Galaxy Gallery - 3


Click on a picture or link to view that gallery


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


NGC 6744 This galaxy lies about 30 million light-years away in the southern constellation of Pavo and is about 170,000 light-years across. It is an intermediate galaxy, which means it is in between a barred and an unbarred galaxy (the bar stretching across the center of the galaxy) NGC 247 In the southern constellation of Cetus lies NGC 247. Cetus is the sea monster that both Perseus and Hercules were to slay. Perseus saved Andromeda from Poseidon's wrath when he killed the monster. It is also one of the 12 Zodiac constellations. It lies outside the galactic plane which leaves it unobstructed by dust and gas in the Milky Way.
Note the far-distant galaxy PGC 834794 in the upper-left
NGC 1291 NGC 1291 is what is called a Ring Galaxy. Its outer ring is still producing new stars at a slow rate. Even though it has an unusual inner bar, it is classified as a lenticular galaxy. It also has a large central bulge. It is an early-type galaxy, which means that it has a lot of old globular clusters, 65% of which are metal-poor. The rest are newer, metal-rich globular clusters. It is nearly face-on and lies about 33 million light-years away Messier 66 M66 is an intermediate spiral galaxy located in the constellation Leo (The Lion). It is part of a group of galaxies known as the Leo Triplet. It lies about 31 million light-years from Earth and has been disfigured by a gravitational encounter of some kind in the past
  • Location: El Sauce Observatory, Chile
  • Date: October 2023
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 117x5min LRGB 9hrs 15min
  • Location: El Sauce Observatory, Chile
  • Date: July - August 2022
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: FLI PL9000 @ -25c CHI-1
  • Exposure: 44x10min LRGB 7hrs 10min
  • Location: El Sauce Observatory, Chile
  • Date: July - December 2023
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: FLI PL9000 @ -25c CHI-1
  • Exposure: 50x50min LRGB 4hrs 10min
  • Location: El Sauce Observatory, Chile
  • Date: June 23, 2023
  • Mount: Officina Stellare EQ Mount
  • Telescope: Officina Stellare Pro RC 700 (27" f/8)
  • Camera: QHY600m @-25c SPA-2
  • Exposure: 81x2 min LRGB 2hrs 40min
NGC 6744 NGC 247 NGC 1291 Messier 66



Messier 74 - The Phantom Galaxy Messier 74 is a spiral galaxy located in the constellation Pisces. It lies about 32 million light-years away and is known for its well-defined spiral arms. Because of its low surface brightness, it is sometimes called the Phantom Galaxy NGC 300 NGC 300 is a spiral galaxy in Sculptor. It is about 6 million light-years away and although not quite a part of it, is very close to our Local Group of galaxies. Although we see it at a different angle, it is very similar to the Triangulum Galaxy NGC 1232 - The Eye of God Galaxy This galaxy is technically of the Grand Design family of galaxies, although it is normally classified as an intermediate spiral galaxy. It was discovered by William Herschel in 1784 and lies about 61 million light-years away. It also appears to have been disturbed by a gravitational encounter, as the spiral arms on the right side are disfigured. I always enjoy processing galaxies in deep-sky fields. Once I'm done I can zoom in real tight and count the other distant galaxies. I counted 401 galaxies in one image that I did recently NGC 1313 - The Topsy Turvy Galaxy This galaxy was discovered by James Dunlop back in 1826. It has a diameter of about 50,000 light-years which is about half the size of the Milky Way. It is in the constellation Reticulum and lies about 13 million light-years away. It is an irregular galaxy as well as a field galaxy. A field galaxy is one that is not part of a galaxy group which leaves it gravitationally alone
  • Location: El Sauce Observatory, Chile
  • Date: November 2023
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c (CHI-1)
  • Exposure: 57x5min LRGB 4hrs 45min
  • Location: El Sauce Observatory, Chile
  • Date: June 2023
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 36x5min LRGB 4hrs 40min
  • Location: El Sauce Observatory, Chile
  • Date: December 2023
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 105x5min LRGB 8hrs 15min
  • Location: El Sauce Observatory, Chile
  • Date: October - November 2023
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c (CHI-1)
  • Exposure: 125x5min LRGB 9hrs 55min
Messier 74 NGC 300 NGC 1232 NGC 1313



NGC 6822 - Barnard's Galaxy This galaxy is located in the constellation Sagittarius and although it looks like an elliptical galaxy, it is actually a barred irregular galaxy. Most of its stars were formed in the last 3–5 billion years. It lies about 1.63 million light-years away from us. Although it's difficult to see in this image, the galaxy actually extends outward considerably from the bright central area. At the 11:30, 1 o'clock, and 2 o'clock positions there are three very active Hydrogen II star formation areas Markarian's Chain Markarian's Chain is a group of galaxies in the constellation Virgo that form a curved line, or chain. The two brightest galaxies were first cataloged by Charles Messier in 1781. The rest of the galaxies in the chain were discovered by William Herschel. In about the center of the chain (right side) there appear to be two interacting galaxies. There are a couple more interacting galaxies toward the lower left. The chain is roughly 50 million light-years away. As I was processing this image I noticed that there were a lot of galaxies in the image. So I zoomed in really close and counted 276 additional galaxies. Also, if you trace the chain from right to left, it forms a well-defined question mark NGC 253 - The Sculptor Galaxy This galaxy was discovered by Caroline Herschel in 1783 while she was looking for comets. It resides in the constellation Sculptor. It is a starburst type galaxy, meaning that it is actively making new stars all across the galaxy. It is thought to have a black hole at its center that is about 5 million times the mass of our Sun. It is roughly 10.9 million light-years away from us IC 1613 IC 1613 is a diffuse dwarf irregular galaxy in the constellation Cetus. It is a member of our Local Group of galaxies and lies about 2.38 million light-years away from Earth
  • Location: El Sauce Observatory, Chile
  • Date: August 10, 2021
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: FLI PL9000 @ -25c (CHI-1) (CCD)
  • Exposure: 42x10min LRGB 7hrs
  • Location: El Sauce Observatory, Chile
  • Date: March 2024
  • Mount: Paramount MX+
  • Telescope: Takahashi FSQ-106ED SPA-1
  • Camera: QHY600m CMOS @ -25c
  • Exposure: 60x5 min LRGB 5hrs
  • Location: El Sauce Observatory, Chile
  • Date: March 2024
  • Mount: Paramount MX+
  • Telescope: Takahashi FSQ-106ED SPA-1
  • Camera: QHY600m CMOS @ -25c
  • Exposure: 65x5 min LRGB 5hrs 25min
  • Location: El Sauce Observatory, Chile
  • Date: August 24, 2024
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 111x5 min LRGB 5hrs 55min
NGC 6822 Markarian's Chain SPA-1 ngc 253 IC 1613



NGC 3521 NGC 3521 sits about 26 million light-years away in the constellation Leo (the Lion). It is classified as a flocculent intermediate spiral galaxy, which means that it is a spiral galaxy with a trace of a bar and moderately to loosely wound spiral arms NGC 1512 NGC 1512 is a barred spiral galaxy in the constellation Eridanus Messier 33 - The Triangulum Galaxy The Triangulum Galaxy is one of our Local Group of galaxies and is gravitationally bound to the Andromeda Galaxy. It is the third largest galaxy of our Local Group after the Andromeda Galaxy and the Milky Way. It is an average sized spiral galaxy located 3 million light-years away. Also known as the Pinwheel Galaxy and contains 40 billion stars NGC 2997 This galaxy was discovered by William Herschel in 1793 in the southern constellation Antlia (the Pump). It is a Grand Design Galaxy as well as a Barred Spiral Galaxy. The magenta knots scattered around the spiral arms indicate active star-forming regions. 2003 and 2008 each saw a supernova in the galaxy. It is about 40 million light-years away
  • Location: El Sauce Observatory, Chile
  • Date: February 2024
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c (CHI-1)
  • Exposure: 40x5 min LRGB 6hrs 20min
  • Location: El Sauce Observatory, Chile
  • Date: July 2024
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 135x5 min LRGB 10hrs 35min
  • Location: IC Astronomy Observatory, Spain
  • Date: July 2023
  • Mount: Paramount MX+
  • Telescope: Takahashi FSQ-106ED SPA-1
  • Camera: FLI PL16083
  • Exposure: 92x10min LRGB 14hrs 20min
  • Location: El Sauce Observatory, Chile
  • Date: March 2021
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: FLI PL9000 @ -25c CHI-1 CCD
  • Exposure: 49x10 min LRGB 8hrs 10min
NGC 3521 NGC 1512 Messier 33 NGC 2997



NGC 1398 Way out in the constellation Fornax lies this beautiful double-ringed barred galaxy. It boasts over 100 billion stars and spans 135,000 light-years. Its distance from Earth is approximately 65 million light-years and it was first discovered by the German astronomer Friedrich Winnecke in 1868 while he was searching for comets NGC 660 This fascinating galaxy, located in Pisces, is both a peculiar galaxy as well as a polar ring galaxy. It is thought to either be a disk galaxy that has been accumulating matter throughout its life or a lenticular galaxy that collided with another galaxy sometime in the past. It is about 45 million light-years away Large Magellanic Cloud The LMC is classified as a Magellanic Spiral. It has a stellar bar that is off-center which leads us to believe that it was once a barred spiral galaxy before its arms and structure were disrupted by an encounter with the nearby Small Magellanic Cloud (SMC). It lies about 163,000 light-years away from Earth and has a diameter of about 32,200 light-years Messier 64 - The Black Eye Galaxy This galaxy is a Seyfert galaxy meaning that it has a quasar-like nucleus and is an X-ray source. It has two counter-rotating discs that have about the same mass. The counter-rotation may have been caused by an interaction with another galaxy that had an opposite direction (retrograde) orbit. It lies about 17 million light-years away in the constellation Coma Berenices. It gets its name from the dark dust lane that partially rings the nucleus giving it the appearance of a black eye
  • Location: El Sauce Observatory, Chile
  • Date: November 2024
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 123x5 min LRGB 9hrs 45min
  • Location: El Sauce Observatory, Chile
  • Date: December 2024
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 86x5 min LRGB 7hrs 10min
  • Location: Heaven's Mirror Observatory, Australia
  • Date: January 2021 - January 2022
  • Mount: Paramount MX+
  • Telescope: FSQ-106ED AUS-2
  • Camera: FLI PL16083 @-25c
  • Exposure: 211x5 min LRGB 17hrs 05min
  • Location: IC Astronomy Obs, Spain
  • Date: March 2021
  • Mount: OS EQ
  • Telescope: Officina Stellare ProRC 700
  • Camera: FLI PL16803 @ -25c SPA-2 CCD
  • Exposure: LRGB 3hrs
NGC 1398 NGC 660 Large Magellanic Cloud Messier 64 - Black Eye Galaxy



Messier 77 This galaxy is a barred spiral located in the constellation Cetus (the Sea Monster). It was discovered by Pierre Méchain in 1780. He originally thought that it was a nebula. Messier and William Herschel both thought that it was a star cluster. It is also the brightest Seyfert galaxy that can be seen from Earth The Fornax Dwarf Galaxy This is an elliptical dwarf galaxy located in the constellation Fornax. This galaxy is part of our Local Group of galaxies. It contains 6 globular clusters which is considered a lot by current standards. It is also moving away from us Messier 104 - The Sombrero Galaxy Sitting as a member of the Virgo Group, a string of galaxies and globular clusters near the Virgo Supercluster, the Sombrero Galaxy is about 31.1 million light-years away from us and has a diameter of about 105,000 light-years, making it slightly larger than our Milky Way. It is currently classified as a peculiar galaxy but no other information about its classification is known since we can't see into the interior to see if it has a bar (or two) or even if it is a spiral galaxy. It has a very well-defined dust lane along its outer edge as well as some interior dust lanes Messier 100 - The Mirror Galaxy This galaxy resides in the constellation Virgo (The Virgin). It is classified as a Grand Design Intermediate Spiral Galaxy. It sits 55 million light-years away from us and is the largest and brightest galaxy in the Virgo cluster of galaxies. Its diameter is 166,000 light-years. It was discovered by Pierre Méchain in 1781 and then again by Charles Messier just 29 days later
  • Location: El Sauce Observatory, Chile
  • Date: December 2021
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: FLI PL9000 @ -25c CHI-1 CCD
  • Exposure: 32x10 min LRGB 5hrs 20min
  • Location: Heaven's Mirror Observatory, Australia
  • Date: April 2025
  • Mount: Paramount MX+
  • Telescope: FSQ-106ED AUS-2
  • Camera: QHY600m @ -25c CMOS
  • Exposure: 47x5 min LRGB 3hrs 55min
  • Location: El Sauce Observatory, Chile
  • Date: April 2025
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 124x5 min LRGB 9hrs 50min
  • Location: El Sauce Observatory, Chile
  • Date: May 2025
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 84x5 min LRGB 7hrs
Messier 77 Fornax Dwarf Galaxy Messier 104 - Sombrero Galaxy Messier 100



NGC 5128 - Centaurus A This galaxy is found in the southern hemisphere and sits around 12 million light-years away in the constellation Centaurus (The Centaur). It is the fifth brightest galaxy in our nighttime sky as well as the closest radio galaxy to Earth. It also has a very active galactic nucleus. There isn't complete agreement as to whether this is a lenticular galaxy or a giant elliptical galaxy. At its center is a supermassive black hole that weighs in at around 55 million solar masses. There are two relativistic jets being ejected perpendicular to the brown dust lanes that are heavy in X-ray and radio frequencies. It is thought that a collision between this galaxy (elliptical) and a smaller spiral galaxy has caused massive amounts of new star formation Messier 83 - The Southern Pinwheel Galaxy Charles Messier added this object to his catalog in March of 1781 after it was discovered by Nicolas-Louis de Lacaille in 1752 at the Cape of Good Hope. It is in the constellation Hydra (the snake that was slain by Hercules) and is one of the closest and brightest galaxies in our night sky. It is probably about 15 million light-years away. It is a massive barred spiral Grand Design galaxy and an interaction with the dwarf galaxy NGC 5253 within the last billion years began its active starburst period
  • Location: El Sauce Observatory, Chile
  • Date: May 2025
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 159x5 min LRGB 13hrs 15min
  • Location: El Sauce Observatory, Chile
  • Date: April 2023
  • Mount: Mathis MI-1000
  • Telescope: Planewave CDK24 f/6.6
  • Camera: QHY600m @-25c CHI-1
  • Exposure: 124x5 min LRGB 10hrs 20min
NGC 5128 - Centaurus A Messier 83
Except as noted, all images Copyright © by Ron Yelton and may not be used without permission
Contact Ron at Aileron355@aol.com