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Showing posts with label meteor. Show all posts
Showing posts with label meteor. Show all posts

Thursday, August 20, 2026

Meteor over the Milky Way – Swain, New York

Meteor streak over the Milky Way photographed near Swain, New York on August 15, 2026
Cropped view showing a faint meteor crossing the Milky Way during a 308.6-second exposure near Swain, New York on August 15, 2026.

On the night of August 15, 2026, near Swain, New York, I was photographing the Milky Way with my Canon EOS Ra. During one long exposure, my wife and I saw a meteor cross the sky. It was not especially bright, but later I found what appears to be the same meteor recorded in the photograph.

I have watched Perseid meteors before, and even visually this one did not particularly look like a bright, typical Perseid to me. My first impression was that it could be a sporadic meteor. However, August 15 is still within the active period of the Perseid meteor shower, so I wanted to investigate whether it could have been a Perseid — and, perhaps even more importantly today, whether the streak could instead have been a satellite.

Meteor, Perseid or Satellite?

The meteor moved approximately from the upper-left toward the lower-right in the photograph. This is generally the correct direction for an object moving away from the Perseid radiant, which was located toward Perseus on the northeastern side of the sky.

The full photograph contains enough recognizable stars to check the orientation of the camera. The Milky Way crosses the frame, the Summer Triangle is prominent, and Beta Cassiopeiae (Caph) can also be identified toward the left side of the Milky Way.

When the meteor trail is extended backward across the sky, however, it does not line up perfectly with the expected Perseid radiant for August 15. Because this is a wide-angle photograph and the radiant is well outside the frame, simply extending a straight line on the image is only an approximation. Nevertheless, the difference is large enough that I would not confidently identify this meteor as a Perseid.

For now, my preferred interpretation is therefore simple: it is most likely a meteor, and probably a sporadic meteor rather than a Perseid.

Wide-angle view of the Milky Way and Summer Triangle with a faint meteor near Swain, New York
Full-frame 16 mm view showing the Milky Way, Summer Triangle and a faint meteor near Swain, New York on August 15, 2026. Canon EOS Ra, 308.6 seconds, f/2.8, ISO 1600.

Could It Be a Satellite?

With a five-minute exposure, a satellite has to be considered. A satellite normally produces a long straight trail, and a satellite that slowly flares and fades can sometimes look surprisingly similar to a meteor in a single photograph.

I checked available catalogued satellite trajectories for the location and corrected exposure time. There were satellites in this general region of the sky, but I did not find a convincing illuminated satellite that followed the photographed trail at the correct time and in the correct direction. One geometrically interesting satellite candidate was already inside Earth's shadow and therefore should not have been visible by reflected sunlight.

This does not provide absolute proof — very faint satellites and some orbital debris can always make identification difficult — but together with the fact that two of us actually watched the meteor at the time of the exposure, a meteor is by far the more natural explanation.

Photography Settings

Camera: Canon EOS Ra
Lens: Canon EF 16–35mm f/2.8L II USM
Focal length: 16 mm
Aperture: f/2.8
ISO: 1600
Exposure: 308.6 seconds
Date: August 15, 2026
Location: Near Swain, New York

Finding the Exact Time

For checking satellites, the exact exposure time is important. I had photographed my computer clock during the same session and later discovered that the camera clock was approximately 8 minutes 1 second fast.

The meteor image has a camera timestamp of 11:39:19 PM. I also tested my Canon EOS Ra afterward and confirmed that the time stored with a photograph corresponds to the beginning of the exposure, not the end.

After correcting the camera clock, this exposure therefore began at approximately 11:31:18 PM EDT and continued for about 5 minutes 9 seconds, ending near 11:36:27 PM.

I later synchronized the Canon EOS Ra clock with my computer using Canon EOS Utility. This is a very useful setting for astrophotography, especially for meteors, eclipses, satellite identification, or any observation where the exact time matters. It is also important to check the camera's Daylight Saving Time setting; for New York in summer the DST setting should be enabled.

Meteor Photography in the Age of Satellites

There is also something a little frustrating about photographing meteors today. Twenty years ago, when a short unexpected streak appeared in an astrophotograph, a meteor was often the obvious first possibility. Satellites existed, of course, but there were far fewer of them crossing every part of the night sky.

Today the situation is very different. A long exposure can contain one or several satellite trails, and even a short fading streak has to be investigated before calling it a meteor. Sometimes it feels as if photographing a meteor is no longer only about being lucky enough to catch one — afterward you also have to prove that it was not a satellite.

In this case, fortunately, there was something the camera metadata and satellite catalog could not provide: my wife and I were standing under the sky and actually saw the meteor ourselves.

Dark Sky, Airglow and Dew

The area near Swain, in western New York near the Finger Lakes region, 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. One of my own simple indicators of a genuinely dark sky is visible airglow. Under a dark enough sky, especially in long-exposure photographs, the background is often not black at all but can show green or sometimes reddish emission from Earth's upper atmosphere. The noticeable green airglow close to the zenith in this photograph was another indication of how dark and transparent the sky was that night.

There is also one practical challenge when photographing at night in this area: dew can become very strong. During a long astrophotography session the front lens element can gradually fog, even when the sky looks perfectly clear. An anti-dew heater around the lens is highly recommended for long exposures and overnight photography here.

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Monday, October 5, 2020

Watching the sky, Observing meteors, Making wishes - Cherry Springs State Park Pennsylvania

Cherry Springs State Park is one of the darkest places on the entire U.S. East Coast, making it perfect for meteor watching and night-sky photography. During this calm and crystal-clear night, we observed several meteors streaking across the sky. Even the faint ones were easy to see thanks to the park’s exceptional Bortle 2 skies.

Here is a close-up view of one of the meteors captured that night:

Meteor over Cherry Springs State Park Pennsylvania
Meteor over Cherry Spring State Park Pennsylvania

This meteor appears to be a random sporadic meteor, not part of a major shower — a reminder that even on quiet nights the sky always has surprises.

Here is the full wide-angle image from the same moment:

Watching the sky and observing meteors at Cherry Springs State Park
Watching the sky, Observing meteors, Making wishes - Cherry Spring State Park Pennsylvania

Camera setup:
Canon EOS Ra – ISO 10,000 – 15 sec exposure
Lens: Canon EF 16–35mm f/2.8L II USM – f/2.8

Nights like this, sitting under one of the darkest skies in America, always feel magical. A few meteors… a few wishes… and a perfect quiet night at Cherry Springs.

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Thursday, August 18, 2016

Meteor or Satellite? A Perseid Mystery Near the Andromeda Galaxy

This post tells the story of an unexpected discovery while attempting to photograph meteors during the Perseid meteor shower. These images were captured on April 13, 2016, around 5:00 a.m. When I reviewed the first photo, I was thrilled — a bright streak appeared exactly where I had hoped to catch a meteor.

The streak seemed to originate near the Perseid radiant and appeared very close to the Andromeda Galaxy (M31). At first glance, it looked like a classic meteor trail.

Light streak near the Andromeda Galaxy during the Perseid meteor shower
Andromeda galaxy and meteor-satellite steak during Perseid meteor show April 2016 - photo 2

Camera: Canon EOS 60Da
Lens: EF 16–35mm f/2.8L II USM
Settings: ISO 6400, f/3.5, 90 seconds

While reviewing earlier frames, I noticed something even more surprising — another streak, nearly along the same path. Finding one was exciting. Finding two was extraordinary.


Second light streak near Andromeda Galaxy during Perseid meteor shower
Andromeda galaxy and meteor-satellite steak during Perseid meteor show April 2016 - photo 1

Canon 60Da, EF16-35mm f/2.8L II USM lens, ISO-6400, f/3.5, 120 sec.

However, after closer inspection, something didn’t add up. The two streaks appeared on nearly the same line, but pointed in opposite directions. The exposures were taken only about one second apart.

The probability that this was a single meteor is essentially zero — a meteor would have to be unrealistically slow. The chance of two unrelated meteors following the same path within one second is also extremely small.

To better visualize the geometry, I combined both frames into a single composite image.


Combined image showing two opposite-direction streaks near Andromeda Galaxy
Combined image showing two opposite-direction streaks near Andromeda Galaxy

Probability that this is one meteor I think about zero. Difference between these two photos about one second and in this case meteor would be very slow. Probability that there are two meteors also very small. Definitely such situation would look very strange.


After that I googled if somebody had before such photos and can explain it. Immediately got idea that it can be Iridium satellite. When I asked this question on  astronomy forum http://www.astronomyforum.net/ and immediately received recommendation to check http://www.heavens-above.com/ website for Iridium satellites at this time. Actually it was one at about this time!,  but orbit was projected to Orion constellation from my location.

Iridium satellite flare predicted path with timing across the sky from Heavens-Above
Predicted Iridium satellite pass with flare timing and sky path from Heavens-Above

So continue to search if this is bright satellite. Havens-above web site also have this data. There were a lot of satellite so I got problem with calibration of EXIF DateTimeOriginal values the photos. I did couple of photos of computer time and http://www.time.gov/ time and compare with DateTimeOriginal. Difference about 1 hour (58 min) looks like camera not using summer time. After that I founded two satellites which most close to this time and orbit.

IRS-P2 rocket body predicted sky path with timing from Heavens-Above
Predicted IRS-P2 rocket body trajectory with timing from Heavens-Above

Cosmos 2292 satellite predicted path with timing near Andromeda Galaxy from Heavens-Above
Predicted Cosmos 2292 satellite path with timing from Heavens-Above


One actually was in opposite direction (IRS-P2 Rocket) other in right direction and really on very close line and right direction (Cosmos 2292). But my calculation time is 4:57 a.m. - difference about 3 minutes. Probably camera clock not stable or not using start time or it can be other not so bright satellite or something other. Could not prove that these sky steaks is satellite but I believe it is most probable explanation. I added link in my blog to  http://www.heavens-above.com/   website – really amazing and very useful data. Hope my story was interesting and help other in such situation.

What began as a simple meteor hunt became a reminder that the night sky is no longer purely natural — it now includes the visible footprint of human technology.

Comparison with Real Meteors from My Astrophotography

To avoid speculation, I compared the streaks in this post with confirmed meteor captures from my own astrophotography archive. These reference images were taken years apart, using similar long-exposure techniques, and show how real meteors appear in photographs.

During the Perseid meteor shower on August 11, 2013, I captured a bright meteor displaying the classic signature: a short, tapered streak with uneven brightness along its path, clearly pointing away from the radiant.

Another confirmed example comes from Cherry Springs State Park, Pennsylvania, where a single meteor was recorded. That image shows the same typical meteor characteristics — a brief, asymmetric trail with rapidly changing brightness that does not repeat in subsequent frames.

In contrast, the streaks analyzed in this post are straight, uniform in brightness, and appear along the same trajectory in multiple exposures — behavior that is characteristic of artificial satellites rather than meteors.

Related Astrophotography & Sky Phenomena Posts

These posts explore both natural and human-created sky phenomena — from meteors and auroras to satellite launches and atmospheric light effects.

Sunday, August 11, 2013

Perseid meteor shower: This bright meteor August 11 2013

I would rather be ashes than dust! I would rather be a superb meteor, every atom of me in magnificent glow, than a sleepy and permanent planet.
- Jack London

These images capture a bright Perseid meteor photographed on August 11, 2013, one night before the peak of the annual Perseid meteor shower. Perseids are known for their fast velocities and bluish-white color, caused by their high entry speed and ionization of atmospheric gases.

This meteor streaked across the constellation Cygnus, leaving a sharp, luminous trail characteristic of Perseid meteors originating from comet 109P/Swift–Tuttle. The photograph was taken from New York under summer night skies using a long exposure to maximize the chance of capturing a meteor.

Camera: Canon EOS 40D
Lens: Canon EF 16–35mm f/2.8L II USM
Exposure: 2 minutes
ISO: 1600
Mount: Tripod
Date: August 11, 2013

Bright Perseid meteor streaking across the Cygnus constellation one night before peak, August 11 2013
Perseid meteor shower: This bright meteor across the Cygnus constellation
August 11 2013 - one night before maximum. Canon 40D Ultra Wide Angle Canon Lens EF 16 35mm f2.8L II U, 2min, ISO 1600, Tripode, NY Astrophotography

The second image below is a cropped and zoomed-in view of the same meteor, revealing its sharp core and subtle color variations. The bluish-white hue is a classic Perseid signature, produced by the meteor’s extreme atmospheric entry speed of roughly 55–65 km/s as it vaporizes in Earth’s atmosphere.

In the zoomed image, the meteor trail clearly shows a classic Perseid structure: it begins as a thin, faint streak, rapidly swells into a thicker and brighter central section, and then tapers off again as the meteoroid fragments and fully ablates in the upper atmosphere. This changing width and brightness reflect variations in velocity, mass loss, and ionization along the meteor’s path.

Because this image was captured as a 2-minute long exposure, the stars do not appear as points but as short arcs, reflecting Earth’s rotation. Despite this, the Cassiopeia constellation is still identifiable in the lower-left corner of the first (wide-field) image, although it falls outside the frame in the zoomed view.

Using Cassiopeia as a reference and comparing the field orientation with a Stellarium sky map, the meteor’s trajectory can be traced back toward the Perseids radiant, which lies just outside the image frame. This confirms the meteor’s direction of motion from lower-left toward upper-right, consistent with a Perseid origin.

Notably, the meteor’s structure also supports this identification: the section closer to the radiant (the beginning of the trail) appears longer and fainter, while the terminal portion farther from the radiant is shorter, brighter, and sharper. This asymmetry reflects the rapid increase in ablation and brightness as the meteoroid penetrates deeper into the atmosphere.

The longer, fainter beginning of the meteor trail can be explained by a combination of perspective effects and atmospheric physics. Near the Perseids radiant, the meteor’s motion is largely along the line of sight, producing a foreshortened, slow-appearing streak. At these very high altitudes, the atmosphere is extremely thin, resulting in faint emission that can extend over a comparatively long visible path.

As the meteoroid penetrates deeper into the denser mesosphere, ablation increases rapidly, producing the bright, thick central section of the trail. Once the particle is fully consumed, the light drops off abruptly, creating a short, sharp terminal end rather than a gradual fade.

Zoomed-in crop of bluish-white Perseid meteor showing sharp luminous trail, August 11 2013
Perseid meteor shower: This bright meteor August 11 2013, Canon 40D Ultra Wide Angle Canon Lens EF 16 35mm f2.8L II U, Astrophotography

Together, the meteor’s color, direction, brightness profile, and changing trail structure all point to a classic Perseid meteor captured under summer skies just before peak activity. Even in a single long exposure, careful analysis reveals both the geometry of the radiant and the physical processes governing meteoroid ablation high above Earth.

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