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The Heart Nebula, IC 1805 is some 7500 light years away from Earth and is located in the Perseus Arm of the Galaxy in the constellation Cassiopeia. Processed in Hubble Palette.
Kind of reminded me of a deep space nebula shot!
Was torn between the shot for this week, flip-flopped between this and a high speed capture created by dropping coins into a shot glass of water, but ended up with this. It’s a cobweb on our outside tap that I misted with a water atomiser and lit with LED lights.
HMM!
Object: IC1805 – The Heart Nebula SHO (2022)
The Heart Nebula, IC 1805, Sh2-190, lies some 7500 light years away from Earth and is located in the Perseus arm of the Galaxy in the constellation Cassiopeia. This is an emission nebula composed of glowing gases (ionized hydrogen, sulfur and oxygen) and darker cold dust lanes. The nebula is shape and illumination are produced by a central star cluster known as Melotte 15 aka Collinder 26.
Details:
- Acquisition Date: 11/23/2022 to 11/24/2022
- Location: Western Massachusetts, USA
- Imaging Camera: QHY600PH-M -10°C - Mode 1(High Gain) Offset:15 Gain:56
- Telescope: Takahashi FSQ106 EDXIII @ f/5 (530mm focal length - 106mm aperture)
- Mount: Astro-Physics AP1100 w/GTO4
- Guide scope: Celestron Off Axis Guider
- Guide Camera: ASI174m mini
- Software: Adobe Photoshop CS5, Sequence Generator Pro, PixInsight 1.8 Ripley, Aries Astro Pixel Processor
Filters:
- Chroma Ha 3nm 50mm
- Chroma OIII 3nm 50mm
- Astrodon SII 3nm 50mm
Exposure Times:
- Hydrogen Alpha (Ha): 30 x 10min. (300min) bin 1x1
- Oxygen III (OIII):30 x 10min. (300min) bin 1x1
- Sulfur II (SII):25 x 10min. (250min) bin 1x1
Total Exposure:610min. (14.17hrs)
Sky Quality:
-Magnitude: 19.71
-Bortle Class 5
-1.41 mcd/m^2 Brightness
-1234.6 ucd/m^2 Artificial Brightness
Object: The Veil Nebula – Cygnus Loop SHO (2022)
The visual portion of the Cygnus Loop also known as the Veil Nebula, Cirrus Nebula or the Filamentary Nebula is located in the constellation Cygnus. The area includes the components:
-NGC6990 - “Western Veil" or "Witch's Broom",
-NGC6992 – NGC6995 – IC1340 - “Eastern Veil"
-Pickering's Wedge, or Pickering's Triangular Wisp.
The entire area is the remnant of a supernova explosion that occurred about 20.000 years ago and has been expanding ever since.
Distance from Earth: about 2400 light years
Details: The visual portion of the Cygnus Loop also known as the Veil Nebula, Cirrus Nebula or the Filamentary Nebula is located in the constellation Cygnus. The area includes the components: NGC6990, "Western Veil" or "Witch's Broom", NGC6992 "Eastern Veil", and Pickering's Wedge, or Pickering's Triangular Wisp.
The entire area is the remnant of a supernova explosion that occurred between 5000 to 8000 years ago and has been expanding ever since.
Distance from Earth: about 1470 light years
- Acquisition Date: 10/27/2022 to 11/20/2022
- Location: Western Massachusetts, USA
- Imaging Camera: QHY600PH-M -10°C - Mode 1(High Gain) Offset:15 Gain:56
- Telescope: Takahashi FSQ106EDXIII @ f/5 (530mm focal length - 106mm aperture)
- Mount: Astro-Physics AP1100 w/GTO4
- Guide scope: Celestron Off Axis Guider
- Guide Camera: ASI174m mini
- Software: Adobe Photoshop CS5, Sequence Generator Pro, PixInsight 1.8 Ripley, Aries Astro Pixel Processor
Filters:
- Chroma Ha 3nm 50mm
- Chroma OIII 3nm 50mm
- Astrodon SII 3nm 50mm
Exposure Times:
- Hydrogen Alpha (Ha): 25 x 10min. (250min) bin 1x1
- Oxygen III (OIII):20 x 10min. (200min) bin 1x1
- Sulfur II (SII):21 x 10min. (210min) bin 1x1
Total Exposure:660min. (11hrs)
Sky Quality:
-Magnitude: 19.71
-Bortle Class 5
-1.41 mcd/m^2 Brightness
-1234.6 ucd/m^2 Artificial Brightness
Original Artist Unknown
Edit © Ron Fleishman 2020
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#The #Worlds #Most #Colorful #Digital #Art
Messier 20 (M20, NGC 6514) in Sagittarius is a magnificent deep sky object that combines an open cluster of stars, an emission nebula (red), a reflection nebula (blue) and a dark nebula that divides the emission nebula in three parts, thus giving it the name the Trifid Nebula. The Trifid Nebula lies in a rich area of the Milky Way, with adjacent Messier objects M21 (open star cluster, at upper right) and M8 (Lagoon, a part of which is visible at the left edge) visible in the same binocular field of view. The region is also filled with other emission nebulae such as NGC 6526 (top left) and Sh2-26 (bottom left).
The Hubble and Spitzer Space Telescopes revealed hot, young energetic stars at the central region emitting radiation and stellar jets that tear apart the gas and dust from which stars are born.
M20 is estimated to be about 5200 light years away, at which it spans a diameter of about 10 light years across.
Clear Skies to all!
Image Details:
Telescope: Orion EON 80mm/f6.25 ED refractor
Camera: Canon EOS 20Da, no filter
Mount: Modified Vixen Sphinx (NexSXW)
Guiding: Skywatcher SynGuider with 80mm achromatic refractor, mounted side by side
Exposure: Total 16 mins (8 x 2 mins), Daylight WB, ISO 1600, calibrated with darks and bias frames
Location: Vavdos, Chalkidiki - 14/07/18
Processing: DSS 4.1.1, Photoshop CS6
(english follow)
Nebula / Nébuleuse
Carl Sagan, scientifique et auteur, soutenait dans Cosmos que l’homme « s’était attardé assez longtemps sur les rives de l’océan cosmique et qu’il était enfin prêt à partir vers les étoiles.»
Prêts à partir pour les étoiles? Il m’arrive de me demander ce qui arrivera lorsque notre espèce parviendra à rejoindre de lointaines planètes habitables.
Cet exploit sera t-il de nature à changer la culture humaine, la perspective qu’ont les humains sur eux-mêmes et sur les conflits et les peurs qui les animent ici sur ce grain de sable cosmique appelé Terre ou alors…. cette expansion aura t-elle simplement pour effet de transposer à une plus vaste échelle les conflits incessants qui nous opposent ici?
En regardant vers les étoiles, à partir de ma petite planète, je ne veux pas chercher une réponse à ces questions difficiles. L’émerveillement devant la beauté grandiose de cet univers de démesures me suffit. » (Patrice)
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Nebula
Carl Sagan, scientist, and author argued in "Cosmos" that man "have lingered long enough on the shores of the cosmic ocean. We are ready at last to set sail for the stars ».
Ready to go for the stars? I sometimes wonder what will happen when our species manages to reach distant habitable planets. . .
Will this feat be such as to change the human culture, the perspective that humans have on themselves and on the conflicts and fears that animate them here on this cosmic sandstone called Earth or so... will this expansion simply have the effect of transposing at a larger scale the continuing conflicts we have here?
Looking towards the stars, from my little planet, I don't want to seek an answer to these difficult questions. The wonder in front of the grandiose beauty of this universe of excessiveness is enough for me.
The Rosette Nebula.
Processed in the Hubble Palette, this vast emission nebula is located about 5200 light years from Earth.
83 x 5 min lights shot over 2 nights using a Williams Optics Z73 telescope and ZWO ASI533MC mounted on a Skywatcher EQ5 Pro.
The Horsehead Nebula is a small dark nebula in the constellation Orion. The nebula is located just to the south of Alnitak, the easternmost star of Orion's Belt, and is part of the much larger Orion molecular cloud complex
The Rosette nebula is an emission nebula in the Monoceros constellation, around 5200 light years from earth.
Image acquisition details:
36x300" HA
36x300" OIII
40x300" SII
B33 (Horsehead Nebula) is a dark nebula in the Orion constellation, around 1375 light years from earth.
Because emissions within this region/frame are mostly limited to HA and SII (tiny bit of OIII, but largely neglectable), I decided to see what I could do with only using that data. The reason why there's little OIII emissions in the region is fairly straightforward. Hydrogen (HA) and Sulfur (SII) quite simply have a much lower energy requirement for ionization (the processs that "triggers" these emissions) to take place compared to Oxygen (OIII). Due to there being a lot of dark dust (the whole reason we even see the horsehead) in the area; energy transmission is limited to the extent where there's enough for the former two elements to get ionized, not quite enough for (large amounts of) the latter.
Image acquisition details:
20x1800" HA
30x1800" SII
Used the typical HSS colour scheme and created a synthetic luminance layer on top to pull out a bit more detail. This layer consisted of a combined HA/SII signal, weighted down to include 33% of each.
Lagoon Nebula (M8) in the constellation Sagittarius.
One of the finest star-forming regions in the sky, faintly visible to the naked eye.
Image details:
Telescope: Orion EON 80mm/f6.25 ED refractor
Camera: Canon EOS 20Da, no filter
Mount: Vixen Sphinx (NexSXW)
Guiding: Skywatcher SynGuider/80mm refractor
Exposure: Total 14 mins, Daylight WB, ISO 1600, calibrated with darks, no flats
The Lagoon Nebula (also known as M8 or NGC 6523) is a giant interstellar cloud in the constellation Sagittarius, around 4,077 light-years from Earth, give or take.
This image was captured over two hours on an icy and dark night in outback NSW, Australia.
📷 Camera: ZWO ASI533 MC Pro
🔭 Scope: SkyWatcher Esprit 80
🌏 Mount: SkyWatcher EQ6-R Pro
📷 Guide Camera: ZWO ASI120MM
🔭 Guide Scope: Orion 50
🔥 Blanket: Plush pink polyester cotton blend from the motel closet
The luminance has been composed as a mosaic of approx. 200 frames recorded by the Subaru Telescope (filter 671nm, narrow).
RGB data from a former image:
SII: 20x900s
Ha: 17x900s
OIII: 16x900s
Takahashi FSQ106EDXIII and QSI683
Data: NAOJ, R. Colombari
Assembling and processing: R. Colombari
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The prominent ridge of emission featured in this dramatic skyscape is cataloged as IC 5067. Part of a larger emission nebula with a distinctive shape, popularly called The Pelican Nebula, the ridge spans about 10 light-years following the curve of the cosmic pelican's head and neck. This false color view also translates the pervasive glow of narrow emission lines from atoms in the nebula to a color palette made popular in Hubble Space Telescope images of star forming regions. Fantastic, dark shapes inhabiting the 1/2 degree wide field are clouds of cool gas and dust sculpted by the winds and radiation from hot, massive stars. Close-ups of some of the sculpted clouds show clear signs of newly forming stars. The Pelican Nebula, itself cataloged as IC 5070, is about 2,000 light-years away. To find it, look northeast of bright star Deneb in the high flying constellation Cygnus.
Source: APOD NASA
The Crescent Nebula (also known as NGC 6888, Caldwell 27, Sharpless 105) is an emission nebula in the constellation Cygnus, about 5000 light-years away from Earth. It was discovered by William Herschel in 1792. It is formed by the fast stellar wind from the Wolf-Rayet star colliding with and energizing the slower moving wind ejected by the star when it became a red giant around 250,000 to 400,000 years ago. The result of the collision is a shell and two shock waves, one moving outward and one moving inward. The inward moving shock wave heats the stellar wind to X-ray-emitting temperatures.It is a rather faint object located about 2 degrees SW of Sadr.
I present to you an apparently unnamed nebula in the large Sadr nebula complex. In my opinion it is on a par with many better-known nebulae. I especially like those intriguing yellow streaks below the blueish centre of the image. I wonder if they are formed by solar winds and radiation from the stars in the centre.
I took this image from my backyard in Luxembourg (Europe) on the nights between June 18 and 24.
Total exposure is about 17 hours (9h halpha, 4h SII and 4h OIII).
Equipment: 8” ONTC Newton, Avalon Linear mount, ASI 1600mmc Pro and Baader narrowband filters.
I've always enjoyed images from space, can't really afford an astro photography rig so I thought I would make my own nebula, three images taken in my kitchen with a small fish tank, water and paint, the 'stars' are air bubbles stuck to the front of the tank, a little play in lightroom then into CS5, layers were blended and a few adjustments, back into lightroom and a little work with curves, contrast and clarity, two flash guns used at 3o/c and 9 o/c and at 12o/c for the last image, not the hubble but I like it😊
Taken at Inspire Space Park (the only editing in my photos is cropping and use of a filter sometimes, everything is as seen in world)
My first record of the Trifid Nebula. The stacked frames, captured on two consecutive nights, totaled 5 hours and 10 minutes of exposure.
"The Trifid Nebula, also known as Messier 20 (M20), is a large star-forming region located in the southern constellation Sagittarius. The nebula’s name means “divided into three lobes,” and refers to the object consisting of three types of nebulae and an open star cluster. The open cluster is surrounded by an emission nebula, a reflection nebula, and a dark nebula within the emission nebula that gives M20 the trifurcated appearance for which it is known". Source: constellation-guide.com
Sky-Watcher 203mm F / 5 EQ5 reflector with Onstep, Canon T6 (primary focus) modified, Optolong L-eNhance filter (in one third of the frames). Guidescope 50mm with ASI 290MC. 62 light frames (42x300 "ISO 800 + L-eNhance: 20x300" ISO 1600). Processing: Sequator and PixInsight.
@LopesCosmos
This supernova remnant in the constellation Gemini is about 5,000 light years away from earth.
Image taken with TS Star71/347mm, ATIK 383l+ and Baader narrowband filters (Ha, OIII, SII). Total exposure: 12*1200s Ha, 8*1200s OIII, 10*600s SII (bin2x2) = about 9 hours.
Started this project of the Horsehead Nebula with "first light" from my new observatory on 10/21/15. Finally collected enough sub-frames to complete the project on 11/15/15.
2 panel mosaic
Telescope: Celestron 11" EdgeHD w/Hyperstar (F/2)
Camera: QHY23M @-30C
Each panel(2) consists of the following filtered images
Lum- 25x120sec
Red-10x120sec
Green-10x120sec
Blue-10x120sec
Guiding with 50mm refractor,QHY5L-IIM & Metaguide. Acquired with APT, processed with Nebulosity V4, Photoshop CS6.
The Veil nebula in dual channel narrowband (HA and OIII); a supernova remnant in the Cygnus constellation, around 1500 light years from earth.
Image acquisition details:
20x600" HA
15x600" OIII
Serena and i seem to be having an umbrella theme going on, maybe due to the amount of rain in England atm. I might grab an umbrella too and get behind the camera...watch this space!
*Items worn were purchased at below
maps.secondlife.com/secondlife/8%208/67/117/1086
*Pic taken at Backdrop city, neon area.
Two nights of acquisition - 160 minutes of total integration time.
Nikon D5300 Nikon 500mm catadioptric lens. 320 thirty-second light frames, plus dark. bias and flat calibration frames. Astro Pixel Processor, LR and PS.
Messier 42 - Orion Nebula - a diffuse nebula ~1344 light years away. Fo-Sho processing
54x3min exposures stacked in PixInsight
Camera: ASI2600 MC Pro
Telescope: Explore Scientific ED102-FCD100 (4" Refractor)
ASI AM5
Back to adventures in astrophotography. Found in the constellation Gemini, here is a supernova remnant at a distance of 5,000 light years from Earth. The span of the nebula is 70 light years-- must have been quite an explosion! Astronomers can only give a wide estimate of when the supernova event occurred: 8,000 - 30,000 years ago.
I wonder how bright it appeared from Earth...? The brightest supernova in recorded history was observed in 1066 AD. Roughly 16 times brighter than Venus and easily visible during daylight hours, it was written about in many corners of the world. It is said that some North American petroglyphs likely depict the 1066 supernova.
Image obtained after approx 2.5 hours each through Ha and OIII filters. Exposures of 5 minutes. It actually looks like a jellyfish, yes???
Portion of the Eastern Veil Nebula also known as Caldwell 33, whose brightest area is NGC6992.
The Veil Nebula is a cloud of heated and ionized gas and dust in the constellation Cygnus.
The Nebula was discovered on 1784 by William Herschel.
Given a distance of 2400 Light Years, this gives the radius of the entire nebula as 64 Light Years.
Undulations in the surface of the shell lead to multiple filamentary images, which appear to be intertwined.
Equipment:
Celestron 9.25” 2350mm Edge-HD Telescope
Sky-Watcher EQ6-R Pro Computerized GoTo Telescope Mount
Orion 50mm Helical Guide Scope & StarShoot AutoGuider
Celestron 9x50 Finder Scope
ZWO ASI294MC Pro Color Camera
Celestron .7 EdgeHD Reducer Lens
PHD2 Guiding Software
SharpCap Pro
Thank you for your comments.
Gemma
20x30 in 77x51 cm
None of my work is Ai assisted and is copyright Rg Sanders aka Ronald George Sanders.
WIP.
I wanted to release this a while ago (before the Sinistre eyes), but i changed them a lot, to a point where they barely look like the first editions...
Previously known as "Ilz named our picture: Kamikaze" "laughs"
More details on Nebula post
Feat: Tentacio, tomoto, EMBW, (red) Mint, Takeo, HPMD, MelonBunny, Maru Kado
Pose by Focus Poses
The Rosette Nebula (also known as NGC 2237 and C 49) is a large, roughly circular H II region located on the edge of a giant molecular nebula in the constellation Unicorn. The nebula has an angular diameter of 1.3° and is located at a distance of 1600 parsecs (about 5200 light years) from the solar system; it is approximately 100 light-years in size. At the center of the Rosette Nebula is a bright open cluster known as NGC 2244; the blue stars of the cluster, forming part of the OB association known as Monoceros OB2, emit ultraviolet radiation, which excites the gas of the nebula leading it to emit red light. The stellar wind from the O and B group of stars is thought to exert pressure on the interstellar cloud causing compression, followed by star formation; in fact, many Bok globules have been observed in the region, believed to be the site of star formation.