Sunday, July 30, 2023

Emission Nebula Sh2-140 (LBN 505)

Sh2-140 is a hydrogen emission nebula located approximately 3,000 light-years away on the edge of a ring of molecular gas and dust known as the Cepheus Ring. From what I can tell in the literature, Sh2-140, refers to the more dense star forming the bottom edge of the nebular complex while LBN 505 is the nebula as a whole. Larger telescopes can reveal some of the star formation detail in the Sh2-140 region especially using IR filters.

There are many other objects in this field such as reflection nebulae, a star cluster, and colorful stars. The bright yellow star on the right is known as 25 Cep (25 brightest star in Cepheus). Up near the top the bright blue star has some blue reflection which also seems to be associated with an emission nebula, LBN 500. On the lower right side of the image there is another blue reflection nebula named vdB 153 which is adjacent to reflection nebula LBN 508.


Sh2-140 (LBN 505)
Dates: 6-29-23, 7-6, 7-10, 7-11
Camera: ZWO ASI1600MM-Pro
Telescope: Astro-Tech AT115EDT 115mm Refractor Telescope
Barlow: None
Focal Length: 805mm (644mm w/ FR)
f/7
Focal Reducer: 0.8x AstroTech Field Flatterner/Focal Reducer
Mount: Orion Sirius
Filter Wheel: ZWO
EFW 8 x 1.25"
Filter: Antlia Ha, ZWO L, R, G, B
Focuser: ZWO EAF
Autoguiding: ASI120 Mini attached to an Agena 50mm Guide Scope/ZWO 60mm Guidescope
Exposure: Ha 79 x 300, L 87 x 90, R 69 x 90, G 62 x 90, B 68 x 90
Gain: 139
Offset 20
Sensor Temp: 0 C
Processing: NINA, PixInsight, Photoshop, BlurXTerminator, StarXTerminator, NoiseXTerminator, Bill Blanshan Masks.

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Sunday, July 16, 2023

Tarantula Nebula & NGC 2070 from CT?

The Tarantula Nebula, also known as 30 Doradus, is an immense hydrogen emission nebula in the Large Magellanic Cloud - a satellite galaxy to the Milky Way approximately 160,000 light-years away. NGC 2070 is a star cluster located in the center of the Tarantula Nebula and provides the energy to ionize the nebula. It is estimated to be 550 LY across and is so bright if it were where the Orion Nebula, the Tarantula, would cast shadows at night. It also happens to be the largest emission nebula in the Local Group of galaxies of which the Milky Way is part of.

For those not in the know, the Tarantula is only visible below 21 degrees north latitude so it is best seen from the Southern Hemisphere. In order to produce this image I used data from Slooh Online Telescopes for Educators (https://www.slooh.com/). Slooh has graciously given our high school a trial year to use their astronomy curriculum which includes their telescopes. What Slooh is NOT is a remote astrophotography observatory like Deep Sky West or Chilescope which is devoted to astrophotography pursuits, rather Slooh is strictly for educational purposes and scientific research.

It is a really ingenious way to learn about astronomy. The way is works is a student or family member (if you get a family membership) will be assigned a quest where they would learn all about a planet, moon, the sun, a star cluster, galaxy, or etc. and as part of the 'Quest' they would have to go on a 'Mission' where they would schedule time on a telescope to image the phenomena - if they are awake they see it acquiring data live. When it is complete, a pretty decent image is produced by a program and saved as a '.png' file. Slooh as of this writing has professional grade equipment in Chile and the Canary Islands so the entire night sky is doable. Chile has two telescopes available and the Canary Islands has four night time telescopes and a fifth solar telescope.

I made a video using Slooh - link (https://www.youtube.com/watch?v=-WTz-uj-sVQ)

The reason it is not good for straight astrophotography purposes is you can only go on one mission (schedule time - 10 min) at a time. Also, you have no control over the exposure time, it is predetermined based on the object. For my image of the Tarantula, the 27 stacked sessions (missions) consisted 20 seconds for RGB band and 50 seconds for luminosity (i.e. each session was 110 seconds). In addition, I have no idea if flats, darks, or bias were even collected but if they were I did not see any of that data.

I scheduled sessions (missions) over 2-month period from March to May using the Chile Two Wide-field Telescope which consists of the following equipment:

Telescope: Planewave CDK17 ($22,500)

Camera: FLI Proline PL16803 Monochrome CCD Camera with 63.5mm Shutter ($12,900)

Filter Wheel: FLI FL-CL1-10 CenterLine Ten Position Filter Wheel ($3,900)

Filters: Astrodon Photometric Johnson/Cousins Filters (50mm) ($660)

Mount: Paramount MEII ($20,000)

You can see from the prices which I included just for giggles that Slooh is using top of the line equipment. I do know people that have this kind of equipment but for most backyard astrophotographers it is not feasible. I managed to collect 32 LRGB sessions over that time period but only used 27 of the best sessions after running it through Subframe Selector. The rest of the processing was straightforward - what I would normally do. As expected I was able to bring out more of the faint nebulosity with the stacked 27 frames than the single frame. Interestingly the stacked image was more red than the single processed frame which was more purple.

I am pretty happy with how it turned out especially for such a short total exposure (49 min. total LRGB). It shows what can be accomplished with bortle 1 skies. I don't know if I will do it anymore as I prefer to collect my data with my own equipment but it was really fun to do. I have always wanted to see and image the Magellanic Clouds and some of the other goodies down south so this is a good consultation prize.

Figure 1 - My Processed Image (27 sessions)



Figure 2 - Slooh Processed Image, same crop (1 session)


Figure 3 - Slooh Processed Image, original field of view (1 session)

Tarantula Nebula & NGC 2070 from CT?
Dates: 3-5-23 ... 5-16-23
Camera: FLI Proline PL16803 Monochrome CCD
Telescope: Planewave CDK17
Barlow: None
Focal Length: 2938mm (native)
F/6.8
Focal Reducer: none?
Mount: Paramount MEII
Filter Adaptor: none?
Filters: Astrodon Photometric Johnson/Cousins Filters
Focuser: FingerLakes?
Autoguiding: none ?
Exposure: Lum 27 x 50, RGB 27 x 20
Gain: ?
Offset ?
Temp: ? 
Processing: PixInsight, Photoshop, BlurXT, NoiseXT, StarX, GradientXT, Bill's Colormasks

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Monday, July 10, 2023

Late to the Supernova Party - M101 (Pinwheel Galaxy)

If you are not in the astro community you may not know that a supernova was discovered in M101, a.k.a. The Pinwheel Galaxy, on May 19 by an amateur astronomer, Koichi Itagaki. Designated as 2023ixf the supernova happens to be the closest to to Earth in a decade and should still be visible through the summer. There have been hundreds of fine images of this galaxy posted over the last month so my image is a bit late. Ironically I started imaging this in May not realizing there was an active supernova - my last image of this was from 2017 when my skills were very low. Although it was finished in mid June, I only now had time to processed it.

Located in Ursa Major approximately 21 million light-years from us M101 is an immense face-on spiral galaxy 170,000 LY across containing over a trillion stars. The outer arms consist of young, hot, blue star clusters that appear as 'knots' on my image. Also, very large pink-red clouds composed of molecular hydrogen are scattered throughout the arms. These nebular regions are large enough to have their own NGC designation and are home to intense star formation. My favorites include the NGC 5450 on the lower right, NGC 5471 to the left of the leftmost outer arm, NGC 5462 on the left outer arm, and NGC 5461 just below NGC 5462. The very large star adjacent to NGC 5461 is the supernova (SN 2023ixf). A dwarf galaxy, NGC 5477, is located on the far left side of the image.

I captured this over several nights trying to avoid crappy weather and smoke from the wildfires as best I could - a lot of collected data was not used. In addition to capturing natural color with my ASI294MC I decided to capture some Ha data using the IDAS NBZ filter. I separated the NBZ data into RGB channels using the red data since that is where the hydrogen wavelength would fall - of course using a monochrome camera with narrow pass Ha filter would be the optimal way to collect the Ha data.

Dates: 5-26-23, 5-27, 5-28, 5-29, 6-4, 6-10



Late to the Supernova Party - M101 (Pinwheel Galaxy) 
Dates: 5-26-23, 5-27, 5-28, 5-29, 6-4, 6-10
Camera: ZWO ASI294MC-Pro
Telescope: Celestron EdgeHD 800
Barlow: None
Focal Length: 2032mm (native), 1400mm
F/10 (native), F/7
Focal Reducer: Celestron 0.7 Reducer Lens
Mount: Orion Atlas Pro
Filter Adaptor: ZWO Filter Drawer
Filter: Optolong Luminosity, IDAS NBZ
Focuser: ZWO EAF
Autoguiding: ASI120 Mini attached to an Orion ST80
Exposure: Lum 257 x 90, NBZ 126 x 180 
Gain: 139
Offset 0
Temp: 0 C
Processing: Asiair app, PixInsight, Photoshop, BlurXT, NoiseXT, StarX, Bill's Colormasks

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Saturday, July 1, 2023

NGC 5364 & NGC 5363 Galaxy Group

The most prominent object in this image is the beautiful nearly face-on spiral galaxy NGC 5364 (a.k.a. NGC 5317) located in Virgo. William Herschel originally discovered it, however, his son John Herschel rediscovered and labeled it NGC 5317. Approximately 52 million light-years (LY) away it is reported to be about 93,000 LY in diameter. It seems to have an asymmetric galactic bulge and spiral arms which is attributed to interactions with the dwarf galaxy NGC 5360 located above NGC 5364 in my image.

The other major galaxy in this image is the lenticular galaxy NGC 5363. It has a well developed bulge and a diffuse galactic disk. It is approximately 57 million LY away and about 5 million LY distant from NGC 5364, so there is probably no tidal interaction between the two.

I purposely did not center this on the two prominent members as there are other midsized goodies in this image that I wanted to show such as NGC 5356, NGC 5348, and UGC 8818. I really like the structure of UGC 8818 which is 250 million LY away and 39,000 LY in diameter. There are numerous other objects visible in this image including far away galaxies and a quasars.

Typically images taken in the northern hemisphere are oriented with North at the top, however, this is oriented as it would appear taken from the southern hemisphere because I liked the way it looked. Also, this image is cropped quite a bit so I have a link to the full frame image with even more faint fuzzies (https://www.smugmug.com/app/organize/Galaxies/i-QnSTcZC).

cropped image

full frame image

NGC 5364 & NGC 5363 Galaxy Group
Dates: 5-18-23, 5-19, 5-23, 5-26, 5-27
Camera: ZWO ASI1600MM-Pro
Telescope: Astro-Tech AT115EDT 115mm Refractor Telescope
Barlow: None
Focal Length: 805mm (644mm w/ FR)
f/7
Focal Reducer: 0.8x AstroTech Field Flatterner/Focal Reducer
Mount: Orion Sirius
Filter Wheel: ZWO
EFW 8 x 1.25"
Filter: None, ZWO R, G, B
Focuser: ZWO EAF
Autoguiding: ASI120 Mini attached to an Agena 50mm Guide Scope/ZWO 60mm Guidescope
Exposure: None 112 x 90, R 71 x 90, G 67 x 90, B 52 x 90
Gain: 139
Offset 20
Sensor Temp: 0 C
Processing: NINA, PixInsight, Photoshop, BlurXTerminator, StarXTerminator, NoiseXTerminator, Bill Blanshan Masks.

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