The Flickr C11A Image Generatr

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This page simply reformats the Flickr public Atom feed for purposes of finding inspiration through random exploration. These images are not being copied or stored in any way by this website, nor are any links to them or any metadata about them. All images are © their owners unless otherwise specified.

This site is a busybee project and is supported by the generosity of viewers like you.

IC342 Hidden Galaxy by Steve J Peters

© Steve J Peters, all rights reserved.

IC342 Hidden Galaxy

It was bitterly cold on the night of 2nd January 2025, but what a beautifully crystal clear starry night it was. So the year began with stargazing late into the night (or early morning).
To begin proceedings I spent over 4 hours capturing this image of IC 342, the Hidden Galaxy in the northern constellation of Camelopardilus.

It is a spiral galaxy the far side of the equator of the Milky Way’s pearly disk, which is crowded with thick cosmic gas, dark dust, and glowing stars that all obscure our view, earning it the nickname of the Hidden Galaxy. It is roughly 11 million light years away and about 50,000 light-years across (half the size of our own Milk Way galaxy).

~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus
Main Camera: ZWO ASI533MC Pro at -10C
Filter: Optolong L-Pro filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 126 at 120 seconds, gain 101, temp -10C
Darks 30 at 120 seconds, gain 101, temp -10C
Flat 30 at 1.1 seconds, gain 101, temp -10C
Dark Flat 30 at 1.1 seconds, gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in Pixinsight
Captions added in Photoshop CS4

M74 NGC628 Phantom Galaxy in Pisces by Steve J Peters

© Steve J Peters, all rights reserved.

M74 NGC628 Phantom Galaxy in Pisces

Messier 74 (also known as NGC 628 and Phantom Galaxy) is a large spiral galaxy in the constellation Pisces. It is about 32 million light-years away from Earth. The galaxy contains two clearly defined spiral arms and is therefore used as an archetypal example of a grand design spiral galaxy. The galaxy's low surface brightness makes it the most difficult Messier object for amateur astronomers to observe. Its relatively large apparent size and the galaxy's face-on orientation make it an ideal object for astronomers who want to study spiral arm structure and spiral density waves. It is estimated that M74 hosts about 100 billion stars.

~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus
Main Camera: ZWO ASI533MC Pro at -10C
Filter: Optolong L-Pro filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 110 at 120 seconds, gain 101, temp -10C
Darks 30 at 120 seconds, gain 101, temp -10C
Flat 30 at 1.1 seconds, gain 101, temp -10C
Dark Flat 30 at 1.1 seconds, gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in Pixinsight
Captions added in Photoshop CS4

NGC 7331 Deer Lick Galaxy Group by Steve J Peters

© Steve J Peters, all rights reserved.

NGC 7331 Deer Lick Galaxy Group

The Deer Lick Galaxy Group is really only a visual grouping of galaxies in the constellation Pegasus.

The large, spiral galaxy NGC 7331 in the centre of this picture is a foreground galaxy in the same field of view as the collection known as the Deer Lick Group. It contains four other members, affectionately referred to as the "fleas": the lenticular or unbarred spirals NGC 7335 and NGC 7336, the barred spiral galaxy NGC 7337 and the elliptical galaxy NGC 7340. These galaxies lie at distances of approximately 332, 365, 348 and 294 million light years, respectively.

Although adjacent on the sky, this collection is not a galaxy group, as NGC 7331 itself is not gravitationally associated with the far more distant "fleas"; indeed, even they are separated by far more than the normal distances (~2 million light years) of a galaxy group.

Even so, it is nice to be able to capture so many galaxies in one shot.


Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Pro
Main Camera: ZWO ASI533MC Pro at -10C
Filter: ZWO UV/IR Cut filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 93 at 120 seconds, gain 101, temp -10C
Darks 30 at 120 seconds, gain 101, temp -10C
Flat 30 at 1.14s, gain 101, temp -10C
Dark Flat 30 at 1.14s, gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight.
Captions added in Photoshop CS4

Comet C/2023 A3 Tsuchinshan-ATLAS by Steve J Peters

© Steve J Peters, all rights reserved.

Comet C/2023 A3 Tsuchinshan-ATLAS

This is my only shot of the comet C/2023 A3 (Tsuchinshan–ATLAS) that everyone has been talking about in recent weeks. It has passed its prime and is fading now as it zooms away from the sun for another 80,000 years.

The relentless cloud cover prevented me from seeing it until a couple of days ago. A rare clear night, so I pointed my Celestron C11 scope up and this is what it saw, after a bit of processing with PixInsight to extract and align the coment and reapply to the starless image. It turns out that is harder than it sounds.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus 256G
Main Camera: ZWO ASI533MC Pro at -10C
Filter: ZWO UV/IR Cut filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 40 at 10 seconds, gain 101, temp -10C
Darks 30 at 10 seconds, gain 101, temp -10C
Flats 30 at 610ms, gain 101, temp -10C
Dark Flats 30 at 610ms, gain 101 temp -10C

Bortle 4 sky.
Integrated and processed in PixInsight
Added captions in Photoshop CS4

NGC457 Owl Cluster in Cassiopeia by Steve J Peters

© Steve J Peters, all rights reserved.

NGC457 Owl Cluster in Cassiopeia

The Owl Cluster is a bright open star cluster located approximately 8,000 light-years away in the northern constellation Cassiopeia. It has the designation NGC 457 in the New General Catalogue and is listed as Caldwell 13 in Sir Patrick Moore’s Caldwell catalogue.

The Owl Cluster is one of the finest telescope targets in the northern sky. It is easy to find because it appears in the region of Cassiopeia’s W. NGC 457 is also popularly known as the E. T. Cluster, Dragonfly Cluster, Kachina Doll Cluster, and Phi Cassiopeiae Cluster. I'll go with Owl Cluster as it is easier to spell.

The brightest members of the Owl Cluster are blue stars which are hot, massive, luminous stars that burn through their supply of fuel quickly and evolve into giants or supergiants within only a few million years. They have very short lives due to their high mass. The most massive of these stars will end their lives as supernovae, while others will cast away their outer layers to form planetary nebulae and slowly fade away as dim white dwarfs.

NGC 457 gets its most common nicknames – the Owl Cluster and the E.T. Cluster – because of two bright stars that appear in the same field. These two stars look like a pair of eyes, while the fainter stars form an outline of an owl - or the popular character E.T. from Steven Spielberg’s 1982 film.

This image was taken by integrating 20 two-minute exposures using my C11 telescope. That is not long for astrophotography, but the camera sensor picks up light from the stars much faster than the faint glow from nebulae.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus 256G
Main Camera: ZWO ASI533MC Pro at -10C
Filter: Optolong L-Pro filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 20 at 120 seconds, gain 101, temp -10C
Darks 30 at 120 seconds, gain 101, temp -10C
Flats 30 at 1.1 seconds, gain 101, temp -10C
Dark Flats 30 at 1.1 seconds gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Added captions in Photoshop CS4

NGC1491 Fossil Footprint Nebula in Perseus by Steve J Peters

© Steve J Peters, all rights reserved.

NGC1491 Fossil Footprint Nebula in Perseus

NGC 1491 is called the Fossil Footprint Nebula. It is a bright emission nebula and hydrogen (HII) region, located on the edge of a vast cloud region of neutral gas, about 10,700 light-years away in the Perseus arm of our Milky Way Galaxy in the constellation Perseus.

HII regions are well known for being places where new stars are born, and are created when ultraviolet radiation from hot stars ionizes the surrounding gas, causing it to glow in visible light. The surrounding dust is also heated by this radiation, so we also see it glow in infrared light.

The bright, blue star near the centre is illuminating the nebula while its strong stellar wind is “blowing” a bubble in the gas that immediately surrounds it. The intense radiation from the star is also eroding the gas clouds surrounding it.

The entire nebula is quite irregular with a subtle bite cut out of the nebulosity that creates a darker hollow, and a high surface brightness region as seen in this image. A faint, elongated haze extends from this patch past the star, giving an elongated appearance.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus 256G
Main Camera: ZWO ASI533MC Pro at -10C
Filter: Optolong L-eNhance filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 63 at 120 seconds, gain 101, temp -10C
Darks 30 at 120 seconds, gain 101, temp -10C
Flats 30 at 6.5 seconds, gain 101, temp -10C
Dark Flats 30 at 6.5 seconds gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Added captions in Photoshop CS4

M27 Dumbbell Nebula by Steve J Peters

© Steve J Peters, all rights reserved.

M27 Dumbbell Nebula

The Dumbbell Nebula is a bright, large planetary nebula located in Vulpecula constellation. The nebula is about 1,300 light years from Earth. It is sometimes also called the Apple Core Nebula or Diablo Nebula, and has the designation NGC 6853 in the New General Catalogue.

The Dumbbell Nebula was the first planetary nebula to be discovered. Charles Messier included it as M27 in his catalogue of deep sky objects in 1764.

Planetary nebulae, like this and the Ring Nebula, are the remains of stars similar to our Sun. When they reach the end of their life cycle as evolved red giants, they expel their outer gaseous layers to form the nebula, which is then heated by the hot core of the central white dwarf. This will be the fate of our Sun in roughly five billion years.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus 256G
Main Camera: ZWO ASI533MC Pro at -10C
Filter: Optolong L-Pro filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 58 at 120 seconds, gain 101, temp -10C
Darks 30 at 120 seconds, gain 101, temp -10C
Flats 30 at 1.1 seconds, gain 101, temp -10C
Dark Flats 30 at 1.1 seconds gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Added captions in Photoshop CS4

M29 The Cooling Tower Open Cluster in Cygnus by Steve J Peters

© Steve J Peters, all rights reserved.

M29 The Cooling Tower Open Cluster in Cygnus

At the end of my stargazing session last night there was still a bit of dark sky remaining so I spent about three quarters of an hour on Messier 29.

M29, also known as NGC 6913, is sometimes called the Cooling Tower Cluster. It is a quite small, bright open cluster of stars just south of the central bright star Gamma Cygni in the constellation of Cygnus, the Swan.

I didn't have to spend hours capturing faint wisps of galactic spiral arms or fetching the folds and details of a nebula because the stars show up quickly against the dark sky.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus 256G
Main Camera: ZWO ASI533MC Pro at -10C
Filter: ZWO IR Cut filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 23 at 120 seconds, gain 101, temp -10C
Darks 30 at 120 seconds, gain 101, temp -10C
Flats 30 at 1.08 seconds, gain 101, temp -10C
Dark Flats 30 at 1.08 seconds gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Added captions in Photoshop CS4

Albireo - Beta2 in Cygnus by Steve J Peters

© Steve J Peters, all rights reserved.

Albireo - Beta2 in Cygnus

I captured this image of Albireo, one of the main, visible stars in the constellation of Cygnus. Actually, make that two as it is a double star. They stand out brightly against the glittering backdrop of the Cygnus Star Cloud.

Albireo A is the larger, amber star and Albireo B is the smaller sapphire blue star. If they are orbiting each other the orbital period is at least 75,000 years.

It turns out that Albireo A is itself a binary star with the components orbiting every 100 years. This whole system is a mere 380 light years away. You could almost touch it - if you had long arms.

The amber star is about 50 times the size of our sun and shines 950 times as bright. The little blue star is only 3 times the mass of our sun and only shines 190 times as bright.

This is a combination of 62 ten-second exposures using my C11. Any longer and the bright stars would have been way over exposed, any less and the background stars would not have shown up.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus 256G
Main Camera: ZWO ASI533MC Pro at -10C
Filter: ZWO UV/IR Cut filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 62 at 10 seconds, gain 101, temp -10C
Darks 30 at 10 seconds, gain 101, temp -10C
Flat 30 at 570 ms, gain 101, temp -10C
Dark Flat 30 at 570 ms gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Added captions in Photoshop CS4

M40 Double Star in Ursa Major by Steve J Peters

© Steve J Peters, all rights reserved.

M40 Double Star in Ursa Major

Sometimes I find there are nothing like as many stars to see as other times.

Take this picture which includes M40, a pair of bright stars that Charles Messier thought was a double star. It is in Ursa Major (or the Plough, near to Megrez the star that connects the handle to the plough).

The stars form an optical pair, lying along the same line of sight, but not physically connected to each other as they are now known to be at different distances from Earth. One is about 470 light years away and the other is over 1000.

Messier was trying to identify nebulae but at that time it was hard to distinguish between galaxies and nebulae. This one of the few objects that made it into his catalogue that were neither.

What he missed were two spiral galaxies that my C11 picked up near to M40. The larger one just under the word Major is NGC 4290 and the much fainter one below that is PGC 39934.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus 256G
Main Camera: ZWO ASI533MC Pro at -10C
Filter: ZWO UV/IR cut filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 12 at 120 seconds, gain 101, temp -10C
Darks 30 at 120 seconds, gain 101, temp -10C
Flat 30 at 430ms, gain 101, temp -10C
Dark Flat 30 at 430ms gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Added captions in Photoshop CS4

M3 Globular Cluster in Canes Venatici by Steve J Peters

© Steve J Peters, all rights reserved.

M3 Globular Cluster in Canes Venatici

While the Seestar was snapping away on Thursday, my Celestron C11 was also busy.

This is another of the 250 or so globular clusters visible in our Milky Way. Messier 3 (M3) is located in the constellation Canes Venatici, the Hunting Dogs.

M3 is one of the largest and brightest star clusters, and is made up of around 500,000 stars. It is located at a distance of about 33,900 light-years from Earth, the cluster spans about 220 light-years. It is estimated to be 8 billion years old, making M3 one of the oldest formations in our galaxy. To put that in perspective, this nebula was already half its current age when our own Sun was formed.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus 256G
Main Camera: ZWO ASI533MC Pro at -10C
Filter: ZWO UV/IR cut filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 20 at 60 seconds, gain 101, temp -10C
Darks 30 at 60 seconds, gain 101, temp -10C
Flat 30 at 10s, gain 101, temp -10C
Dark Flat 30 at 10s gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Added captions in Photoshop CS4

IC1318B Butterfly Nebula in Cygnus by Steve J Peters

© Steve J Peters, all rights reserved.

IC1318B Butterfly Nebula in Cygnus

When I saw the name "Butterfly Nebula" and that it was clearly visible in the night sky near the star Sadr in the constellation Cygnus, I decided to capture it with the C11 spending 200 minutes soaking up that image until dawn obliterated the night sky. The result was this glowing red cloud of gas and dust.

Sadly I can't make out the "Butterfly", mainly because it is huge; way too large for the narrow focus of my big scope.

The Sadr Region (also known as IC 1318 or the Gamma Cygni Nebula) is the diffuse emission nebula surrounding Sadr (γ Cygni) at the centre of Cygnus's cross. The Sadr Region is one of the surrounding nebulous regions; others include the Butterfly Nebula (IC1318B) and the Crescent Nebula. It contains many dark nebulae in addition to the emission diffuse nebulae.

What I have captured is possibly one wing of the butterfly and a dark nebula Barnard 347 (B347) slightly left of centre at the bottom of this picture. A dark nebula is a type of interstellar cloud that is so dense that it obscures the light from objects behind it, such as background stars and nebulae. Dark clouds appear so because of sub-micrometre-sized dust particles, coated with frozen carbon monoxide and nitrogen effectively block the passage of light at visible wavelengths.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus 256G
Main Camera: ZWO ASI533MC Pro at -10C
Filter: Optolong L-Pro filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 100 at 120 seconds, gain 101, temp -10C
Darks 30 at 120 seconds, gain 101, temp -10C
Flat 30 at 10s, gain 101, temp -10C
Dark Flat 30 at 10s gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Added captions in Photoshop CS4

M64 Black Eye Galaxy in Coma Berenices by Steve J Peters

© Steve J Peters, all rights reserved.

M64 Black Eye Galaxy in Coma Berenices

It was supposed to be a clear night all night last night. It started well, but then banks of clouds rolled in and out so I only got a little over an hour's worth of data when I had to let it run all night.

The Black Eye Galaxy (also called Sleeping Beauty Galaxy or Evil Eye Galaxy and designated Messier 64, M64, or NGC 4826) is a relatively isolated spiral galaxy 17 million light-years away in the northern constellation of Coma Berenices.

Easily identified by the spectacular band of absorbing dust partially obscuring its bright nucleus, the Black Eye galaxy is characterized by its bizarre internal motion. The gas in the outer regions of this remarkable galaxy is rotating in the opposite direction from the gas and stars in its inner regions. This strange behaviour can be attributed to a merger between M64 and a satellite galaxy over a billion years ago. So this impact gave it that distinctive black eye.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus 256G
Main Camera: ZWO ASI533MC Pro at -10C
Filter: Optolong L-Pro filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 38 at 120 seconds, gain 101, temp -10C
Darks 30 at 120 seconds, gain 101, temp -10C
Flat 30 at 210 ms, gain 101, temp -10C
Dark Flat 30 at 210 ms gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Added captions in Photoshop CS4

Gulfstream Aerospace C-11A Gulfstream II by The Roving Aircraft Historian

© The Roving Aircraft Historian, all rights reserved.

Gulfstream Aerospace C-11A Gulfstream II

Though Grumman had a good aircraft in the turboprop Gulfstream I, it was clear by the mid-1960s that the future of executive transports was jet-powered. A host of new small business jets were coming into service from Cessna, Learjet, Lockheed, and North American, and Grumman needed to keep up. As a result, the company began development of its own "bizjet," the Gulfstream II.

The new aircraft bore almost no resemblance to its turboprop predecessor; only the forward fuselage was the same. Finding the right kind of jet engine was an obstacle, as turbojets were too noisy and smoky, but Grumman settled on the Rolls-Royce Spey turbofan for powerplant. A swept wing offered superb performance; the wing was based on Grumman's A-6 Intruder attack aircraft. Interiors were left to customer preference.

The Gulfstream II was immediately a hit with buyers, and 256 would be built. The basic design would also become the basis for the even more successful Gulfstream series, such as the Gulfstream III and IV and G.550. Ironically, one of the Gulfstream IIs weaknesses was engine noise, and those aircraft not equipped with hushkits have been withdrawn from service. A number are still in service.

N947NA was an "off the shelf" Gulfstream II bought for NASA as one of four Shuttle Training Aircraft in 1980 to train Space Shuttle pilots how to land the aircraft--while simulators were useful, there was nothing like as close to the real thing as NASA could make it. The pilot's seat and instrument panel were modified to be identical to the Shuttle's, while panels were placed to give the pilot roughly the same view; the copilot retained the Gulfstream's usual controls. To simulate the Shuttle's approach, the trainee took the C-11 up to 37,000 feet and put the aircraft in a shallow dive, lowering the main landing gear to slow it down to the Shuttle's gliding speed. The nose gear would be lowered on approach for safety reasons, and at 36 feet above the runway--the Shuttle's height--a light would come on to simulate touchdown. The pilot would then either land normally or take the C-11 up for another pass.

N947NA was based at one of four spots: El Paso or Ellington Field, Texas for training, the Kennedy Space Center (for either training or to act as a chase plane for actual Shuttle landings), and White Sands Space Harbor (for training and to assess flight conditions in case the Shuttle needed to land there). N947NA was retired in 2012 after the retirement of the Shuttle fleet, and was donated to the Evergreen Air and Space Museum.

This was another aircraft I missed in 2015, though I had seen N947NA in its position in the parking lot; at the time, we were all pretty tired and none of us felt like walking over there on a hot day. In May 2024, I made sure to get a picture--it helped that the weather was cooler! Despite sitting outside for awhile, N947NA looks like it just flew in.

M99 Coma Pinwheel Galaxy in Coma Berenices by Steve J Peters

© Steve J Peters, all rights reserved.

M99 Coma Pinwheel Galaxy in Coma Berenices

Messier 99 (M99), also known as the Coma Pinwheel or Virgo Cluster Pinwheel, is an unbarred spiral galaxy in Coma Berenices. The galaxy is a member of the Virgo Cluster. It is about 56 million light years from Earth. Its designation in the New General Catalogue is NGC 4254.

The Coma Pinwheel has a linear diameter of 85,000 light years. It is one of the brighter spiral galaxies in the Virgo Cluster and appears almost face-on.

Even though the Virgo Cluster Pinwheel is almost the same size as the Milky Way it has an estimated mass of 50 billion solar masses, which is only 5 percent of our galaxy’s mass.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Pro
Main Camera: ZWO ASI533MC Pro at -10C
Filter: Optolong L-Pro filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 48 at 120 seconds, gain 101, temp -10C
Darks 30 at 120 seconds, gain 101, temp -10C
Flat 30 at 230 ms, gain 101, temp -10C
Dark Flat 30 at 230 ms gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Added captions in Photoshop CS4

M33 the Triangulum Galaxy by Steve J Peters

© Steve J Peters, all rights reserved.

M33 the Triangulum Galaxy

The small, northern constellation Triangulum harbours this magnificent face-on spiral galaxy, M33. Its popular names include the Pinwheel Galaxy or just the Triangulum Galaxy. M33 is over 50,000 light-years in diameter, third largest in the Local Group of galaxies after the Andromeda Galaxy (M31), and our own Milky Way. About 3 million light-years from the Milky Way, M33 is itself thought to be a satellite of the Andromeda Galaxy and astronomers in these two galaxies would likely have spectacular views of each other's grand spiral star systems. As for the view from planet Earth, this image nicely shows off M33's star clusters and pinkish star forming regions along the galaxy's loosely wound spiral arms. In fact, the cavernous NGC 604 is the brightest star forming region, seen here at about the 2 o'clock position from the galaxy centre.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Pro
Main Camera: ZWO ASI533MC Pro at -10C
Filter: Optolong L-Pro filter
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 60 at 120 seconds, gain 101, temp -10C
Darks 30 at 120 seconds, gain 101, temp -10C
Flat 30 at 100 ms, gain 101, temp -10C
Dark Flat 30 at 100 ms gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Added captions in Photoshop CS4

M104 Sombrero Galaxy in Virgo by Steve J Peters

© Steve J Peters, all rights reserved.

M104 Sombrero Galaxy in Virgo

I liked the look that my Seestar got of M104, the Sombrero Galaxy so I took a closer look with my C11 last night for about three and a half hours.

The Sombrero Galaxy, also known as Messier 104 (M104), is a famous unbarred spiral galaxy. It lies at a distance of 29.3 million light years from Earth in the direction of the constellation Virgo.

The Sombrero Galaxy is known for its appearance, similar to that of a Mexican hat, with a bright white core surrounded by thick lanes of dust and a halo of globular clusters and stars. The galaxy appears almost exactly edge-on when observed from Earth.

There is a supermassive black hole at the heart of the Sombrero Galaxy. It is one of the most massive black holes detected in galaxies near the Milky Way. It is believed to have a mass of at least a billion suns. This would make it about 250 times larger than the black hole in the centre of our galaxy, the Milky Way.


~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus
Main Camera: ZWO ASI533MC Pro at -10C
Filter: Optolong L-Pro filter 1.25"
Filter Wheel: ZWO EFW 5 Mini
Focal reducer: TS Optics 0.63x
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 217 at 60 seconds, gain 101, temp -10C
Darks 30 at 60 seconds, gain 101, temp -10C
Flats 30 at 220 ms, gain 101, temp -10C
Dark Flats 30 at 220ms gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Labels added in Photoshop CS4

M92 Globular Cluster in Hercules by Steve J Peters

© Steve J Peters, all rights reserved.

M92 Globular Cluster in Hercules

It was clear last night so I was able to set up my C11, spend several hours setting up the mount and the scope, faffing about with focus and guiding and calibration frames and all that sort of guff.

Then I pointed at M92, a globular cluster of stars in the constellation of Hercules. A grand sight. For all of 15 minutes before the clouds rolled in. Oh well. At least I got enough data to build this image.

The cluster lies at a distance of 26,700 light years from Earth and has an estimated mass of up to 330,000 solar masses. With an estimated age of 14.2 billion years – almost the same age as the universe itself – M92 is one of the oldest clusters known and possibly the single oldest globular in the Milky Way

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Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus
Main Camera: ZWO ASI533MC Pro at -10C
Filter: Optolong L-Pro filter 1.25"
Filter Wheel: ZWO EFW 5 Mini
Focal reducer: TS Optics 0.63x
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 15 at 60 seconds, gain 101, temp -10C
Darks 30 at 60 seconds, gain 101, temp -10C
Flats 30 at 220 ms, gain 101, temp -10C
Dark Flats 30 at 220ms gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Labels added in Photoshop CS4

M37 January Salt and Pepper Cluster in Auriga by Steve J Peters

© Steve J Peters, all rights reserved.

M37 January Salt and Pepper Cluster in Auriga

While I was setting up my C11 on Sunday I pointed it at M37, known as the January Salt and Pepper cluster in the constellation Auriga. I used these stars to adjust focus and set up tracking as there were plenty of points of reference.
Once that was done I took just three 60-second frames. I was pleasantly surprised at the results I got from just three minutes on this target. Even the red and the blue colours of these stars shows up.

Messier 37 (M37) is an open cluster in the constellation Auriga. It has the designation NGC 2099 in the New General Catalogue. M37 is the brightest, richest and largest of the three open clusters in this constellation that were catalogued by Messier. It has an apparent magnitude of 6.2 and lies at a distance of 4,511 light years from Earth.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus
Main Camera: ZWO ASI533MC Pro at -10C
Filter: ZWO UV/IR Cut filter 1.25"
Filter Wheel: ZWO EFW 5 Mini
Focal reducer: TS Optics 0.63x
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 3 at 60 seconds, gain 101, temp -10C
Darks 30 at 60 seconds, gain 101, temp -10C
Flats 30 at 40 ms, gain 101, temp -10C
Dark Flats 30 at 40ms gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Labels added in Photoshop CS4

M46 Open Cluster in Puppis and NGC 2438 Planetary Nebula by Steve J Peters

© Steve J Peters, all rights reserved.

M46 Open Cluster in Puppis and NGC 2438 Planetary Nebula

Messier 46 (M46) is an open star cluster located in the southern constellation Puppis, the Stern. It occupies an area of 27 arc minutes of apparent sky, almost the size of the full Moon, and has a spatial diameter of 30 light years.

Messier 46 is a relatively bright, large cluster containing about 500 stars. About 150 of its members are of magnitude 10 to 13 and the brightest stars belong to the spectral class A0. These stars are about 100 times more luminous than the Sun. The single brightest star in M46 has a visual magnitude of 8.7.
The cluster’s estimated age is 300 million years.

The cluster has an apparent magnitude of 6.1 and lies at an approximate distance of 5,400 light years from Earth. It has the designation NGC 2437 in the New General Catalogue.

The planetary nebula NGC 2438 appears superimposed on M46 and is located about 7 arc minutes northeast of the cluster’s centre. The nebula is believed to lie in the foreground, at a distance of about 2,900 light years from Earth.

~~~~~

Telescope: Celestron C11-A XLT Schmidt Cassegrain OTA
Mount: SkyWatcher EQ6-R Pro

Controller: ZWO ASIAIR Plus
Main Camera: ZWO ASI533MC Pro at -10C
Filter: ZWO UV/IR Cut filter 1.25"
Filter Wheel: ZWO EFW 5 Mini
Focal reducer: TS Optics 0.63x
Focuser: ZWO EAF
Guide Camera: ZWO ASI174MM Mini guidecam
Guide via: ZWO OAG

Stacked from:
Lights 44 at 60 seconds, gain 101, temp -10C
Darks 30 at 60 seconds, gain 101, temp -10C
Flats 30 at 40 ms, gain 101, temp -10C
Dark Flats 30 at 40ms gain 101 temp -10C

Bortle 4 sky.
Integrated the saved frames in Astro Pixel Processor.
Processed in PixInsight
Labels added in Photoshop CS4