Monday dawned clear and bright so we set up the hydrogen-alpha (Ha) solar telescope and recorded some image sequences. Today was a dull and cloudy day so we spent some time learning new processing techniques for our solar imaging and were rewarded with our best shot yet. The processing of choice was Solar Toolbox — a script package developed for use in PixInsight software — just the set of tools we were looking for! We’ve a long way to go but we think this picture shows great progress!
A design rendering of the SkyShed POD-S Mark 4 – Tall observatory. Image Credit: SkyShed Observatories.
Following the evaporation of our first observatory deal we revisited our pre-purchase research from two years ago. We quickly settled upon the SkyShed Observatories POD-S Mark IV in this project reset. Today we placed our order and paid for the ready-to-assemble kit.
While we were originally hoping for fiberglass construction, the POD-S is built from double-walled polyethylene — much the same as plastic garden sheds. The material actually provides some advantages over other construction but presents an interesting issue: daytime IR heating. It seems white poly is translucent to infrared light (solar heat rays) which causes the interior to heat up. We chose a light gray color which, while not the classic choice for a dome or observatory, we are told will allow less of interior heating, as it blocks more IR than the white color reflects. This flies in the face of the usual reflective white or metallic silver specified for observatories but those buildings aren’t made of polyethylene.
We don’t have production or delivery schedule information at this time (the order’s brand-new) but there are other things to do such as acquiring a new building permit, pulling electrical wire to the telescope pier site, building a warm/control room in a nearby shed.
The bad news is that the deal we made for an observatory building is dead after two years of waiting. We received the news via email this morning. The final straw was that the manufacturer was unable –due to factors outside of his control– to ship the finished package! At a financial loss due to packaging costs, he canceled the deal and will issue a refund. The problem was so bad for him, he’s leaving the US market entirely!
The good news is that we have selected a product we had researched two years ago, along with our original choice. Ironically, we originally bypassed this manufacturer because it was going to be two years before their product could be shipped. Now they ship in 6 to 8 weeks!
We’ll post pictures and identify the new choice once we’ve closed that deal. We’re actually feeling pretty good about this. Except for the time lost not having an observatory.
Our temporary observing setups are assembled on the base/floor of the planned observatory. The light orange bucket, at center, protects an empty electrical conduit that will provide utility power to a permanent pier that will be installed there. In the foreground is a table supporting a light shield for the laptop computer. The large tripod next to the table supports the white light imaging scope. In the background is the Sky-Watcher SolarQuest mount with our Coronado hydrogen-alpha solar scope attached.
We’re still doing open-air astronomy though we have a nice, solid, clean, and level space to set up our gear! This is the setup we were using today to record the sunspot at active region 4079 as it is about to roll over the solar limb/horizon. Fortunately, though it’s a very temporary setup, the portable gear we use for casual solar imaging is fairly easy to set up.
From an unusual vantage point, a picture of the solar setup used today to record the passage of active region 4079 toward Sun’s horizon. The red object is the planetary camera.
We continued experiments to determine what gear will work together for imaging. There were a few surprises and there’s need for more experimentation. What we settled on for today’s solar efforts is pictured above and includes: Askar 103 APO telescope, Meade LXD75 Goto Mount, TeleVue 2X Barlow, Baader Planetarium Safety Herschel Wedge, and ZWO ASI678MM monochrome planetary camera.
The sun as it appeared at 11:32 AM EDT on May 10, 2025. Sunspot/Active Region numbers are labeled in this image with AR4079 very near the solar western limb or edge.
Although the sky was clear, seeing was a bit shaky so once again, sharpness wasn’t what we’d like. Still, in all, we got the shot we wanted and learned a few things about our astronomy equipment. Also, the sky was blue, the air was pleasant, and birds were singing, so not a bad way to spend a couple of hours.
A closeup view of the sunspot at AR4079. There is a bright line splitting the dark central umbra of the sunspot, the gray penumbra radiating in filaments around it. White cloud-like areas surround the sunspot, especially to its north; called plage, they are associated with areas of concentrated magnetic field.
The patio floor of the observatory awaits its observatory.
Frustration continues as we await word that the observatory has been shipped. We’ll be firing off another query of the manufacturer tonight reminding them, yet again, that we’re still waiting. Not that our questions or complaints have helped move things along. We’ll likely soon go ahead with pulling wiring through the buried conduit — utility power could be helpful even without the building. We hope to install landscape plants next week in the curved area along the north (left) edge of the patio. Our plant of choice is “Creeping Juniper”. Will we need to make some sort of temporary telescope shelter while we await our observatory (telescope shelter) in order to make better use of what we have? Maybe.
The Sun, as it appeared on April 17, 2025, in hydrogen-alpha light. The image was recorded using a Coronado solar telescope, a Sky-Watcher SolarQuest mount, and a ZWO ASI 678MM camera. Photo by James Guilford.
Taking advantage of midday clear skies, Thursday, we set up the hydrogen-alpha telescope and did a little observing and imaging. Seeing conditions were only good but we could make out several prominences along Sun’s limb. (The proms did not record well and we need to figure out how to enhance their visibility in our images.) Most notable, however, was the shear number of filaments in Sun’s northern hemisphere. None visible in the south! Fragments of exploding filaments launched from Sun and produced two CMEs that, when they reached Earth on April 16, caused strong geomagnetic storm activity and widespread auroras. The storm, however, died out before northern lights could be seen here.
The Sky-Watcher SolarQuest mount is shown here aiming our Coronado 60mm hydrogen-alpha solar telescope at Sun.
Aiding in our efforts was a device we used for the very first time in this session: The Sky-Watcher SolarQuest with its HelioFind system. The device is lightweight, easily supported our rather robust Coronado solar telescope, and was exceptionally easy to learn and operate. Essentially, all that was needed was to set the tripod up so that it was level, turn the device on, and let it do its thing! It is powered by four AA batteries, placed inside the unit. As an alt-az mount, no counterweights or muliti-axis balancing was needed; just mount the scope with its balance point at the center of the dovetail clamp. No remote control, no app, the compact and self-contained SolarQuest established GPS contact, leveled the scope, then looked for Sun. The SolarQuest turned and elevated the telescope, quickly acquiring our nearest star. When the motion stopped, we looked through the eyepiece to discover Sun well within the field of view. A few nudges of the system’s adjustment buttons and Sun was centered. Tracking was excellent throughout the observing/imaging session. Provision is made for further refinement of tracking but that adjustment was unnecessary for the day’s activity. The SolarQuest will make our daytime astronomy a whole lot more convenient and enjoyable!
A business-class jet airplane trailing twin contrails is seen in silhouette against the roiling surface of the sun. The image is recorded in hydrogen-alpha light. Photo by James Guilford.
We had just finished setting up for some solar astronomy and tapped the button to begin a video sequence when something flashed across the computer screen. A jet appeared for less than a second, contrails briefly persisting, silhouetted against the roiling solar disk! We’ve only seen this twice while observing Sun, this being the second time, and we only captured this image by shear luck. The first time we witnessed a solar “photo-bombing” was under similar circumstances. Previously, we had completed setup, was refining focus, and just about to begin recording exposures. We missed imaging that encounter by about the same interval as we succeeded this time!
The latest from the manufacturer of our observatory structure: “The [shipping] broker advised me to wait until the 2nd of April USA time to see what extra paperwork there might be under Trump’s tariffs.” It appears to us that our tariff-loving President’s “Liberation Day” will mean more money “liberated” from our bank account.
And so, another delay in shipping, for yet another reason — they recently had to remake the shipping crate due to wood content — costing more money in the end. If the manufacturer had shipped earlier, and from our viewpoint, it appears they could have, this latest mess and expense would have been avoided — it’s not like it was a secret widespread tariffs were coming!
We can only hope all will be resolved and shipping will actually begin early this month. Will we be able to build the thing this summer, a year-plus from our original expectation?
The experience has, thus far, been frustrating, and disheartening. We have little faith the path ahead will be smoother.
Note: We know of no U.S. manufacturer of small observatories made of fiberglass or non-metal materials. These unique products are imported and subject to shipping charges and import costs such as tariffs.
Just when we thought the manufacturer of our observatory was actually about to ship, they report new problems causing yet another delay. This time it has something to do with a tropical cyclone hitting their port, and port officials later demanding certification that the wood pieces of the crate are safe (presumably from insect infestation) for international shipping. Now a replacement crate is being built from plastic and metal parts. This, by the way, was previously promised over the Christmas/New Year’s holiday. Still hoping we can maybe get the thing here and built sometime this summer. Another week, another delay, another sad disappointment.
The total lunar eclipse of March 13 – 14, 2025 did not disappoint! We resolved to capture images from the late partial eclipse to maximum eclipse, mostly to be able to fit in a little sleep! Catching it all, which we could from our North America location, would have required, essentially, an all-night session. Just a bit too much!
Early partial eclipse. The brighter shadow within the penumbra lights the top portion of this image. Note a bit of reddish tone within the dark umbra. 2:08 AM EDT
I sat on a pad over the paved surface where in the cold, where the observatory is to eventually stand. The old telescope mount ticking away as it tracked the moon across the sky. Occasionally geese and ducks on the nearby pond called out against some unseen disturbance. The stars of Great Orion were sinking behind nearby trees.
Moon is deep within the umbra and last penumbra light about to be left behind. 2:19 AM EDT
In the otherwise quiet chill, I watched the lunar transition, from a bright sliver left over from the night’s Full Moon, to glowing copper orb. With a cable release I manually triggered the camera’s shutter: click — pause — click, to record the event.
Maximum eclipse. Moon is fully within the umbra but because it is not traveling through the center of Earth’s deepest shadow, scattered light from the penumbra brightens the upper limb. 2:58 AM EDT
Shortly after maximum eclipse (shown above), at 2:58 AM EDT, I shut down the telescope and, casting a wistful eye at the still-darkened Moon, went indoors. I fed the waiting cat, changed back to pajamas, and returned to bed. In fitful sleep, somehow still cold, happy to have sacrificed rest for the experienced phenomenon.
Tech: Askar 103 ED telescope, Canon EOS 5D Mk 4 camera, Meade Goto Mount, Photoshop. ISO 400, variable exposure times.
The total lunar eclipse of November 8, 2022, as viewed from Medina County. Photo by James Guilford.
In the wee hours of Friday, March 14, the Full Moon will pass through Earth’s shadow in space resulting in the coppery-red colors of a total lunar eclipse. While skies are expected to be clear for the event and temperatures tolerable, the show won’t be in “prime time” — maximum eclipse and color will be on display at about 2:58 AM (EDT) Friday. This will be the only total lunar eclipse of 2025.
While the timing of this year’s eclipse may be brutal, it also means the entirety of the process will be visible. By 12:55 AM (an hour after midnight, to be clear) Moon will have a strangely soft, faded appearance, then lit by the diffuse light of Earth’s outer shadow or penumbra.
The partial eclipse begins at 1:09 AM and by 1:47 AM, half of the lunar disk will be dark, hidden in Earth’s deep inner shadow called the umbra. Darkness will progress across Moon and as the last light fades from the lunar surface, color will begin to appear with the onset of totality.
A total lunar eclipse occurs when Moon passes through the central portion of Earth’s shadow, known as the umbra, where all direct light from Sun is blocked and Moon is illuminated only by scattered light passing through Earth’s atmosphere.
At 2:26 AM, with Moon totally inside the umbra, the spooky beauty will be on full display. Earth’s inner shadow is full of colored light — sunlight scattered through the planet’s atmosphere bearing the scattered colors of the globe’s sunrises and sunsets — the source of a total lunar eclipse’s hues.
Maximum eclipse is reached at 2:58 – 2:59 AM and Moon will be as dark and colorful as it can be during the process. The eclipse sequence begins to reverse after the maximum as Moon continues its passage through Earth’s shadow. Observers will note the darker and lighter portions of Moon’s face subtly rotating as the event unfolds because Moon is not passing directly through the center of the umbra — the upper portion of the disk will be near the edge of the shadow area, the lower portion closest to the center and darkest region.
The timing and appearance of the March 14, 2025 total lunar eclipse is illustrated here. Note the penumbra and umbra shadow areas and the rotating shadow distribution on the lunar surface. Movement is right to left. Illustration Credit: NASA Scientific Visualization Studio
By 6:00 AM Moon will have returned to its Full illumination as if nothing had happened. Those who potentially lost sleep watching, however, will perhaps yawn but be will gratified to have seen one of the most impressive and beautiful astronomical events available to us.