New Camera and Dobsonian Telescope

Testing a New Combination

Although my 12-inch Dobsonian telescope doesn't track stellar motion caused by Earth's rotation, I thought it would be interesting to test short exposure times with my new Nikon Z6 2 camera attached to this large aperture. On February 6th I gave it a try. A special adapter is required to attach the camera to the scope. The camera would not reach focus with first adapter I purchased. Eventually, I bought another adapter that brought the camera's focal plane a couple centimeters forward, enough to achieve focus.

The telescope effectively acted like a 1500 mm telephoto lens. I quickly discovered stars would trail unless exposures were very short. An approximate rule for avoiding star trails in unguided photos is to keep exposure times in seconds less than 500 divided by the lens focal length. For my telescope the rule said 500/1500 = 0.3 seconds would be the longest exposure I could take. Trial and error proved the rule accurate. To compensate for short exposure time I cranked the ISO up to 51200! The next image is a 0.3-second exposure of the Orion Nebula, M42, at ISO 51200. In spite of background noise associated with high ISO the image captured a lot of detail in only 0.3 seconds!

The Pleiades were high in the sky above most light pollution before the Moon rose. Another 0.3-second exposure at ISO 51200 captured only part of this cluster as seen in the next image. I should have moved the field of view around, taken a series of images, and then combined them to capture the entire cluster. Maybe I'll try this another time. The diffraction spikes on bright stars are kind of pretty!

I was particularly interested to see how Jupiter would look in a short exposure. The following 0.05-second exposure at ISO 500 overexposes the planet but allows all four major Jovian moons to be visible.

Based on the previous picture it looks like this particular telescope/camera combination might be great for capturing certain kinds of planetary conjunctions.

On this night, February 6th, comet C/2022 E3 ZTF was passing near the star, Capella, in the constellation, Auriga. I searched the neighborhood of Capella while looking at the camera's viewfinder screen, but couldn't find the comet. Instead, I took a picture of bright Capella itself with a 0.3-second exposure at ISO 51200. Yellow overexposed Capella shines nicely with accompanying diffraction spikes in the next image.

In my light polluted sky I misidentified the star Almach in Andromeda and photographed Mirach instead. I was surprised to see a faint, fuzzy object to the lower right of bright Mirach in the following image. The faint object is actually the 10th magnitude elliptical galaxy NGC 404! It's amazing how this faint distant object actually showed up in just a 0.3-second exposure at ISO 51200!

Finally, I tried a 0.2-second exposure at ISO 51200 to capture most of the star cluster, M41, in Canis Major. 

Soon after capturing M41 the nearly full Moon rose making the sky even worse for imaging. It was time to quit.

These results with very short exposure times make me wonder how nice it would be to have a 12-inch telescope on a tracking equatorial mount. Longer exposures with no star trailing would really show amazing stuff!

Comet C/2022 E3 ZTF

Partial Success

Almost all comets I've been able to observe have been difficult targets. They usually appear inconveniently close to the horizon, often before dawn when it's hard to get out of bed. Recently, prominent comet C/2022 E3 (ZTF) had an orbit bringing it close to the north celestial pole, so, for a good stretch of days, the comet was located relatively high in the sky to the north.

The comet's unfamiliar name has the following explanation according to earthsky.org: "It was discovered on March 2, 2022 and it was the third such object discovered in the fifth half month (A, B, C, D, E) of the year". (E3) It was discovered by a 48-inch telescope on Mount Palomar which is part of the Zwicky Transient Facility (ZTF). The C indicates it is a non-periodic comet.

I made several attempts to photograph the comet with my new Nikon Z6 2 camera. The first attempt on January 15th was successful as you can see in the following image which was constructed by stacking five 30-second guided exposures with a 70 mm f/2.8 lens at ISO 800.

The green coma and brighter part of the yellow dust tail are visible. Ultraviolet light from the Sun excites diatomic carbon present in gases emitted by the comet. The excited diatomic carbon then emits a green visible color. The dust tail's yellow color comes from reflected yellow sunlight. Darker skies, larger apertures, longer exposures, and telescopic magnification would be needed to reveal the long, dim, wispy ion tail which is not visible above.

I tried again on January 24th when the comet was closer to Earth. The next image is a stack of six 6-second unguided exposures at ISO 6400 with the 70 mm lens set at f/2.8.

Now the comet tail had spread out into a fan shape with a spike pointing ahead of the coma. This is a little easier to see in the following heavily enhanced, cropped image. Enhancing the image to reveal dim details also, unfortunately, brightens background noise. Therefore, the background sky doesn't look as black as it should. (All these images should be enlarged to see the comet in better detail.)

Viewing conditions were much more difficult on January 30th, two days before the comet made its closest approach to Earth. On this night the temperature was wonderfully mild, but the Moon was almost full, and the sky was covered with hazy thin clouds. In addition, it was very humid, and dew rapidly formed on exposed surfaces. Since the comet was closer to the celestial pole this night, I tried a slightly longer exposure time with the unguided camera mounted on an ordinary stationary tripod. The next image is a stack of nineteen 8-second exposures at ISO 6400 with the 70 mm lens at f/2.8.

Unfortunately, haze and moonlight worked together to diminish what should have been a brighter coma and possibly longer dim tail. 

The sky was completely overcast when the comet came closest to Earth on February 1st. After February 1st there were a few more opportunities for interesting comet pictures. For example, on February 6th the comet passed close to the bright star, Capella, in the constellation, Auriga. The Moon was nearly full that night when I tried imaging the comet with a 12-inch Dobsonian telescope. Unfortunately, I couldn't find the comet in the telescope's relatively small field of view. On February 10th the dimming comet passed close to Mars, but the sky was cloudy again. Clouds were forecast for almost every night after February 10th. The comet will rapidly dim as it recedes from the Sun and Earth and travels out into the solar system.

Venus-Saturn Conjunction

Pretty Scene at Dusk

Close after sunset on January 23rd Venus and Saturn were only about 1.25 degrees apart as they sank in the western sky below a nice crescent Moon. My new camera produced this nice image which is best viewed at full size. (Bright Venus is above dim Saturn.)

Earthshine on the Moon adds to the beauty! On the previous evening the planets were even closer together - only about 1/3 degree apart. Unfortunately, it was cloudy on January 22nd.
 

Constellations

New Nikon Z6 2 Camera

I've grown increasingly frustrated with the limited capability of my phone camera for night sky photography. The phone is conveniently portable and easy to set up, but the simple phone lens, restricted exposure times, and low available ISO values always make me wish for more. So I was excited to see how a newly purchased Nikon Z6 2 mirrorless camera would perform when imaging starry skies.

The new camera, with its 24-70 mm f/2.8 lens, is a beauty, although the number of small control buttons makes it look like it's suffering from control button pox!

Check out all the tiny buttons on the back. 

I've been finding it hard to work these controls with cold fingers in the dark! Notice the large view screen which acts like an excellent viewfinder. It makes focusing on dim targets much easier than squinting through a small viewfinder.

I hurried to use the camera on January 9th, the first clear night available, and set it on an ordinary camera tripod for some trial exposures. The next image is a 6-second unguided exposure at ISO 800 with the lens set at 49 mm and f/2.8. Orange colored Mars is the bright object between the V-shaped Hyades Cluster of Taurus below center and the Pleiades cluster above center. Wow! I was pleasantly astounded by the number of stars visible and how well they were focused. If you enlarge this image to 100 percent, you'll see how amazingly sharp it is! It looks best when enlarged.

In order to increase exposure time and magnification the camera needs to be attached to a polar aligned mount with a motorized drive that follows Earth's rotation. I haven't had much luck with ordinary camera tripod drives. I find them too fragile and easily knocked out of polar alignment when moving a camera to different views. So I attached the new Nikon to my sturdy, solid Paramount MX telescope mount as seen below.

This setup is obviously more complicated than a simple camera tripod. It also requires a laptop to initially start up the mount. But the camera can be pointed in all directions without disturbing polar alignment. After initial start up the laptop isn't required for pointing because the mount can be moved with a hand controller alone. Notice the red band wrapped around the forward end of the lens. 

This is a Haida dew heater which prevents dew or frost forming on the lens as temperature drops during the night. Dew covered lenses have endlessly frustrated me in the past! This dew heater works perfectly!

I was now ready to try longer guided exposures and higher magnification. On January 15th skies were clear again. Temperatures in the low 30's made me suffer, but I managed to obtain some good images through lots of trial and error. For example, the next picture is the constellation, Auriga, showing the bright star, Capella, in the upper left and Auriga's three major star clusters, M38, M36, and M37 arrayed top to bottom on the right of center. The winter Milky Way runs through the center of Auriga and you can see the huge number of stars captured in this image. The image was constructed by stacking five 30-second exposures for an equivalent 2.5 minute single exposure. The lens was set at 70 mm and f/2.8, and ISO was 800. Enlarge the image by clicking on it to see it in best detail.

Notice the apparent lack of color in Auriga's stars. Capella should be yellow. At this point I hadn't yet learned enough to make star colors more apparent.

The Paramount isn't perfectly polar aligned, but the inaccuracy usually doesn't cause much star trailing in 30-second exposures. Also, 30-second exposures are the maximum the camera allows unless an external controller manages the "bulb" exposure setting. I need to explore longer exposures in the future.

Another successful image was obtained by stacking three 30-second exposures of a portion of the constellation, Andromeda. This portion contained the Andromeda galaxy, M31, as you can see below. The lens was set on 70 mm and f/2.8, and ISO was 800. Once again, the image needs to be enlarged to see hints of a dust lane in M31 as well as M31's small companion galaxy, M110, to the right of M31.

Mount tracking was slightly inaccurate during this Andromeda exposure. Stars are slightly elongated. Color is also lacking in the image.

I eventually discovered color appears when choosing higher ISO numbers and using different options during the stacking process, including specifying HDR (high dynamic range). For example, look at the next image of the constellation, Canis Major. The bright star, Sirius, has a distinctive blue color. This image was made by stacking three 30-second exposures made at ISO 3200 with lens setting 70 mm and f/2.8. Star cluster M41 is visible below Sirius. Enlarge the image to see best detail.

Notice the incredible number of stars visible! These really are stars because I checked their locations on detailed star maps. There is an unfortunate bright background blemish between stars on the left edge of the previous image. Although the winter Milky Way is located to the left of Canis Major, the bright background between stars on the left is likely noise I've failed to eliminate.

Finally, I pointed the camera toward the constellation, Orion, placed nicely high above murky horizon light pollution. With luck, all my neighbors' annoying floodlights were miraculously turned off, so conditions were near the best possible in my back yard. The next picture is a stack of four 30-second exposures at ISO 3200 with lens set at 70 mm and f/2.8. Lots of colors appear! I was honestly exhilarated to see this image emerge from the stacking process! Please enlarge the image to explore its contents.

The Orion Nebula, M42, is shining in Orion's sword. The Flame nebula is visible above the star, Alnitak, on the left side of Orion's belt. Dim red nebulosity containing the Horsehead Nebula is even visible below Alnitak. (The Horsehead itself is a dark indentation in the red nebulosity, but isn't sharply defined.) Also visible is part of Barnard's Loop, a dim red circular arc on the left of Orion's belt. Betelgeuse is orange, Rigel is blue, and the number of visible stars down to roughly magnitude 15 is absolutely amazing! Most of the tiny, tiny dots visible upon enlarging the image are actually stars, not noise! Unfortunately, the image is blemished by hazy bluish background noise which I am not skilled enough to remove. I didn't capture a dark frame or a good quality flat field frame. I'd like to apply these calibration images in the future to see if they will reduce background noise.

I tried increasing ISO to 6400 and made the next Orion image from a stack of only two 30-second exposures with lens set at 70 mm and f/2.8.

There isn't much obvious difference between the ISO 3200 image and the ISO 6400 image, so 3200 might be a good choice for future settings. Now that I know setting combinations that work I'd like to try either stacking more individual images or use exposure times longer than 30 seconds. Better mount polar alignment would help, but, even after years of experience, I still haven't discovered a quick, efficient method of improving the Paramount's alignment beyond rough approximation. 

My ability to tolerate cold night observing and sleep deprivation has diminished with age. It doesn't take long for my fingers to numb and my resolve to weaken. I look forward to warmer weather in the coming months.
 
 

 

Solar Flare

Explosion in Progress

During the morning of October 7th a complex sunspot group produced an M1 class solar flare over a period of about 3 hours. At this time my sky was clear and observing conditions were excellent. For a telescopic sun watcher like me this was like winning a lottery prize! Here's a satellite picture of cloudless Virginia while the flare happened (from the Penn State Weather Wall Map). My observing site is marked with a red X. There was no wind, the atmosphere was steady, and temperature ranged in the upper 60's. Conditions don't get much better than this, although I was buzzed by a few hovering yellow jackets! Two neighboring sunspot groups produced the flare. When I began recording at 13:54 UT (9:54 EDT) the eruption was already in progress. In the next image sunspot group 3116 is on the left and 3112 is on the right. The flare is in the white overexposed areas left of the largest umbra. (Click on the images for enlarged views.)  Later, at 14:35 UT (10:35 EDT), the situation had changed. The next image shows the sunspots 41 minutes after the previous image was recorded. Seven minutes later, at 14:42 UT (10:42 EDT) the white energetic areas deformed further.  My last image, captured at 14:56 UT (10:56 EDT), showed more changes. I quit imaging when seeing conditions worsened. Apparently, I stopped before peak flare output, as you can see in this graph from the Space Weather website. It shows the timing and intensity of the flare. It would have been nice to record a series of evenly spaced images over an hour or more to produce a smooth time lapse flare animation. Unfortunately, it's only possible to animate a time span of 21 minutes between 14:35 and 14:56 UT with four unevenly spaced pictures. The greatest changes happen in the white eruption just above center. Small arching filaments also change shape just to the right of the biggest dark sunspot umbra.  Next is a 9-panel disc mosaic which shows the sunspot group nearly centered. A few filaments are scattered about. There were nice prominences around the solar rim as you can see in the next 15-panel mosaic. The disc has been overexposed to make the relatively dimmer prominences stand out.  Just as in my last observing session, the eyepiece view of prominences was outstanding. The delicate, fan-like prominence on the bottom was particularly beautiful! In the eyepiece the Sun and prominences are a deep red color that I find difficult to faithfully reproduce in my images. The next picture, with overexposed disc blacked out, attempts to capture the eyepiece view. It doesn't quite do the job, however. All images above can be enlarged for a more detailed view. They look best that way.
  

Scattered Sunspots

Good Seeing

Sometimes observing conditions are so good it's worth setting up my solar telescope even if solar features aren't particularly outstanding. September 26th began mild and cloudless with occasional gentle breezes. Temperature ranged from 68 to 73 degrees during the morning observing window. Most importantly, the atmosphere was very steady, so there was "good seeing". No big dramatic solar features were present, just a scattered bunch of relatively small sunspots as you can see in the following 7-panel mosaic. Sunspot 3110 is the dark umbra left of center. A group of small sunspots stretches diagonally upward across the lower right. From left to right they are sunspots 3107, 3105, and 3108. The mosaic image can be enlarged to full size without blurring detail because seeing was so excellent. Next is a single close image of sunspot 3110.  The string of small sunspots 3107 and 3105 are portrayed in the next image which also looks good at full enlargement. Previous images were all made with a solar filter tuned to the exact wavelength of red hydrogen-alpha light at 656.28 nanometers. Tuning the filter away from this wavelength produces an image that fails to show surface spicules and filaments, but still shows sunspot umbras and penumbras. The next image shows many small scattered umbras in the 3107 to 3105 sunspot groups. Unfortunately, this picture has annoying vertical fringes not removed by a flat field frame.  Only one significant prominence was present on the northwestern limb. Notice spiky spicules on the top limb. The excellent observing window only lasted one hour before clouds began appearing on the southeastern horizon. Seeing conditions also deteriorated, so it was time to quit.
 

Active Solar Limb

Prominences All Around

After two months of cloudy, hot, humid weather a mild, cloud free morning good for solar observing arrived on September 15th. The sky was milky white from high thin haze. Temperature ranged from 72 to 75 degrees during my brief 50-minute observing window. Despite a promising 9:40 am start, clouds began appearing at 10:40 am and atmospheric turbulence increased. I always have to hurry to capture images before conditions worsen.

On this day only a few relatively small sunspots were present, but a nice array of prominences were scattered around the Sun's limb. These prominences were spectacularly bright and clear when viewed through the eyepiece of my solar telescope! Image quality below really doesn't match the eyepiece view this time! I wished I could have shared the view with others, but no one was available or interested, so I enjoyed them alone.

The next image is a 6-panel mosaic of the southern solar hemisphere processed to show prominences around the edge. Although the disc is, consequently, overexposed, you can still see two sunspots. The large arching prominence on the lower left is really grand! Northern hemisphere prominences were also numerous as shown in the next 6-panel mosaic. Activity associated with departing sunspot 3098 in the upper right included some spiky eruptions. These show more clearly if you enlarge the image by clicking on it. Here's an enlargement of sunspot 3098 and its spiky emissions. Two sunspots in the southern hemisphere appear in more detail in the following imperfect 6-panel mosaic processed to show disc detail instead of prominences. Sunspot 3102 is on the left and sunspot 3100 is right of center. Next is a closer view of sunspot 3102. This long lasting sunspot previously disappeared around the Sun's western limb almost three weeks ago. As the Sun rotated it then traversed across the solar back side for almost two weeks before emerging around the eastern limb to appear as it does in the image below. The large arching prominence was near sunspot 3102. The suspended arch was considerably dimmer than its base near the limb. I always have trouble making prominences stand out from noisy background. Prominence detail is hardly improved in the following yellow colored image with blacked out disc. I  look forward to cooler weather and clearer sky as autumn begins.