Nebulae Page - 6

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Except as noted, all of the images in this gallery were
processed by Ron Yelton, original data from Telescope Live

Abell 36 Out in the constellation of Virgo (the Virgin) is this cool looking planetary nebula. The gas that we can see is what's left of the central star's atmosphere once it went nova. The bright star in the center is now a white dwarf. It is thought that this nebula was formed about 10,000 years ago. It is about 780 light-years away BBWo 56 This is an emission nebula - meaning that the gases are heated by the radiation from a nearby star just off to the left to the point that it begins to glow. This image was taken using regular, visible light filters (RGB), as well as a hydrogen filter. This molecular cloud is almost exclusively made up of hydrogen which gives it the deep red color. This object is in the constellation Vela (the sails of a ship - the Argo) Collinder 399 - Brocchi's Cluster This image was originally taken to photograph the group of stars in the center, upper-right. There are ten stars that form an asterism known as The Coathanger. I'm including it here in the nebula section because of the gas and dust that lies behind the stars. The cluster is just a happy coincidence. It sits in the constellation Vulpecula NGC 3372 - The Carina Nebula This nebula resides in the constellation Carina about 8500 light-years away. It's one of the largest diffuse nebulae that we can see from Earth. It is four times as large and brighter than the famous Orion Nebula. It was discovered by Nicolas Louis de Lacaille in 1752 at the Cape of Good Hope. It is also one of the first five object that were photographed by the James Webb Space Telescope
  • Location: El Sauce Observatory, Chile
  • Date: July 2022
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: FLI PL9000 @-25c CHI-1 CCD
  • Exposure: 73x3 min LRGB 3hrs 30min
  • Location: Heaven's Mirror Obs, Australia
  • Date: November 2024
  • Mount: Paramount MX+
  • Telescope: FSQ-106ED AUS-2
  • Camera: QHY600m @-25c CMOS
  • Exposure:162x5 min RGB+Ha 13hrs
  • Location: Heaven's Mirror Obs, Australia
  • Date: April 2023
  • Mount: Paramount MX+
  • Telescope: FSQ-106ED AUS-2
  • Camera: QHY600m @-25c CMOS
  • Exposure: 74x5 min LRGB 6hrs 10min
  • Location: Heaven's Mirror Obs, Australia
  • Date: December 2024
  • Mount: Paramount MX+
  • Telescope: FSQ-106ED AUS-2
  • Camera: QHY600m @-25c CMOS
  • Exposure: 97x5 min HSO 7hrs 35min
Abell-36-LRGB-Jul22-CHI-1-CCD BBWo56-HRGB-Nov24-AUS-2-CMOS Brocchis-Cluster-WF-Apr2 ngc3372-SHO-Carina-Nebula-5-11-21
NGC 6888 - The Crescent Nebula (WF) This is a cool wide-field view of the area surrounding the Crescent Nebula (in the center). It's a faint object and requires a filter with good contrast. It's in the constellation Cygnus and sits about 5000 light-years away. This image was processed using OHS filter combination Cygnus North This is the northern section of the Veil Nebula in the constellation Cygnus, the Swan. It is part of a larger structure known as the Cygnus Loop. It's a supernova remnant whose original star exploded between 10,000 and 20,000 years ago and was roughly 20 times more massive than our Sun. It sits about 2400 light-years away from us Dust in Chamaeleon This is an image of some interstellar dust in the constellation Chamaeleon, the Chameleon or Lizard Sh2-190 - The Heart Nebula Also known as the Running Dog Nebula, this is a close-up view of the interior of the Heart Nebula. This nebula is located in the constellation Cassiopeia and is about 7500 light-years away. The majority of this nebula is made up of ionized oxygen and sulfur, which give the nebula its blue and orange/gold colors
  • Location: IC Astronomy Observatory, Spain
  • Date: April 2024
  • Mount: Paramount MX+
  • Telescope: Takahashi FSQ-106ED SPA-1
  • Camera: FLI PL 16083
  • Exposure: 69x5 min SHO 5hrs 45min
  • Location: El Sauce Observatory, Chile
  • Date: September 2023
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 51x5 min OHS 4hrs 15min
  • Location: Heaven's Mirror Obs, Australia
  • Date: January 11, 2021
  • Mount: Paramount MX+
  • Telescope: FSQ-106ED AUS-2
  • Camera: FLI PL16083 @-25c
  • Exposure: 8x10 min Ha and OIII 1hr 20min
  • Location: IC Astronomy Observatory, Spain
  • Date: January 2022
  • Mount: OS EQ
  • Telescope: Officina Stellare ProRC 700
  • Camera: FLI PL16803 @-25C SPA-2 CCD
  • Exposure: 62x5 min HSO 5hrs 10min
Crescent-WF-OHS-Apr24-SPA-1-CMOS Cygnus-North-HSO-Sep23-CHI-1-CMOS Dust-In-Chamaeleon-LRGB-Jan22-AUS-2-CCD Heart-Nebula-OHS-Dec21-SPA-2-CCD-cropped
Sh2-190 - The Heart Nebula This is the same image as the one above except that I processed it in a completely different way. By changing the color scheme different details can be seen IC 63 or Sh2-185 The central star in this image is Gamma Cassiopeiae. Just up and to the left is the main part of the nebula. This is an active star-forming region, heavy in Hydrogen gas. It was discovered by Max Wolf in 1893. The radiation from this central star is in the process of eroding the nebulosity that surrounds it. The areas that are less dense disappear, leaving the more dense areas which usually hold newly forming stars. This nebula lies about 10,500 light-years away IC 1396 - The Elephant's Trunk Nebula Located in the constellation of Cepheus (the King of Ethiopia, husband of Cassiopeia and father of Andromeda). In the deep interior of this nebula is the Elephant's trunk, which is a dense globule and an area of star formation. It's about 2400 light-years away IC 405 - The Flaming Star Nebula This nebula sits in the constellation Auriga (the Charioteer) - just about 1500 light-years away and 5 light-years across. It's both an emission and reflection nebula. This particular image was processed in the Hubble Palette OHS. The following two images show how different an image can be when the palette is changed around
  • Location: IC Astronomy Observatory, Spain
  • Date: January 2022
  • Mount: OS EQ
  • Telescope: Officina Stellare ProRC 700
  • Camera: FLI PL16803 @-25C SPA-2 CCD
  • Exposure: 62x5 min SHO 5hrs 10min
  • Location: IC Astronomy Observatory, Spain
  • Date: December 2023
  • Mount: Paramount MX+
  • Telescope: Takahashi FSQ-106ED SPA-1
  • Camera: FLI PL 16083
  • Exposure: 91x5 min HSO 7hrs 35min
  • Location: IC Astronomy Observatory, Spain
  • Date: August 2022 - September 2023
  • Mount: Paramount MX+
  • Telescope: FSQ-106ED SPA-3
  • Camera: FLI PL16083
  • Exposure: 98x5 min LRGB+Ha 14hrs 10min
  • Location: IC Astronomy Observatory, Spain
  • Date: November 2020 - September 2022
  • Mount: Paramount MX+
  • Telescope: Takahashi FSQ-106ED SPA-1
  • Camera:FLI PL16083 @-25c CCD
  • Exposure: 42x5 min OHS 10hrs 30min
Heart-Nebula-SHO-Dec21-SPA-2-CCD ic63-HSO-Dec23-SPA-1-CMOS-cropped ic1396-HLRGB-Aug22-Sep22-SPA-3 ic405-OHS-Mar22-SPA-1-CCD
IC 405 - The Flaming Star Nebula This version was processed in HSO. IC 405 - The Flaming Star Nebula This third version was done with the SHO palette. IC 1848 - The Soul Nebula This nebula is commonly known as the Soul Nebula. Located in the northern constellation of Cassiopeia, the Queen mother of Andromeda, this emission nebula contains a number of small open clusters embedded in its interior. Just to the lower-left of the Soul is the Heart Nebula, another emission nebula IC 4812 - The Coalsack Nebula The Coalsack Nebula lies about 600 light-years from Earth in the Southern constellation of Crux, the Southern Cross. It is one of the rare DSOs that can be seen with the naked eye. It plays an important part in the mythologies of the Australian Aboriginal people, and forms the head of the Emu in the Sky. For the Inca people, this nebula was called Yutu, a partridge-like bird in South America
  • Location: IC Astronomy Observatory, Spain
  • Date: November 2020 - September 2022
  • Mount: Paramount MX+
  • Telescope: Takahashi FSQ-106ED SPA-1
  • Camera:FLI PL16083 @-25c CCD
  • Exposure: 42x5 min OHS 10hrs 30min
  • Location: IC Astronomy Observatory, Spain
  • Date: November 2020 - September 2022
  • Mount: Paramount MX+
  • Telescope: Takahashi FSQ-106ED SPA-1
  • Camera:FLI PL16083 @-25c CCD
  • Exposure: 42x5 min OHS 10hrs 30min
  • Location: IC Astronomy Observatory, Spain
  • Date: November 2023
  • Mount: Paramount MX+
  • Telescope: Takahashi FSQ-106ED SPA-1
  • Camera: FLI PL16083
  • Exposure: 75x5 min SHO 6hrs 15min
  • Location: Heaven's Mirror Obs, Australia
  • Date: August 2023
  • Mount: Paramount MX+
  • Telescope: FSQ-106ED AUS-2
  • Camera: QHY600m @-25c CMOS
  • Exposure: 12x5 min LRGB 4hrs
ic405-HSO-Mar22-SPA-1-CMOS ic405-SHO-Mar22-SPA-1 ic1848-HSO-Nov23-SPA-1-CMOS ic4812-LRGB-Aug23-AUS-2-CMOS
Lupus Dust Panel 3 This one is a dark nebula in the constellation Lupus, the Wolf. A dark nebula is simply a cloud of gas or dust that is cold and dense enough to block the light coming from stars or objects behind it Messier 1 - The Crab Nebula The Crab nebula is a supernova remnant as well as a pulsar wind nebula located in the constellation Taurus (the Bull). It sits about 6500 light-years away. It was given its name because of an early drawing that resembled a crab. Remember, telescopes weren't as good back in the 1600s and 1700s as they are now. At its heart is a pulsar star which is only about 18 miles in diameter and spins at a rate of 30.2 times per second as it emits massive amounts of x-ray and gamma-ray radiation Messier 6 Messier 6 is actually the open cluster at the center of the image. I include it here because of the nebula right next to it - IC 4605. It is a reflection nebula located in the constellation Scorpius, and illuminated by its central star HD 148605 Messier 6 This is a close-up view of the object in the panel to the left, taken with a larger telescope
  • Location: Heaven's Mirror Obs, Australia
  • Date: November 2024
  • Mount: Paramount MX+
  • Telescope: FSQ-106ED AUS-2
  • Camera: QHY600m @-25c CMOS
  • Exposure: 60x5 min LRGB 5hrs
  • Location: IC Astronomy Observatory, Spain
  • Date: October 2023
  • Mount: Officina Stellare EQ Mount
  • Telescope: Officina Stellare ProRC 700
  • Camera: QHY600m @-25c SPA-2
  • Exposure: 74x5 min LRGB 6hrs 10min
  • Location: Heaven's Mirror Obs, Australia
  • Date: July 2021
  • Mount: Paramount MX+
  • Telescope: FSQ-106ED AUS-2
  • Camera: FLI PL16083 @-25c
  • Exposure: 72x10 min OHS 12hrs
  • Location: El Sauce Observatory, Chile
  • Date: May 2023
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 72x5 min OHS 6hrs
Lupus-Dust-Panel-3-RGB-Nov24-AUS-2-CMOS m1-LRGB-Oct23-SPA-2-CMOS m6-OHS-Jul21-AUS-2-CCD m6-OHS-May23-AUS-2-CMOS
Messier 42 Wide-Field A wide-field view of the larger molecular cloud around Messier 42, the Great Orion Nebula, which is the orange area to the right side. The Orion Nebula is a fascinating object. It sits about 1344 light-years away and has a mass of about 2000 times that of the Sun. It's also about 25 light-years across at its maximum. It is the largest star formation region closest to Earth. At its center is an area known as the Trapezium, where a number of hot, new stars can be seen. This is one of the most studied and photographed objects in our night sky Messier 42 Wide-Field - Starless This is the same image as the one to the left except that all of the stars have been removed. I like this version, as it has kind of a surreal look and feel to it Sh2-274 - The Medusa Nebula This object is a planetary nebula, and was discovered by UCLA astronomer George Abell in 1955. Abell thought that it was an old planetary nebula. Then, in 1975 researchers found that it was indeed a PN. The nebula is very large due to its expansion over a very long period which makes its surface brightness very low. That means that you'd need to use a camera with longer exposure times to see it. It is about 1500 light-years away in the constellation Gemini Sh2-1 Known as Sharpless-1, this is both a reflection and emission nebula as well as a diffuse nebula in Scorpius. It sits about 650 light-years away from Earth. This image was processed using visible light filters (RGB) as well as a hydrogen filter which brings out the deep red hydrogen region on the left side
  • Location: IC Astronomy Observatory, Spain
  • Date: November 2023
  • Mount: Paramount MX+
  • Telescope: FSQ-106EDX4 SPA-3
  • Camera: FLI PL16083
  • Exposure: 127x5 min OHS 10hrs 5min
  • Location: IC Astronomy Observatory, Spain
  • Date: November 2023
  • Mount: Paramount MX+
  • Telescope: FSQ-106EDX4 SPA-3
  • Camera: FLI PL16083
  • Exposure: 127x5 min OHS 10hrs 5min
  • Location: El Sauce Observatory, Chile
  • Date: November 2024
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 18x5 min OHS 5hrs 15min
  • Location: Heaven's Mirror Obs, Australia
  • Date: October 2024
  • Mount: Paramount MX+
  • Telescope: FSQ-106ED AUS-2
  • Camera: QHY600m @-25c CMOS
  • Exposure: 60x5 min LRGB+Ha 5hrs
m42-WF-OHS-Nov23-SPA-3-CCD m42-WF-OHS-Nov23-SPA-3-CCD-starless Medusa-Nebula-OHS-Nov24-CHI-1-CMOS Sh2-1-HLRGB-Oct24-AUS-2-CMOS
NGC 2014 This nebula, located in the Large Magellanic Cloud (LMC), is a red emission nebula which sits at an impressive distance of 163,000 light-years away NGC 6188 (The Rim Nebula) and NGC 6165 Also known as the Dragons of Ara, the Rim Nebula is just a small part of a much larger molecular cloud. This part of the planetary nebula contains an emission nebula that includes some dark nebulae as well. It lies about 4000 light-years away from us and is about 300 light-years in diameter. The small blue nebula in the upper right has two sections: an outer bubble and an inner bubble - probably from an earlier mass ejection from its central star, a type of star that burns hot and lives a short life. Since the larger nebula is often referred to as the Fighting Dragons of Ara, this smaller nebula is called The Dragon's Egg Caldwell 49 - The Rosette Nebula This object, located in Monoceros (the Unicorn), is part of a much larger molecular cloud complex. It sits about 5000 light-years away and is about 130 light-years in diameter. Some say that it resembles a human skull and is sometimes called the Skull Nebula. It has, at its center, an open cluster. The radiation from these hot, young stars excites the gas nearby and heats it until it begins to glow - making this an emission nebula. There are around 2500 hot, new stars. Most of the active star-forming is in the lower central region. For this version I removed the stars and applied a portrait tool in PixInsight to give it this unique look placeholder
  • Location: El Sauce Observatory, Chile
  • Date: October 25, 2020
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: FLI PL9000 @-25c CHI-1 CCD
  • Exposure: 8x10 min LRGB+Ha 1hr 20min
  • Location: Heaven's Mirror Obs, Australia
  • Date: May 2023
  • Mount: Paramount MX+
  • Telescope: FSQ-106ED AUS-2
  • Camera: QHY600m @-25c CMOS
  • Exposure: 20x5min HSO 1hr 40min
  • Location: IC Astronomy Observatory, Spain
  • Date: October 2023
  • Mount: Paramount MX+
  • Telescope: Takahashi ESQ-106ED SPA-1
  • Camera: FLI PL16083
  • Exposure: 93x5 min OHS 7hrs 45min
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ngc2014-OHS-Jul21-CHI-1-CCD RCW108-HSO-Apr23-AUS-2-CMOS-1 Rosette-Nebula-OHS-Oct23-SPA-1-CMOS-crop-2enhanced placeholder
Except as noted, all images Copyright © by Ron Yelton and may not be used without permission
Contact Ron at Aileron355@aol.com