Tuesday, March 3, 2020
"Two ways to die", an alternative composition
One of the dimmest targets I have ever shot. The supernova remnant Simeis 147 is large and dim but this nebula pair in Auriga is much dimmer. There are very few images about this target around. Photo is taken with Tokina AT-x 300mm f2.8 camera lens and Apogee Alta U16 astro camera.
This is an alternative vertical composition, the horizontal composition can be seen here, https://astroanarchy.blogspot.com/2020/03/two-ways-to-die-sh2-216-sh2-221.html
I think this vertica version is little more dynamic as a composition.
Supernova remnant and a planetary nebula in the same field of view
Click for a large photo
Photo is in mapped colors from the emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen. Image spans vertically about six degrees, (That's equal to 12 full Moons side by side in the sky.) The planetary Nebula Sharpless 216 at top and the supernova remnant Sharpless 221 lays at bottom.
H-alpha, 36 x 1200 s, binned 1x1 = 12 h
O-III, 33 x 1200 s, binned 2x2 = 11 h
S-II, 9 x 1200 s. binned 2x2 = 3 h
INFO
Sh2-216, the closest planetary nebula to earth ever discovered.
Image spans about six degrees horizontally, at left lays the large and very dim planetary nebula Sharpless 216 (aka Simeis 288, Marsalkova 44, LBN 742, GN 04.41.3)
This planetary nebula is the closest known planetary nebula to Earth, about 390 light years, and also one of the oldest known. Due the old age, it's very diffused, dim and large, apparent diameter is about 1,6 degrees. (Full Moon is about 0,5 degrees wide)
Supernova remnant Sh2-221
At right side of the photo lays a dim nad diffused supernova remnant Sh2-221 (SNR G160.4+02.8, HB9) it locates in constellation Auriga, about one degree West from star Capella. (Doesn't show in my image) The distance from the Earth, 2600 light years, is determined recently at 2007. This object was recognized as a supernova remnant back at seventies.
Technical details
Processing workflow
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
Tokina AT-x f2.8 camera lens
Mount
10-micron 1000
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and an old spotting scope of Meade LX200
Astrodon filters,
5nm H-alpha 3nm S-II and 3nm O-III
5nm H-alpha 3nm S-II and 3nm O-III
Total exposure time 26h
H-alpha, 36 x 1200 s, binned 1x1 = 12 h
O-III, 33 x 1200 s, binned 2x2 = 11 h
S-II, 9 x 1200 s. binned 2x2 = 3 h
Monday, March 2, 2020
Supernova remnant IC 443 wide field
The imaging season up here 65N will end in a month since we are rapidly running out of darkness. I spend last Friday night with the Jellyfish nebula, IC 443, in Gemini.
The current imaging system takes me deep very fast, Tokina AT-x 300mm f2.8 camera lens, Astrodon narrowband filters and Apogee Alta U16 camera. This combination has turned to be a very nice imaging tool inteed.
IC 443, NGC 2175 & Messier 35
Click for a large image, it's worth it!
Mapped colors from the emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen.
A star cluster Messier 35 at upper right, IC 443 at middle left and NGC 2175 at lower right.
H-alpha alone
Click for a large image
3h of light emitted by an ionized hydrogen, H-alpha.
INFO
Source Wikipedia, http://en.wikipedia.org/wiki/IC_443
A star cluster Messier 35 at upper right, IC 443 at middle left and NGC 2175 at lower right.
H-alpha alone
Click for a large image
INFO
One of the reasons i took this image is the "Monkey head nebula", NGC 2175, at lower right corner.
I have shot this area with a much longer focal length back in 2015. At my image there is a very faint extended shape visible in my photo. I wanted to see, if I'm able to catch it with my current imaging system as well. This very dim feature is strongly visible in my new photo too! (Monkey head nebula is rotated 180 degrees in large image below.)
Older long focal length photo of NGC 2175 from Spring season 2015, more info here, https://astroanarchy.blogspot.com/2015/03/ngc-2174-monkey-head-nebula-project.html
IC 443
IC 443 (also known as the Jellyfish Nebula and Sharpless 248 (Sh2-248)) is a Galactic supernova remnant (SNR) in the constellation Gemini. It locates visually near the star Eta Geminorum at distance of about 5000 light years.
IC 443 may be the remains of a supernova that occurred 3,000 - 30,000 years ago. The same supernova event likely created the neutron star CXOU J061705.3+222127, the collapsed remnant of the stellar core. IC 443 is one of the best-studied cases of supernova remnants interacting with surrounding molecular clouds
IC 443 may be the remains of a supernova that occurred 3,000 - 30,000 years ago. The same supernova event likely created the neutron star CXOU J061705.3+222127, the collapsed remnant of the stellar core. IC 443 is one of the best-studied cases of supernova remnants interacting with surrounding molecular clouds
Source Wikipedia, http://en.wikipedia.org/wiki/IC_443
Technical details
Processing workflow
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
Tokina AT-x f2.8 camera lens
Mount
10-micron 1000
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and an old spotting scope of Meade LX200
Astrodon filters,
5nm H-alpha 3nm S-II and 3nm O-III
Total exposure time
H-alpha, 9 x 1200 s, binned 1x1 = 3 h
O-III, 3 x 1200 s, binned 2x2 = 1 h
S-II, 3 x 1200 s. binned 2x2 = 1 h
O-III, 3 x 1200 s, binned 2x2 = 1 h
S-II, 3 x 1200 s. binned 2x2 = 1 h
Sunday, March 1, 2020
Two ways to die, Sh2-216 & Sh2-221, Supernova remnant and a planetary nebula
This must be one of the dimmest targets I have shot. The supernova remnant Simeis 147 is large and dim but this nebula pair in Auriga is much dimmer. There are very few images about this target around. Photo is taken with Tokina AT-x 300mm f2.8 camera lens and Apogee Alta U16 astro camera.
Supernova remnant and a planetary nebula in the same field of view
Click for a large photo, it's worth it!
NOTE, the apparent size of the Full Moon is marked at lower left corner.
INFO
Sh2-216, the closest planetary nebula to earth ever discovered.
Image spans about six degrees horizontally, at left lays the large and very dim planetary nebula Sharpless 216 (aka Simeis 288, Marsalkova 44, LBN 742, GN 04.41.3)
This planetary nebula is the closest known planetary nebula to Earth, about 390 light years, and also one of the oldest known. Due the old age, it's very diffused, dim and large, apparent diameter is about 1,6 degrees. (Full Moon is about 0,5 degrees wide)
Supernova remnant Sh2-221
At right side of the photo lays a dim nad diffused supernova remnant Sh2-221 (SNR G160.4+02.8, HB9) it locates in constellation Auriga, about one degree West from star Capella. (Doesn't show in my image) The distance from the Earth, 2600 light years, is determined recently at 2007. This object was recognized as a supernova remnant back at seventies.
H-alpha image with labels
Click for a large photo
Technical details
Processing workflow
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
Tokina AT-x f2.8 camera lens
Mount
10-micron 1000
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and an old spotting scope of Meade LX200
Astrodon filters,
5nm H-alpha 3nm S-II and 3nm O-III
5nm H-alpha 3nm S-II and 3nm O-III
Total exposure time 26h
H-alpha, 36 x 1200 s, binned 1x1 = 12 h
O-III, 33 x 1200 s, binned 2x2 = 11 h
S-II, 9 x 1200 s. binned 2x2 = 3 h
Orientation in Auriga
Sunday, February 23, 2020
Cederblad 214, the Cosmic Question mark in visual colors
This photo was taken with my "new" imaging system. I managed to mate an old Tokina AT-x 300mm f2.8 camera optics with the Apogee Alta U16 astro camera and filter wheel. Some angle grinder was needed to have enough back focus... More info here, https://astroanarchy.blogspot.com/2020/01/the-frankenstein-monster-my-current.html
This photo of Cosmic Question Mark has a great symbolic value for me. The cosmic curiosity is the very reason I'm doing this difficult, and sometimes frustrating, form of nature photographing.
Cederblad 214 and Sharpless 170, " ? "
Please, click for a full size image
A two panel mosaic panorama to SNR CTB1
Please, click for a full size image
INFO
This cosmic question mark, in constellation Cepheus, contains following objects; At top, Cederblad 214(Ced 214) surrounded by NGC 7822, a dot like nebula at the bottom is known as Sharpless 170,(Sh2-170). Image spans over Five degrees vertically. Distance from my observatory, is ~2750 light years and it spans about 40 light years.
Orientation in the sky
Technical details
Processing workflow
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
Tokina AT-x f2.8 camera lens
Mount
10-micron 1000
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and an old spotting scope of Meade LX200
Astrodon filters,
5nm H-alpha 3nm S-II and 3nm O-III
5nm H-alpha 3nm S-II and 3nm O-III
Total exposure time
H-alpha, 12 x 1200 s, binned 1x1 = 4 h
O-III, 1x 1200 s, binned 2x2 = 20 min.
S-II, 1 x 1200 s. binned 2x2 = 20 min.
Saturday, February 22, 2020
Simeis 147 (Sh2-240), a large supernova remnant in visual colors
Simeis 147 is a difficult target due to a low surface brightness and a very large angular diameter.
Yesterday I published a mapped color version of this supernova remnant. This time I have composed the narrowband channels to a visual palette. Ionized hydrogen, H-alpha emits deep red light. Since the hydrogen is the most common element in our universum, red is dominating the view. There are some very dim bluish hues from a light of an ionized oxygen, O-III.
I collected the data for this image between 27.12.2019 and 19.02.2020.
Simeis 147 (Sharpless 240)
Click for a large image it's worth it!
Note, the relative size of a full Moon is marked as a white circle at bottom left, this is a large object!
Red light from an ionized hydrogen is dominating the view.
An experimental starless version
Click for a large image
The starless version Complex filaments are easier to see in this experimental starless image.
INFO
Red light from an ionized hydrogen is dominating the view.
An experimental starless version
Click for a large image
INFO
Simeis 147 (sharpless 240), is a very faint and large supernova remnant in constellation Taurus at distance of ~3000 light years. It's constantly expanding at speed of 1000 km/second but due the size of it, we can't see any movement in it. This SN spans over 160 light years and the apparent scale in the sky is about three degrees (Moon has an apparent size of 30" = 0,5 degrees). Explosion took place approximately 30.000 years ago and left behind a pulsar (Neutron star). The pulsar has recently identified.
How long it'll takes to this supernova remnant to expand 1% large when the diameter is 160 light years and it expands at speed of 1000km/second.
How long it'll takes to this supernova remnant to expand 1% large when the diameter is 160 light years and it expands at speed of 1000km/second.
Answer is ~480 years.
(1% of diameter 160/100= 16, as kilometers ~151.372.800.000.00, = Y, km,
1000km/second is ~315.360.000.00, = Z, kilometers/year.
So, X x Z = Y and X=Z/Y, X = 480 with given values)
(1% of diameter 160/100= 16, as kilometers ~151.372.800.000.00, = Y, km,
1000km/second is ~315.360.000.00, = Z, kilometers/year.
So, X x Z = Y and X=Z/Y, X = 480 with given values)
Technical details
Processing workflow
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
Mount
10-micron 1000
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and an old spotting scope of Meade LX200
Astrodon filters,
5nm H-alpha 3nm S-II and 3nm O-III
Total exposure time
H-alpha, 15 x 1200 s, binned 1x1 = 5 h
O-III, 24x 600 s, binned 2x2 = 4 h
S-II, 1 x 12 x 600 s. binned 2x2 = 2 h
Friday, February 21, 2020
Simeis 147 (Sh2-240), a large supernova remnant in Taurus
I collected the data for this image between 27.12.2019 and 19.02.2020.
Simeis 147 (Sharpless 240)
Click for a large image
Note, the relative size of a full Moon is marked as a white circle at bottom left, this is a large object!
Image is in mapped colors, from the emission of ionized elements, R=Sulphur, G=Hydrogen and B=Oxygen.
INFO
INFO
Simeis 147 (sharpless 240), is a very faint and large supernova remnant in constellation Taurus at distance of ~3000 light years. It's constantly expanding at speed of 1000 km/second but due the size of it, we can't see any movement in it. This SN spans over 160 light years and the apparent scale in the sky is about three degrees (Moon has an apparent size of 30" = 0,5 degrees). Explosion took place approximately 30.000 years ago and left behind a pulsar (Neutron star). The pulsar has recently identified.
How long it'll takes to this supernova remnant to expand 1% large when the diameter is 160 light years and it expands at speed of 1000km/second.
How long it'll takes to this supernova remnant to expand 1% large when the diameter is 160 light years and it expands at speed of 1000km/second.
Answer is ~480 years.
(1% of diameter 160/100= 16, as kilometers ~151.372.800.000.00, = Y, km,
1000km/second is ~315.360.000.00, = Z, kilometers/year.
So, X x Z = Y and X=Z/Y, X = 480 with given values)
(1% of diameter 160/100= 16, as kilometers ~151.372.800.000.00, = Y, km,
1000km/second is ~315.360.000.00, = Z, kilometers/year.
So, X x Z = Y and X=Z/Y, X = 480 with given values)
Technical details
Processing workflow
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
Mount
10-micron 1000
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and an old spotting scope of Meade LX200
Astrodon filters,
5nm H-alpha 3nm S-II and 3nm O-III
Total exposure time
H-alpha, 15 x 1200 s, binned 1x1 = 5 h
O-III, 24x 600 s, binned 2x2 = 4 h
S-II, 1 x 12 x 600 s. binned 2x2 = 2 h
Sunday, February 16, 2020
Panorama mosaic, Cederblad 214, Sharpless 170 and supernova remnant CTB1
his morning I published the photo of supernova remnant CTB1 (Abell 85). Photos are overlapping, so I was able to build a mosaic image out of them. image spans about ten degrees of sky vertically, that's as large as twenty full Moons side by side.! (The CTB1 at lower center has a same angular diameter as our Moon.) Photo is taken with the Tokina AT-x 300mm f2.8 camera lens, Apogee Alta U16 astro camera and Astrodon narrowband filters. Info about my current setup here, https://astroanarchy.blogspot.com/2020/01/the-frankenstein-monster-my-current.html
A two frame mosaic panorama from constellation Cassiopeia
Click for a large image, it's worth it!
mage is in mapped colours, from the emission of ionized elements, R=Sulphur, G=Hydrogen and B=Oxygen.
Upper part of the mosaic image
Click for a large image
Image details here, https://astroanarchy.blogspot.com/2020/02/new-photo-of-cederblad-214-cosmic.html
Lower part of the mosaic image Click for a large image
Image details here, https://astroanarchy.blogspot.com/2020/02/ctb1-supernova-remnant-in-cassiopeia.html
Upper part of the mosaic image
Click for a large image
Image details here, https://astroanarchy.blogspot.com/2020/02/new-photo-of-cederblad-214-cosmic.html
Lower part of the mosaic image Click for a large image
Technical details
Click for a large image
Processing workflow
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
Tokina AT-x f2.8 camera lens
Mount
10-micron 1000
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and an old spotting scope of Meade LX200
Astrodon filters,
5nm H-alpha 3nm S-II and 3nm O-III
Total exposure time for both panels
H-alpha, 21 x 1200 s, binned 1x1 = 7 h
O-III, 2x 1200 s, binned 2x2 = 40 min.
S-II, 2 x 1200 s. binned 2x2 = 40 min.
Click for a large image
Processing workflow
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
Tokina AT-x f2.8 camera lens
Mount
10-micron 1000
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and an old spotting scope of Meade LX200
Astrodon filters,
5nm H-alpha 3nm S-II and 3nm O-III
Total exposure time for both panels
H-alpha, 21 x 1200 s, binned 1x1 = 7 h
O-III, 2x 1200 s, binned 2x2 = 40 min.
S-II, 2 x 1200 s. binned 2x2 = 40 min.
An older longer focal length image of CTB1 from 2016
Please, click for a large image
Please, click for a large image
More info about this photo here, https://astroanarchy.blogspot.com/2016/01/abell-85-ctb1-dim-galactic-supernova.html
An older longer focal length image of Cederblad 214 from 2016
Please, click for a large image
An older longer focal length image of Cederblad 214 from 2016
Please, click for a large image
A detail shot from the bright central region of the image at the top. This photo was taken with my new setup, Celestron Edge HD 1100 f7, Apogee Alta U16 astro camera and the Astrodon narrowband filters, Spring 2014. The original blog post from 2012, with technical details, can be seen HERE
CTB1, a supernova remnant in Cassiopeia
CTB1 (Abell 85)
Please, click for a large image, it's worth it.
A closer look
Please, click for a large image
An older longer focal length image back from 2016
Please, click for a large image
More info about this photo here, https://astroanarchy.blogspot.com/2016/01/abell-85-ctb1-dim-galactic-supernova.html
INFO
Abell 85 is a very faint supernova remnant in constellation Cassiopeia. It's difficult to image with any details due to extremely low surface brightness. Abell 85 has a largish diameter, about half a degree, it has a same apparent diameter as a full Moon. The physical diameter is about 98 light years across. This SNR locates about 9800 light years from the Earth. CTB1 was originally thought to be a planetary nebula and it was included the Abell catalog of planetary nebulae under a name Abell 85. It was confirmed to be a supernova remnant by Willis & Dickel at 1971.
Technical details
Processing workflow
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
Tokina AT-x f2.8 camera lens
Mount
10-micron 1000
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and an old spotting scope of Meade LX200
Astrodon filters,
5nm H-alpha 3nm S-II and 3nm O-III
Total exposure time
H-alpha, 9 x 1200 s, binned 1x1 = 3 h
O-III, 1x 1200 s, binned 2x2 = 20 min.
S-II, 1 x 1200 s. binned 2x2 = 20 min.
INFO
Abell 85 is a very faint supernova remnant in constellation Cassiopeia. It's difficult to image with any details due to extremely low surface brightness. Abell 85 has a largish diameter, about half a degree, it has a same apparent diameter as a full Moon. The physical diameter is about 98 light years across. This SNR locates about 9800 light years from the Earth. CTB1 was originally thought to be a planetary nebula and it was included the Abell catalog of planetary nebulae under a name Abell 85. It was confirmed to be a supernova remnant by Willis & Dickel at 1971.
Technical details
Processing workflow
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
Tokina AT-x f2.8 camera lens
Mount
10-micron 1000
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and an old spotting scope of Meade LX200
Astrodon filters,
5nm H-alpha 3nm S-II and 3nm O-III
Total exposure time
H-alpha, 9 x 1200 s, binned 1x1 = 3 h
O-III, 1x 1200 s, binned 2x2 = 20 min.
S-II, 1 x 1200 s. binned 2x2 = 20 min.
A single calibrated and stretched 20 min. H-alpha frame as it comes from the camera (Downscaled)
Friday, February 14, 2020
Cosmic heart beats for the Valentine's Day
The Heart nebula
Monday, February 10, 2020
Cederblad 214, the Cosmic Question mark, in visual colors
This photo was taken with my "new" imaging system. I managed to mate an old Tokina AT-x 300mm f2.8 camera optics with the Apogee Alta U16 astro camera and filter wheel. Some angle grinder was needed to have enough back focus... More info here, https://astroanarchy.blogspot.com/2020/01/the-frankenstein-monster-my-current.html
This photo of Cosmic Question Mark has a great symbolic value for me. The cosmic curiosity is the very reason I'm doing this difficult, and sometimes frustrating, form of nature photographing.
" ? "
Cederblad 214 and Sharpless 170,
Please, click for a full size image
Visual palette combined from emissions of ionized elements. Red = hydrogen + 33% sulfur, Green = oxygen and Blue = oxygen + 20% hydrogen to compensate missing h-beta emission.
INFO
This cosmic question mark, in constellation Cepheus, contains following objects; At top, Cederblad 214(Ced 214) surrounded by NGC 7822, a dot like nebula at the bottom is known as Sharpless 170,(Sh2-170). Image spans over Five degrees vertically. Distance from my observatory, is ~2750 light years and it spans about 40 light years.
Orientation in the sky
Cederblad 214 can be seen at upper left corner. Image shows its location related to constellation Cepheus.
Technical details
Processing workflow
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
Tokina AT-x f2.8 camera lens
Mount
10-micron 1000
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and an old spotting scope of Meade LX200
Astrodon filters,
5nm H-alpha 3nm S-II and 3nm O-III
5nm H-alpha 3nm S-II and 3nm O-III
Total exposure time
H-alpha, 12 x 1200 s, binned 1x1 = 4 h
O-III, 1x 1200 s, binned 2x2 = 20 min.
S-II, 1 x 1200 s. binned 2x2 = 20 min.
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