find a solution for you, I'm sure.
I can highly recommend Astrosweden, if you'll have any needs for Astronomy, nature photographing, hunting scopes or microscopy.
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Ask for an offer or just have a look to the webshop: http://www.astrosweden.se/
Interior of the shop, they have a large stock of products on site.
Duel of the nature photographers
Tuesday, March 24, 2015
The blue dot and rings in Sh2-232
This is a followup to my previous blog post. When I was processing the data, I noticed a small nebula in center of the large complex of Sharpless 232. It seems to be the only O-III emission source in this large emission nebula. My O-III exposure was relatively short though, only 2h. The origin of this small ionization zone puzzles me. I made a small animation from integrated emission channels. No other processing, than calibration and simple un linear stretching has been done to the images.
EDIT
One mystery solved with a help from another astroguy. "Saloja" from a Finnish astro group used the Megastar database and found out, that this blue dot is a known planetary nebula, PN G173.5+03.2. Thank you Saloja!
Narrowband image of Sh2-232 in mapped colors
This animated GIF shows all three emission channels imaged for this photo, O-III, S-II and H-alpha.
The small nebula is visible in both, H-a and O-III, S-II doesn't show it. It could be nice to understand the mechanism behind this small object.
Is it part of the large nebula and what is the energy source for the ionization? It might even be a planetary nebula, part of the large Sh2-232 complex or a separate object front or behind it.
Has anyone else noticed this object? Let me know, if you have some info about it.
Is it part of the large nebula and what is the energy source for the ionization? It might even be a planetary nebula, part of the large Sh2-232 complex or a separate object front or behind it.
Has anyone else noticed this object? Let me know, if you have some info about it.
Another interesting feature of Sh2-232
A ring like formation
Monday, March 23, 2015
Sharpless 232 (Sh2-232) and companions in Auriga
This was one of the most difficult targets I have shot lately, very diffused and dim. Now when the season is about to end, up here 65N, we have had clear skies one after another and I have collected exposures to unveil this target. Total exposure time is now about 24h hours. Image is a two frame mosaic.
There seems to be some interesting looking structures in this emission nebula. One of them can be seen at bottom right, just under the larger nebula. It looks like some kind of circular formation with several dim concentric layers. An other one is a very small area emitting light from an ionized oxygen (O-III) at center of the Sh2-232 at right.
Sharpless objects 232, 231, 233 and 235
Image is a two frame mosaic, click for a large image
Image is in mapped colors from an emission of the ionized elements. Golden areas are from emission of sulfur and hydrogen. There is a very little an ionized oxygen, O-III, in there.
An experimental starless version
This starless image shows better the details of the actual nebula complex. (The blue dot is not a star)
A single frame closeup of Sharpless 232
Note the blue dot at middle of the photo, it's not a star but a small area of nebula emitting the O-III light.
A closeup of the blue dot at the middle
There is a small area of an ionized Oxygen (O-III) it can be seen as a blue dot at the center.
An animation
This animated GIF shows all three emission channels imaged for this photo, O-III, S-II and H-alpha.
The small nebula is visible in both, H-a and O-III, S-II doesn't show it. It could be nice to understand the mechanism behind this small object. Is it part of the large nebula and what is the energy source for the ionization? Has anyone else noticed this object? Let me know, if you have some info about it.
EDIT
INFO
Sharpless 232 (Sh2-232) large and very faint member of coplex of diffused nebulae in Auriga. One frame photo covers about a square degrees of sky. Panorama spans about 1,5 degrees horizontally. There are generally very little information about this group of nebulae.
Photo in visual colors
Click for a large image
The Sh2-232 in visual colors
Orientation in wide field mosaic of the Auriga
The are of interest is marked as a white rectangle. More info about this wide field photo can be found HERE
Technical details
Processing work flow
Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack2.
Deconvolution with a CCDStack2 Positive Constraint, 33 iterations, added at 50% weight
Color combine in PS CS3
Levels and curves in PS CS3.
Imaging optics
Celestron Edge HD 1100 @ f7 with 0,7 focal reducer for Edge HD 1100 telescope
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x2
Astrodon filter, 5nm H-alpha
Astrodon filter, 3nm O-III
Astrodon filter, 3nm S-II
Exposure times
H-alpha, 60 x 1200s = 20h
O-III, 6 x 1200s = 2h min.
S-II, 6x1200s = 2h min.
Total 24h
A single un cropped, calibrated and stretched 20 min. H-alpha frame as it comes from the camera
Another interesting feature of Sh2-232
A ring like formation
I have animated to this starless version of Sh2-232 photo, what I'm seeing in lower part of the nebula. There is a ring like formation and I'm seeing some hints of the concentric structure too.
Sunday, March 22, 2015
Messier 13, the Great Globular Cluster in Hercules
The season is about to end up here 65N for about six months. We have had clear skies for a couple of weeks now and I have lots of new material to publish in near future.
Messier 13 is a kind of fast project shot between dimmer targets. My location is not ideal for a broadband targets, like galaxies and clusters, due to massive light pollution. How ever, this is my try with a M13.
Messier 13
Click for a much large image
LRGB photo of the Great Globular Cluster in Hercules. Note. galaxy NGC 6207 at a lower left corner.
Click for a much large image
INFO
M13 locates in constellation Hercules at a distance of 25000 light years. The Great Globular Cluster in Hercules is one of the most brightest globular star clusters in northern sky. Stars are backed to a spherical formation with a diameter of about 150 light years.
Technical details
Processing work flow
Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack2.
Deconvolution with a CCDStack2 Positive Constraint, 33 iterations, added at 50% weight
Color combine in PS CS3
Levels and curves in PS CS3.
Imaging optics
Celestron Edge HD 1100 @ f7 with 0,7 focal reducer for Edge HD 1100 telescope
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x2
Custom Scientific LRGB 50mm Square Filters
Exposure times
Luminance, 14 x 600s = 2h 20min
Red, 6 x 200s binned 2x2 = 20 min.
Green, 6 x 200s binned 2x2= 20 min.
Blue, 6 x 200s binned 2x2 = 20 min
Total 3h 20min
Thursday, March 19, 2015
NGC 2174, the Monkey Head Nebula, project finalized
This photo shows more about this nebula, than I have used to see in any images taken with the same detail level. I haven't been aware of the curved dimmer areas at lower part of my photo.
NGC 2175
Click for a large image
are from emission of sulfur and hydrogen, bluish hues are from ionized oxygen.
A large version
Click for a 1800x1400 pixels, 1,3MB
Fancy a burger?
NGC 2174 in visual colors
INFO
NGC 2174, also known as a Monkey Head Nebula, locates at constellation Orion at distance of about 6400 light years. My photo shows about one square degrees of sky (The apparent size of the Moon is 0,5 degrees) The lower part of the photo shows a rarely imaged dimmer parts of the gas formation.
Image in H-alpha emission alone
Technical details
Processing work flow
Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack2.
Deconvolution with a CCDStack2 Positive Constraint, 33 iterations, added at 50% weight
Color combine in PS CS3
Levels and curves in PS CS3.
Imaging optics
Celestron Edge HD 1100 @ f7 with 0,7 focal reducer for Edge HD 1100 telescope
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x2
Astrodon filter, 5nm H-alpha
Astrodon filter, 3nm O-III
Astrodon filter, 3nm S-II
Exposure times
H-alpha, 16 x 1200s = 5h
O-III, 6 x 1200s = 2h min.
S-II, 6x1200s = 2h min.
Total 9h
A single un cropped, calibrated and stretched 20 min. H-alpha frame as it comes from the camera
Wednesday, March 11, 2015
A start of the new imaging project, NGC 2174, the "Monkey Head Nebula"
At March 9 I managed to exposure about four hours of H-alpha light for NGC 2147.
I'll shoot more exposures for this soon to have more signal and colors.
There seems to be some rarely imaged faint looped shapes at bottom of the object, I haven't seen them before.
NGC 2174, the Monkey Head Nebula in Orion
A starless version
An inverted image to show the bottom filaments better
Monday, March 9, 2015
The heart of the Heart nebula, melotte 15
A new photo from the night of 20. February and 6, March, Melotte 15 in the IC 1805, the Heart nebula.
Melotte 15
Click for a large image
Image is in mapped colors from an emission of the ionized elements. Golden areas
are from emission of sulfur and hydrogen, bluish hues are from ionized oxygen.
And even closer
INFO
An experimental starless image
Click for a large image
This experimental starless photo shows the object in light of an ionized hydrogen alone.
Image in visual colors
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.
Melotte 15
Click for a large image
are from emission of sulfur and hydrogen, bluish hues are from ionized oxygen.
A closeup
Click for a large image
A closer closeup
Click for a large image
And even closer
INFO
The open cluster centered in this image is known as Melotte 15 . Melotte 15 is embedded within a central portion of the much larger glowing nebula identified as IC 1805.
The interesting structure in the image is a giant area of ionized hydrogen, it's caused to glow by the intense ultraviolet radiation from the massive stars of the Melotte 15 star cluster.
Dust and gas clouds are twisted by the pressure of the intense radiation, the solar wind.
This formation is estimated to be 7,500 light years away from Earth, North is up.
An experimental starless image
Click for a large image
Image in visual colors
Orientation in an older wide field image of the area
The Heart and Soul nebulae, IC 1848 and 1805, in constellation Cassiopeia. Area of interest is marked as a white rectangle.
Technical details
Processing workflow
Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack2.
Deconvolution with a CCDStack2 Positive Constraint, 27 iterations, added at 50% weight
Color combine in PS CS3
Levels and curves in PS CS3.
Imaging optics
Celestron Edge HD 1100 @ f7 with 0,7 focal reducer for Edge HD 1100 telescope
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x2
Astrodon filter, 5nm H-alpha
Exposure times
H-alpha, 12 x 1200s = 4h
O-III and S-II channels are from an older wide field photo of this area.
A single un cropped, calibrated and stretched 20 min. H-alpha frame as it comes from the camera
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