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Showing posts with label New York Astrophotography. Show all posts
Showing posts with label New York Astrophotography. Show all posts

Saturday, August 22, 2026

Green Airglow Through Thin Clouds – Swain, New York

Green airglow visible through thin atmospheric clouds near Swain, New York
Green airglow shining through thin atmospheric clouds in the night sky near Swain, New York on August 15, 2026. Canon EOS Ra, EF 16–35mm f/2.8L II at 16 mm, f/2.8, ISO 40000, 25 seconds.

On the night of August 15, 2026, near Swain in western New York, I was photographing the night sky with my Canon EOS Ra. The sky was dark enough that a noticeable green color from atmospheric airglow was visible across much of the photograph.

What caught my attention was not only the green sky, but also the thin atmospheric clouds crossing parts of the frame. Stars remain clearly visible through them, showing that these clouds were optically thin.

Most of the thin clouds lie outside the brightest part of the Milky Way and appear greenish against the strong green airglow background. Small portions that cross the Milky Way appear somewhat warmer or more reddish. The effect is subtle, but it raises an interesting question: why can thin clouds appear green at night?

Green Airglow High Above the Clouds

The green night airglow is produced mainly by atomic oxygen emitting at a wavelength of 557.7 nm. The strongest part of this emission comes from Earth's upper atmosphere at roughly 90–100 km altitude, far above ordinary weather and tropospheric clouds.

The atmospheric clouds in these photographs are much lower. Because they are thin enough for stars to remain clearly visible, a significant part of the green airglow coming from above and behind them can simply pass through the cloud layer.

The clouds can also scatter some of the surrounding light. However, scattering by cloud droplets and ice crystals is different from the Rayleigh scattering by molecules that makes the daytime sky blue. Cloud particles are much larger and their scattering is considerably less selective by wavelength, so a thin cloud can retain much of the color of the illumination and sky background around it.

Different from Light-Polluted Clouds

This appearance is very different from the clouds we commonly see near cities. Under a light-polluted sky, clouds can become white, yellow, or orange because they reflect artificial light coming upward from the ground. Thick clouds may become much brighter than the clear sky, while stars behind them disappear completely.

Here the situation is almost the opposite. The clouds are faint and transparent, stars remain visible through them, and much of the observed color appears to come from the natural night-sky background rather than from strong artificial illumination below.

There is another subtle detail in the main photograph. Where the background sky is dominated by green airglow, the transparent clouds appear greenish. Near some of the more reddish regions of the Milky Way, their color also seems to shift slightly toward warmer tones.

The Canon EOS Ra has enhanced sensitivity to red astronomical emission, particularly around the H-alpha wavelength at 656.3 nm, so reddish emission regions along the Milky Way can be recorded more strongly than with a standard digital camera.

Why This Effect Is Easy to Overlook

Greenish atmospheric clouds are not necessarily rare in night-sky photographs, but the effect is easy to overlook. In many astrophotographs the green color is simply described as airglow, while the clouds themselves are treated as an unrelated foreground or atmospheric feature.

The important distinction is that the clouds are not producing airglow. The green emission originates much higher in Earth's atmosphere, while ordinary weather clouds are far below it. When those clouds are optically thin, part of the green airglow remains visible through them, and the cloud-covered part of the sky can therefore appear greenish in the photograph.

This can easily be confused with several other effects: light pollution reflected from clouds, aurora, camera white-balance shifts, or simply aggressive color processing. The most useful clue is that stars remain visible through the clouds, showing that the cloud layer is transparent enough for the background sky emission to pass through.

For this reason, I think the effect is probably photographed more often than it is discussed. What makes this Swain observation especially useful is the combination of strong green airglow, a dark sky and thin atmospheric clouds, which makes the relationship between the airglow and the cloud color easier to see.

The Effect Was Visible Even in a 2.4-Second Exposure

Green airglow visible through thin atmospheric clouds in a 2.4-second exposure near Swain, New York
A 2.4-second exposure showing green airglow and thin transparent atmospheric clouds with stars visible through them near Swain, New York on August 15, 2026.

Earlier that night, I took this 2.4-second exposure. Despite the very short exposure time, the green background and greenish transparent clouds are already visible, although the Milky Way and faint cloud structure are less detailed than in the 25-second photograph.

I find this short exposure especially interesting because it shows that the green airglow was strong enough to be recorded in only 2.4 seconds. The later 25-second exposure collected much more light and reveals the airglow, Milky Way and thin cloud structure in considerably greater detail.

A Similar Example from Colorado

A very interesting comparison was photographed by Aaron Watson of Skies-Alive Photography near Paonia, Colorado, on May 21, 2025. His photograph, Emerald Green Airglow with Orange Clouds, shows strong green airglow together with clearly visible atmospheric clouds.

The photograph is especially useful for comparison because the clouds near the horizon are orange from artificial skyglow, while the atmosphere behind and above them shows strong green airglow. It demonstrates that airglow can still be visible even when some light pollution is present near the horizon.

My Swain photographs show a different case. The atmospheric clouds are much thinner and more transparent, with stars clearly visible through them. Most of these clouds appear greenish where they are seen against the green airglow background, while small portions crossing the more reddish Milky Way show slightly warmer tones.

Together, the two observations show that the appearance of nighttime clouds depends not only on the clouds themselves, but also on the light coming from different directions. Artificial light from below can make clouds orange or yellow, while natural airglow high above them can create a green background that remains visible through sufficiently thin clouds.

Airglow Is Not Aurora

A green night sky can easily be mistaken for aurora in photographs, but airglow is a different phenomenon. Aurora is produced mainly when energetic charged particles interact with Earth's upper atmosphere and is strongly connected with geomagnetic activity. Airglow, on the other hand, is present even during quiet geomagnetic conditions and is continuously produced by chemical and physical processes in the upper atmosphere.

The intensity of airglow can vary considerably from night to night and across different parts of the sky. Atmospheric tides, gravity waves, changes in temperature and density, and changes in the distribution of atomic oxygen around the mesopause can all affect the brightness and structure of the green 557.7 nm emission.

This is an important reminder that a genuinely dark night sky is not necessarily black. Under good conditions, a camera can reveal green, reddish and other faint emissions produced by Earth's own atmosphere.

Photography Settings

Main photograph:
Camera: Canon EOS Ra
Lens: Canon EF 16–35mm f/2.8L II USM
Focal length: 16 mm
Aperture: f/2.8
ISO: 40000
Exposure: 25 seconds
Date: August 15, 2026
Location: Near Swain, New York

Short test photograph:
Camera: Canon EOS Ra
Lens: Canon EF 16–35mm f/2.8L II USM
Exposure: 2.4 seconds
Date: August 15, 2026
Location: Near Swain, New York

A Dark Sky Reveals Its Own Color

The area near Swain has a very good dark sky for New York State. According to the Light Pollution Map, this location is approximately between Bortle Classes 3 and 4. However, light-pollution maps should be considered an estimate rather than an exact measurement of what an observer will experience on a particular night. Actual sky quality also depends on atmospheric transparency, humidity, aerosols, nearby lights, the time of night and even the surrounding terrain.

Local geography can sometimes create a significantly darker pocket than a large-scale map might suggest. I experienced a good example at Sand Beach in Acadia National Park, Maine. The beach is only about 290 yards long, but the combination of a dark open-ocean horizon and surrounding mountains that shield light from populated areas creates an unusually dark observing location. Only a few miles away, where that terrain shielding disappears, light pollution becomes more noticeable.

One of my own practical indicators of an excellent astrophotography sky is visible airglow. In the original Bortle scale, readily apparent airglow is one of the characteristics of a Class 1 sky. A camera, however, is much more sensitive than the human eye and can record airglow under skies that would not visually qualify as Bortle Class 1.

The strong green airglow near the zenith in these Swain photographs can therefore have several explanations working together. The site was genuinely dark, photo at ISO 40000 was sensitive enough to reveal very faint atmospheric emission, and the green airglow itself may simply have been stronger than average that night because airglow intensity naturally changes with conditions in the upper atmosphere.

For me, this is one reason airglow is such an interesting practical indicator of sky quality. A light-pollution map provides a useful prediction, but the photograph records what the sky was actually doing at that location and at that moment. When natural green or reddish atmospheric emission becomes clearly visible instead of being overwhelmed by artificial skyglow, I know I am photographing under a genuinely good dark sky.

These photographs also show why atmospheric clouds at night do not always have to be white, gray or black. Under a dark sky, a thin transparent cloud can reveal some of the color of the natural sky behind it. On this night near Swain, that color was unmistakably green.

Related Astrophotography Posts

Tuesday, September 22, 2020

Milky Way Rainbow Panorama Canon EOS Ra over Bethel Catskill NY

This image captures a full arch of our galaxy — often called the Milky Way Rainbow. It is my first full-sky panorama of the Milky Way made with the Canon EOS Ra, and another step in testing the camera’s impressive astrophotography performance.

The Canon Ra handles high ISO extremely well, producing low-noise results even at ISO 20,000. Using short 5-second exposures helped avoid star trailing and made the 20-shot panorama quick to capture. A dedicated contrast-enhancing filter helped bring out the structure of the Milky Way, and the final image was created by stitching all frames together in Photoshop.

The foreground shows tall grass with a line of forest farther in the distance. A bit of light behind the camera softly illuminates the landscape, creating depth and atmosphere while preserving the natural nighttime look. Above the scene, the Milky Way forms a complete glowing arch across the sky — a true “rainbow” of our galaxy rising over Bethel and the Catskill region of New York.


Milky Way Rainbow Panorama Canon EOS Ra over  Bethel Catskill  NY Astrophotography
Milky Way Rainbow Panorama Canon EOS Ra over  Bethel Catskill  NY - Astrophotography

Technical details:
Canon EOS Ra • EF 16–35mm f/2.8L II USM • f/2.8 • 5 seconds • ISO 20,000
Panorama of 20 photos

About the Catskill Region

The Catskill Mountains, located in southeastern New York State, are known for their rugged forests, hiking trails, wildlife, and the protected Catskill Forest Preserve. The area offers some of the darker skies in the region, making it an excellent place for landscape astrophotography.

Related Astrophotography Posts

Monday, September 14, 2020

Topaz DeNoise AI Canon Ra Milky Way Astrophotography

Noise is one of the main challenges in astrophotography. Even though the Canon EOS Ra produces noticeably less noise compared to the older Canon 60Da, high-ISO wide-angle images still show visible grain—especially when zoomed in.

Over the years I tried many noise-reduction tools including Adobe Camera Raw, Noise Ninja, and Photoshop’s built-in filters. But Topaz DeNoise AI completely changed my workflow. Its artificial intelligence–based processing gives far cleaner results with less effort, turning amateur astrophotography into almost professional-level output with just one filter.

Topaz DeNoise AI integrates directly into Photoshop, making the cleanup process simple, fast, and extremely effective.

Topaz DeNoise AI before-after comparison Milky Way astrophotography
Topaz DeNoise AI Astrophotography

This screenshot shows a live split-screen inside Topaz DeNoise AI. The left half displays the original noisy image, and the right half shows the AI-cleaned version. This preview uses my real astrophotography frame of the Milky Way’s bright galactic center rising over the forest in Bethel, Catskill, NY. The software allows adjusting settings in real time, so you can immediately see improvements in star sharpness, dust lanes, and sky texture as noise is reduced.

Canon EOS Ra — 5 sec, ISO 20,000, f/2.8, 16mm + Topaz DeNoise AI

Milky Way after Topaz DeNoise AI Canon EOS Ra noise reduction
Topaz DeNoise AI Canon Ra Milky Way Astrophotography


This is the final processed photo after applying Topaz DeNoise AI. Captured using the Canon EOS Ra in Bethel, Catskill, NY, this Milky Way frame becomes dramatically cleaner after denoising. The AI preserves fine structure in the galactic core, enhances contrast, and minimizes high-ISO grain while keeping the image natural and sharp.

Related Astrophotography Posts

Wednesday, August 26, 2020

Canon Ra Panorama Milky Way Toronto Reservoir Bethel, NY

This is one of my early large-format panoramas taken with the Canon EOS Ra. Previous posts featured single exposures, but here I captured a classic wide-field Milky Way panorama composed of 10 separate images, stitched together to reveal far more detail and structure in the galactic core.

The photo was taken at Toronto Reservoir in Bethel, New York, a quiet and scenic area located about 7.7 miles from Monticello in Sullivan County. The reservoir sits in a relatively dark region compared to NYC, making it a great location for astrophotography when the sky is clear.

In the photo you can clearly see the calm surface of the Toronto Reservoir, framed by the dark silhouettes of trees along the shoreline. The water reflects the trees and several bright stars, creating a peaceful mirrored foreground. Above it, the Milky Way stretches like a river in the sky, while the reservoir becomes the river on Earth — both flowing in parallel. A portion of the Galactic Center is also visible, adding extra detail and structure to the panorama.

Canon EOS Ra Milky Way Panorama over Toronto Reservoir, Bethel NY
Canon EOS Ra Panorama Milky Way Toronto Reservoir Bethel, NY

Technical details:
Canon EOS Ra • EF16–35mm f/2.8L II USM • f/2.8 • ISO 6400
Panorama of 10 images, each 8 seconds

Related Astrophotography Posts

Wednesday, July 22, 2020

The comet NEOWISE reflecting in Wesserlauf Pond, Bethel, New York

Comets are like cats: they have tails, 
and they do precisely what they want. 
- David H. Levy

This photo captures Comet C/2020 F3 (NEOWISE) beautifully reflected in Wesserlauf Pond in Bethel, New York. Both the comet itself and its water reflection were visible to the naked eye that night.

On the image, you can see the comet’s bright nucleus, its long tail stretching upward across the sky, and the clear reflection of both the comet and surrounding trees in the pond. The stars are also visible in the water, creating a peaceful double-sky effect.

The comet shows two tails on the photo: the wider yellow-white dust tail and the thinner blue ion tail, which is usually invisible to the human eye but captured nicely by the camera’s sensor. To reduce noise, I used DeNoise AI during processing.


Comet NEOWISE reflected in Wesserlauf Pond, Bethel NY – Canon Ra nightscape
The comet NEOWISE reflecting in Wesserlauf Pond, Bethel, New York

Technical details:
Wesserlauf Pond, Bethel NY • Canon EOS Ra • EF 16–35mm f/2.8L II USM
f/2.8 • 12.5 seconds • ISO 16,000

About Comet NEOWISE

Comet C/2020 F3 (NEOWISE) was discovered on March 27, 2020 by NASA’s NEOWISE space telescope. In July 2020 it became one of the brightest naked-eye comets visible from the northern hemisphere in more than two decades.

NEOWISE displayed a dramatic dust tail and a faint blue ion tail, making it a rare and unforgettable astronomical event enjoyed by millions around the world.

Related Comet Astrophotography Posts

Sunday, July 19, 2020

Comet C/2020 F3 (NEOWISE) Canon Ra Bethel, New York

We are hit by tons of material every day, but it is all dust. 
We are all walking around with comet dust in our hair.
- Don Yeomans

Comet C/2020 F3 (NEOWISE) became one of the brightest comets visible in the northern hemisphere since Comet Hale–Bopp in 1997. On July 17, 2020, it was bright enough to be seen with the naked eye, even from moderately light-polluted locations.

This image was taken in Bethel, New York using the Canon EOS Ra with a 200mm f/2.8 lens. The photograph clearly shows the comet’s bright nucleus and its beautiful dual tail structure — the wider dust tail and the thinner, straighter ion tail extending upward across the frame.

Comet NEOWISE C/2020 F3 with dual tails photographed in Bethel NY using Canon EOS Ra
Comet C/2020 F3 (NEOWISE) Canon Ra Bethel, New York

Technical details:
Canon EOS Ra • EF 200mm f/2.8L II USM • f/2.8 • ISO 40,000 • 2.5-second exposure

Related Astrophotography Posts

Thursday, July 9, 2020

Green Fireflies Night Landscape Bethel New York Canon Ra

Summer in New York brings one of nature’s most magical night displays — the glowing dance of fireflies. On this warm July night in Bethel, New York, the woods were alive with thousands of green light trails flickering under a crystal-clear, starry sky.

This image is a time-lapse composite created from multiple short exposures taken with the Canon EOS Ra astro-modded camera. The combination of fireflies and a quiet summer landscape creates a peaceful yet vibrant nighttime scene.

Green fireflies glowing under a starry summer sky in Bethel, New York — long-exposure composite captured with Canon EOS Ra astrophotography camera.
Green Fireflies Night Landscape Bethel New York Canon Ra

Camera & Exposure Settings

  • Camera: Canon EOS Ra
  • Lens: Canon EF 16-35mm f/2.8L II USM
  • Aperture: f/2.8
  • ISO: 12,800
  • Exposure: Composite of 30 images (3 seconds each)

The astrophotography-optimized sensor of the Canon Ra helps capture subtle green trails of the fireflies while preserving faint stars above. Stacking multiple short exposures reduces noise and reveals a fuller picture of their delicate light patterns as they move through the summer air.

Related Astrophotography Posts

Tuesday, June 30, 2020

Canon Ra Reflection Night Landscape Bethel, Sullivan County, New York Astrophotography

I continue testing my new Canon EOS Ra astrophotography camera. There is nothing quite like a starry, quiet summer night — the Milky Way moving slowly across the sky while the landscape glows softly beneath it.

This photo was taken in Bethel, Sullivan County, New York, an area that became world-famous in 1969 when nearly 500,000 people gathered on Max Yasgur’s Farm for the legendary Woodstock Festival. Today, the region is peaceful, rural, and surprisingly good for astrophotography.

In the image you can see a small local pond reflecting the surrounding trees and several bright stars. Even though it was nighttime, the landscape appears illuminated enough to reveal the details of the trees and water — the only sign that it is truly night is the Milky Way arching above. This is a simple one-shot exposure, but it carries a calm atmosphere that reminds me of childhood fairy-tale stories.


Milky Way Reflection Landscape in Bethel, Sullivan County NY – Canon EOS Ra
Canon Ra Reflection Night Landscape Bethel,  Sullivan County, New York Astrophotography 

Technical details:
Canon EOS Ra • 25 sec • ISO 20000 • f/2.8
Lens: Canon EF 16–35mm f/2.8L II USM • Single exposure

Related Astrophotography Posts

Tuesday, June 23, 2020

Milky Forest – Testing the New Canon EOS Ra Astrophotography Camera

After many years of shooting with my trusted Canon EOS 60Da, I finally upgraded to the Canon EOS Ra — and this image is one of my very first real-world tests. So far, the camera has exceeded my expectations in every way.

This photograph was taken near Bethel Woods, New York. The light pollution is noticeably lower than in New York City, but still present — a good test environment for seeing how well the Ra handles faint details in the Milky Way’s dense center.

Thanks to the EOS Ra’s enhanced hydrogen-alpha (Hα) sensitivity and modern full-frame sensor, the structure of the Milky Way remains beautifully visible even under moderate sky glow. The difference compared to the 60Da is immediately noticeable: stronger reds, more detail in the galactic core, and much cleaner high-ISO performance.


Milky Forest - Testing new Canon EOS Ra astrophotography camera
Milky Forest - Testing new camera Canon Ra

Camera Settings & Performance

Canon EOS Ra
Lens: Canon EF 16–35mm f/2.8L II USM
Exposure: 6 sec
Aperture: f/2.8
ISO: 20,000
Processing: Minimum Photoshop adjustments — this is almost straight out of camera.

The Ra's sensor allows much shorter exposures than the 60Da (which typically required 10–15 seconds for a similar sky brightness). Despite the short shutter time, the Milky Way’s core is sharp, detailed, and clean. High-ISO noise levels are dramatically lower, making the Canon EOS Ra a superb tool for night-sky photography.

Compare My Astrophotography Cameras

Related Astrophotography Posts

Tuesday, September 25, 2018

Tupper Lake New York Adirondack Mountains Astrophotography

Tupper Lake, located in the heart of the Adirondack Mountains, offers some of the darkest accessible skies in New York State. Under optimal conditions, this region approaches Bortle Class 3 — where the Milky Way appears bright and richly structured to the naked eye.

For this session, I intentionally chose the shoreline of Tupper Lake to create a balanced nightscape composition. While much of the Adirondacks is forested, the lake provided an open foreground and subtle sky reflections — adding depth and symmetry to the scene.

The weather was not perfectly clear. High-level clouds were moving across the sky throughout the night. Rather than ruining the session, they added texture and atmosphere to the images.

Even with upper cloud layers present, the Milky Way structure remained clearly visible under these dark Adirondack skies. The shifting clouds created contrast against the star field, giving the night a dynamic and slightly dramatic character.

All images were captured using a Canon 60Da with the Canon EF 16–35mm f/2.8L II USM lens:
30 seconds · f/2.8 · ISO 6400

The Milky Way rises above the calm waters of Tupper Lake, with visible dust lanes and rich star clouds.

Milky Way over Tupper Lake in the Adirondack Mountains under Bortle Class 3 skies, New York
Tupper Lake New York Milky Way Astrophotography

Looking north across the water, the Big Dipper dominates the sky. Its bright stars stand sharp against the Adirondack darkness, enhanced by the open lake foreground.


Big Dipper above Tupper Lake in the Adirondack Mountains, New York night sky photography
Adirondack Mountains Tupper Lake Big Dipper New York Astrophotography

The Pleiades star cluster (M45) sparkles above the dark horizon. In skies this dark, the cluster is easily visible to the naked eye and appears crisp and diamond-like in long exposures.

 
Pleiades star cluster M45 above Tupper Lake in the Adirondack Mountains, New York
Pleiades over Tupper Lake - Adirondack Mountains Astrophotography

In the final image, a thin layer of fog formed just above the surface of Tupper Lake. This low ground mist added depth to the foreground while the Big Dipper remained clearly reflected in the water.

The combination of stars above, drifting upper clouds, subtle fog at water level, and the dark Adirondack treeline created a layered composition — sky, atmosphere, reflection, and forest all in balance.

Moments like this show that perfect astrophotography does not always require perfectly clear skies — sometimes atmosphere adds more character than clarity.


Reflection of the Big Dipper in Tupper Lake with low fog under Adirondack Bortle Class 3 skies
Reflection of Big Dipper - Tupper Lake Astrophotography


Why Tupper Lake Is One of the Best Dark-Sky Locations in New York

  • Near Bortle Class 3 sky quality on clear nights
  • Minimal direct light glare
  • Accessible dark-sky site in the Northeast United States
  • Excellent seasonal transparency in autumn

Compared to urban environments such as Manhattan (Bortle 8–9), the improvement is dramatic. The Milky Way becomes fully visible to the naked eye, and subtle star clouds emerge clearly in photographs.

For astrophotographers in the Northeast seeking darker skies without traveling to the western deserts, Tupper Lake remains one of the strongest options.

Adirondack Public Observatory

Just outside the village of Tupper Lake is the Adirondack Public Observatory, a community astronomy center hosting public star parties and educational programs.

You can read my full visit here:
Adirondack Public Observatory – Night and Day Visit

The observatory sits under these same dark Adirondack skies, making it an outstanding destination for both visual observing and night-sky photography.

Geographic Advantage on the East Coast

Another important advantage of the Adirondack Public Observatory is its geographic position. Located in northern New York, it is among the easternmost dark-sky observatories in the continental United States.

When transient astronomical events become visible shortly after sunset — such as bright comets, novae, planetary conjunctions, or meteor outbursts — eastern observatories can often observe them earlier in the evening compared to locations farther west.

Combined with relatively dark Bortle Class 3 skies, this makes the Adirondack Public Observatory one of the first truly dark East Coast sites capable of capturing such events under good conditions.

Related East Coast Dark-Sky Locations

Monday, July 14, 2014

Canon 60Da Star Trail Astrophotography — Night Sky Rotation, Time, and the Direction of Clocks

This star trail image was captured in Upstate New York using a fixed tripod and a series of long exposures. Unlike minimalist nightscapes, star trail astrophotography requires significantly more post-processing. By stacking multiple exposures, it allows the motion of the stars — the rotation of the sky — to become visible.

Canon EOS 60Da, Canon EF 16–35mm f/2.8L II USM
Fixed tripod, dew heater
37 images · 2 minutes each · ISO 400 · f/4.0


Canon 60Da star trail astrophotography showing counterclockwise rotation of the night sky in Upstate New York
Canon 60Da Star Trail Astrophotography - Upstate New York

Instead of a single very long exposure, this image was created by stacking multiple shorter exposures. A single exposure of this total duration would have been far too bright and noisy. To combine the frames, I used StarStax, followed by additional processing in Photoshop.

Screenshot of StarStax software combining multiple exposures into a star trail image
StarStax — stacking multiple exposures into star trails

For the final image I used the Star Spikes filter.

Screenshot of Star Spikes filter applied to a star trail image to show rotation direction
StarSpikes Pro for Startrails

From this image, it is easy to see that the stars rotate in a counterclockwise direction. This naturally raises an interesting question.

Why do the stars rotate counterclockwise, while the hands of a clock move clockwise?

The answer is astronomical — but not in an obvious way. To understand it, we have to look at history. Mechanical clocks were designed to follow the motion of a sundial, but not the motion of the Sun itself. They follow the direction of the shadow cast by the Sun, which moves in the opposite direction to the apparent rotation of the night sky.

Sundial at Lowell Observatory showing the clockwise motion of the Sun’s shadow
Sundial at Lowell Observatory — mechanical clocks inherited their direction from the motion of the Sun’s shadow

In other words, when we look at a clock, we are not “following the Sun” — we are following the shadow of the Sun.

This is why I like astrophotography. Even a technically complex image can lead to unexpected questions — about time, history, human conventions, and how we learned to measure the world.

“The photograph comes first; the philosophy follows — as a way to understand what the image revealed.”

Related Astrophotography Posts

This star trail image connects both technical exploration of the Canon 60Da and a broader philosophical approach to astrophotography — where images lead to questions about time, motion, and meaning.

Thursday, July 10, 2014

Canon 60Da Milky Way Astrophotography Catskill Mountains Upstate NY New York

Two simple, minimalistic Milky Way images from my first nights testing the Canon 60Da in the Catskills.
Even single exposures showed a huge improvement over my old Canon 40D.

During my early tests with the Canon EOS 60Da in the Catskill Mountains, I captured two very simple single-frame Milky Way images. Both were taken with the Canon EF 16–35mm f/2.8L II USM using only a fixed tripod. Even without stacking, the 60Da immediately revealed more detail and sensitivity than my older Canon 40D.

These photos became some of my favorite early 60Da shots—minimalistic, quiet, and very natural-looking. Sometimes a single exposure tells the story better than a complex stacked image.

“Now I know where the Milky Way comes from.”


Canon 60Da Milky Way astrophotography in the Catskill Mountains with rooftop foreground, minimalistic wide-angle night sky image.
Canon 60Da Milky Way Astrophotography Catskill mountains

This first image became unintentionally philosophical. In the lower part of the frame you can see the roof of the bungalow where we stayed in the Catskills. Just above it, the Milky Way rises perfectly—almost as if it starts right from the roof. A small tree is visible on the bottom-right, and the entire scene is extremely minimalistic.

Camera settings were: 9 sec, f/2.8, ISO 12800 using the Canon 60Da and an ultra-wide 16–35mm lens.

A Tree Under the Milky Way


Canon 60Da Milky Way astrophotography in Upstate New York with tree silhouette and bright Milky Way core in minimalistic wide-angle composition.
Canon 60Da Milky Way Astrophotography Upstate NY New York

The second image shows a large tree in silhouette with the Milky Way rising directly above it. Another very simple and minimalistic frame. It beautifully demonstrates how much more detail the Canon 60Da can capture compared to the older Canon 40D—more stars, better color, and higher contrast in the Milky Way core.

This exposure was slightly longer: 15 sec, Canon EOS 60Da, Canon EF 16-35mm f/2.8L II USM Ultra Wide Angle Lens, F2.8, ISO 12800.

These two early Canon 60Da images became part of two small “visual stories” in my astrophotography. The first story is about the question “Where does the Milky Way come from?” — in the Catskills it seems to rise straight from the roof of our bungalow, and later in Yellowstone it appears to rise from the Old Faithful geyser. Two completely different landscapes, but the same cosmic river flowing upward.

The second story is about trees and stars. The tree in this Catskills image became the first part of a theme I continued years later in Bethel, New York — capturing another tree under the Milky Way and reflecting on the idea that we have more trees on Earth than stars in our galaxy. A simple comparison, but very beautiful in astrophotography.

Related Astrophotography Posts

Tuesday, November 26, 2013

NYC Solar Eclipse

Location: New York City (JFK Airport area)
Date: November 3, 2013

While waiting for the highly anticipated appearance of Comet ISON in late 2013, I took the opportunity to document a partial solar eclipse visible from New York City. Capturing a solar eclipse from an urban environment like NYC is always challenging due to weather, haze, and city infrastructure—but even a partial eclipse at sunrise offers a unique and atmospheric view.

These images were taken during sunrise near JFK Airport, where the low Sun and eclipse geometry created dramatic silhouettes and warm tones. In one of the related photo sets, flocks of birds (mostly seagulls) are visible flying across the partially eclipsed Sun—an unexpected and fascinating detail that adds life and scale to the scene.

Partial solar eclipse over New York City with many seagulls flying across the Sun
NYC Solar Eclipse November 3 2013

Solar eclipse at sunrise near JFK Airport in New York City
NYC Solar Eclipse JFK Airport Sunrise November 3 2013

Partial solar eclipse photographed from New York City
NYC Solar Eclipse

In these additional images, numerous birds—mostly seagulls—can be seen crossing the Sun during the partial eclipse. This rare combination of urban wildlife and celestial mechanics makes the NYC solar eclipse especially memorable.

Related Solar Eclipse Photos from New York

Tuesday, October 29, 2013

NexImage 5 Coronado SolarMax II 60

Sun – October 26, 2013

This session was captured using a Coronado SolarMax II 60 hydrogen-alpha solar telescope paired with a NexImage 5 CCD planetary camera on a Celestron NexStar 4SE computerized mount.

Equipment:
Coronado SolarMax II 60 (H-alpha)
NexImage 5 CCD camera
Celestron NexStar 4SE mount
2× Barlow lens
Processing: RegiStax stacking + Photoshop false color

H-alpha Sun captured with Coronado SolarMax II 60 and NexImage 5 CCD
Coronado SolarMax II 60 NexImage 5

The NexImage 5 CCD camera records high-frame-rate video, allowing multiple frames to be stacked in RegiStax. Stacking improves signal-to-noise ratio and enhances fine chromospheric detail, including filaments, plages, and active regions.

After stacking, the image was processed in Photoshop and converted to false color to emphasize structure and contrast. Although H-alpha light is monochromatic, false coloring helps visually separate surface detail and prominence structures.

Coronado SolarMax II 60 with NexImage 5 mounted on Celestron NexStar 4SE
Telescope Coronado SolarMax II 60, Celestron NexStar 4SE Computerized Mount and NexImage5

This configuration combines the precision tracking of the NexStar 4SE GoTo mount with the high-frame-rate capabilities of a CCD planetary camera. When properly processed, the final image quality depends primarily on the optical performance of the Coronado SolarMax II 60.

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Monday, October 28, 2013

Solar prominences - Coronado SolarMax II 60 Canon 40D

Solar prominences captured with the Coronado SolarMax II 60 using a Canon 40D DSLR on a Celestron NexStar 4SE computerized mount.

Equipment:
Coronado SolarMax II 60 (H-alpha solar telescope)
Celestron NexStar 4SE mount
Canon EOS 40D
2× Barlow lens
Date: October 20, 2013

Exposure details:
ISO 200 · 1/6 second


Solar prominences captured with Coronado SolarMax II 60 and Canon 40D
Solar prominences - Coronado SolarMax II 60 Canon 40D

This image shows solar prominences only. The inner disk of the Sun is intentionally blocked (black area) so the exposure can be optimized for the faint outer prominences extending beyond the solar limb.

Compared to my earlier images taken with a NexImage planetary camera, this session used a DSLR mainly to compare imaging approaches rather than image quality itself. CCD planetary cameras and DSLR cameras each have their own advantages and limitations.

Planetary CCD cameras allow very fast frame rates and are less sensitive to mount stability, but require more time-consuming video stacking and post-processing. DSLR cameras capture single high-resolution frames, which makes post-processing much simpler, but they require a more stable mount and precise tracking.

When both imaging methods are used correctly, the final image quality depends primarily on the optical performance of the Coronado SolarMax II 60, not on the camera itself.


To simplify the setup, I switched from a piggy-back configuration to a direct mounting solution by using the Coronado Dovetail Mounting Plate for PST and SolarMax (Item #MEAD414-1).

Coronado dovetail mounting plate for SolarMax II 60 telescope
Coronado Dovetail Mounting Plate for PST and SolarMax Item# MEAD414-1 and Coronado SolarMax II 60 

With this mounting plate, the Coronado SolarMax II 60 can be attached directly to the GoTo mount, greatly simplifying alignment and tracking.

Coronado SolarMax II 60 mounted directly on Computerized Mount
Coronado SolarMax II 60 and Celestron 4SE Computerized Mount

This configuration made it possible to use even a heavier camera like the Canon 40D while maintaining accurate solar tracking.

In later posts, I show additional solar images captured with this setup and further refinements to the mounting and imaging process.


Related Posts – Coronado SolarMax II 60

Coronado SolarMax II 60 during the 2017 Total Solar Eclipse:

Wednesday, October 16, 2013

NGC7000 North America Nebula with Tripod

NGC7000 North America Nebula, Pelican Nebula,  Elephant's Trunk nebula, Cygnus Milky Way,  Deneb - Wide field astro photo with a tripod

CAMERA: Canon 40D
OPTIC: Canon 16-35mm f 2.8 L II USM
MOUNT: Tripod
EXPOSURE: 40 X 30 sec. (Total: 20 min)
PROCESSING: DeepSkyStacker, Photoshop


NGC7000 North America Nebula, Pelican Nebula,  Elephant's Trunk nebula, Cygnus Milky Way,  Deneb - Wide field astrophoto with a tripod, Astrophotography


 All single photos for this image were taken April 11-12 during meteor shower. I used wide angle camera 108 degrees and tripod. I think it is good configuration to catch meteors. Indeed, I got some meteors, but also I have a lot of just single images without meteor. So I tried to see what I can do to stack all this images to one. For 5 min I got wider field, but for 20 min (40 images) with static tripod sky I my final image had not so big size and I tried to focus only small part of sky like North America nebula. This part of sky is very rich. So some other nebulae are visible on this image.

Notation - NGC7000 North America Nebula, Astrophotography

Thursday, October 10, 2013

Cygnus Milky Way

Wide field astrophotography - Cygnus Milky Way
CAMERA: Canon 40D
OPTICS: Canon 16-35mm f 2.8 L II USM
MOUNT: Tripod
EXPOSURE: 16 x 30 sec. (Total: 8 min)
PROCESSING: DeepSkyStacker, Photoshop


Summer Milky Way

 Summer triangle

Summer triangle

 Cygnus constellation
Milky Way in Cygnus constellation

Thursday, August 23, 2012

Star Trail Astrophotography Canon 40D and Canon 60Da

Eppur si muove (And yet it moves).
Galileo Galilei

Star trails - Astrophotography. The north celestial pole is at the center of all the star trails. Polaris is the bright star near the pole. New York state Catskill mountains.

6 images - 10 min each, Fixed Tripod , ISO 1600 F3.5, Canon 40D, Lens EF28-135mm f/3.5-5.6 IS USM. All of these short exposures together in StarStax. 

Star Trails Canon 40D. 6 images 10 min each, Stack in StarStax. Photohop: Levels, Curve, Shadow Filter Color, Un-sharp mask, Despeckle
Color Star Trails, Canon 40D, Total Time about 1 hour, Stack in StarStax
Canon 60Da, Canon Lens EF 16 35mm f2.8L II U, Fixed Tripod, Dew Heater, 39 images - Exposure time 2 min , ISO 400, Aperture F4.0. Post-processing: StarStax and Photoshop.

Star Trail Astrophotography Canon 60Da - Catskills

Wednesday, August 1, 2012

Celestron Stereo Binocular Viewer # 93691

I recently received the Celestron Stereo Binocular Viewer #93691, and these photos show it mounted on my Celestron 4SE telescope.

Using a binoviewer noticeably changes the visual observing experience. Viewing with both eyes feels more natural and relaxed, and the image appears more immersive — almost like a subtle 3-D or IMAX-style view, especially when observing the Moon and bright planets.

One of the biggest advantages is how comfortable it makes observing. Eye strain is reduced, it is easier to stay focused, and sharing the telescope becomes more enjoyable. This is especially helpful for kids and beginners, who often find it easier to look through a binoviewer than a traditional single eyepiece.

Overall, the Celestron Stereo Binocular Viewer 93691 is a fun and practical upgrade for visual observing. It adds comfort, improves the viewing experience, and makes outreach sessions more engaging.

Celestron 4SE telescope with Celestron Stereo Binocular Viewer 93691 installed
Celestron 4SE and Binoviewer
Celestron Stereo Binocular Viewer 93691 mounted on Celestron 4SE telescope
Celestron Stereo Binocular Viewer  93691 and 4SE
 Celestron 4SE telescope configured with Celestron Stereo Binocular Viewer 93691
Celestron 4SE and Celestron Stereo Binocular Viewer  93691

Conclusion:
After spending time with this setup, the binoviewer has become one of my favorite visual accessories. It may not replace traditional eyepieces for every situation, but for relaxed observing and sharing the sky with family and friends, it adds a sense of depth and enjoyment that makes the telescope feel new again.

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