Bright NLC in moonlight

Looked out the living room window and saw bright noctilucent clouds low in the sky. Packed up cameras etc and jumped in the car and drove off. Chose a place with a low horizon in the north and easy to bring the equipment from the car. When I have just started preparing for the photo I hear steps in the dark and turn on the headlamp and also see a pair of eyes in the dark. After a while I see that it is a deer buck coming straight towards me. He comes very close and looks at me before he heads off, a powerful meeting in the dark.

In the sky the noctilucent clouds are low in the north but they are very bright and beautiful. The moon is up and creates nice moonlight over the landscape. Choose to do some timelapses and macro/widefield pictures, a nice night and the darkness is on its way back.

 

The Sun

 

Sunny days and the sun shows several sunspots and prominences. The images were taken with Ha and CaK filters, different wavelengths.

 

A CaK filter (Calcium K-line filter) is a specialized solar filter for telescopes that isolates light at a specific wavelength of 393.3 nm in the deep violet/near ultraviolet (UV) spectrum. The filter is used in astronomy to observe and photograph the sun, as it makes the lower chromosphere and the border region with the photosphere visible.

 

H-alpha solar filterH-alpha solar filterA H-alpha (Hydrogen-alpha) solar filter is a specialized and advanced optical system that isolates an extremely narrow light wavelength of 656.28 nanometers (nm), which makes it possible to safely observe the sun's chromosphere. Unlike regular white light solar filters, an H-alpha solar filter shows dramatic details such as prominences (gas clouds ejected from the edge), filaments, sunspots and solar flares.

Bright NLC´s

 

Noctilucent clouds are the highest clouds in Earth's atmosphere, forming in the mesosphere about 76 to 85 kilometers (50 miles) above the surface.

Meaning "night-shining" in Latin, they appear as electric-blue, silvery, or glowing wisps during summer deep twilight when they are illuminated by the sun from below the horizon.

Noctilucent clouds (NLCs), also called polar mesospheric clouds (PMCs) when viewed from space, are a tenuous atmospheric phenomenon. Unlike typical weather clouds that form less than 12 miles above Earth, NLCs occur at the very edge of space.How

For noctilucent clouds to form, three precise ingredients are required:

Extremely Low Temperatures: Temperatures in the mesosphere must drop below -120°C to -140°C.Water

Trace amounts of water vapor must be present.

Tiny dust particles are needed, primarily from micrometeors burning up in the atmosphere.

Water vapor freezes onto the meteoric dust to form microscopic ice crystals, which reflect sunlight. Their striking blue color is a result of the ice crystals scattering sunlight in the upper atmosphere.

Noctilucent clouds are a seasonal and latitudinal phenomenon. They occur only during the summer months when the upper atmosphere above the polar regions experiences its coldest temperatures.

Northern Hemisphere: Best viewed between mid-May and mid-August, primarily at mid-to-high latitudes (roughly 45° to 80° North, including northern Europe, Canada, and the northern United States).

Southern Hemisphere: Best viewed between mid-November and mid-February

Photos taken in Vallentuna Sweden 16-17/7 2026.

Night sky disappearing?

Is this night sky soon gone forever?

We have light pollution, Starlink satellites, and soon maybe sun-reflecting satellites too?

 Light pollution is the overuse or misdirected use of human-made artificial lighting outdoors, altering natural light levels at night. This global environmental problem obscures the starry sky, wastes energy, and harms both human health and ecosystems.

 More than 10,000 Starlink satellites currently orbit the Earth. We see them crawling across dark skies, no matter how remote our location, and streaking through images from research telescopes.

SpaceX recently announced that it wants to launch one million more of these satellites as orbital data centres for AI computing power.

 Mirrors in Space? The FCC Just Approved a Sun-Reflecting Satellite, and Astronomers Are Worried

For now, a single satellite has been cleared for a test demonstration, but the company making it hopes to eventually launch 50,000 of them into orbit.

 This picture was taken on the southern part of the island of Zakynthos, Greece, during a family vacation. Most of the island has light pollution that ruins the night sky, so we took a drive to the southern part where there is no city. And the next mainland to the south is Libya, so the sky was amazingly dark and beautiful. The center of the Milky Way appeared as a cloud in the night sky.

 It would be devastating in many ways if the night sky disappeared more and more, even today not many people have seen a truly dark starry sky. The only way for us to realize our place in the universe, how small we are and that we have to take care of each other.

Great sunspots

Several sunspot groups with active areas. Many eruptions have occurred from these areas in the days, some strong, and have now created auroras as far south as +36 New Mexico. Here in Sweden it is far too bright right now for us to be able to see any auroras. Today's images were taken with CaK filter 394 nm which is in the border area between the photosphere, which is visible in white light, and the sun's chromosphere, which is reserved for narrow-band H-alpha filters. In addition to the structures known from white light, such as sunspots, the network of chromospheric flares distributed over the entire solar surface also becomes visible, which precedes the formation of sunspots, as well as supergranulation cells and Ellerman bombs.

Noctlicent clouds and owls

A clear summer night with fog over open areas. Noctilucent Clouds are visible in the sky. All around me I heard screams in the trees and saw several owls, Strix aluco owls, chicks screaming for food. I managed to catch one of them flying between the trees.

Noctilucent Clouds are thin clouds of ice crystals that form at an altitude of 85 kilometers in the mesosphere. They are the highest clouds on Earth and are visible during the summer months when they are illuminated from below by the sun which is then below the horizon

Active Sun

 A really lovely view through the scope today! A lot of activity at the sun with some great prominences today.

Wonderful prominence

A beautiful view through the Ha solar filter the other day with a fantastic prominence at the eastern limb. 

A prominence on the western edge of the sun is escaping into space. A prominence is a huge, arc-shaped cloud of hot gas and plasma held in place by the sun's strong magnetic field. If the magnetic field becomes unstable, the entire structure can rupture and be hurled into space at a speed of several million kilometers per hour. The image was taken on May 22, 2026 from the Carpe Noctem Observatory in Sweden. 

The Sun 24th of may 2026

A clear morning, but a very turbulent atmosphere and poor visibility. But I still took a chance on taking some pictures. It turned out 4 exposures with 200 stacked sequences per image, then stitched together in Photoshop.

Solar activity on May 24, 2026 is at an elevated and very active level, which is expected as we are close to the expected maximum period of solar cycle 25. Main measurements and events. During the last 24 hours, mainly C-class eruptions have been recorded, including two C3 eruptions early in the morning. The total number of observed sunspots remains high, indicating a continued high potential for further eruptions (such as M or X-class) in the next 24 hours. The last geomagnetic storm noted was at level G2 (moderate storm) on May 16, and currently there are relatively calm geomagnetic conditions.

Solar Prominence

In solar physics, a prominence, sometimes referred to as a filament,[a] is a large plasma and magnetic field structure extending outward from the Sun's surface, often in a loop shape. Prominences are anchored to the Sun's surface in the much brighter photosphere, and extend outwards into the solar corona. While the corona consists of extremely hot plasma, prominences contain much cooler plasma, similar in composition to that of the chromosphere. Prominences form over timescales of about a day and may persist in the corona for several weeks or months, looping hundreds of thousands of kilometers into space. Some prominences may give rise to coronal mass ejections. Exact mechanism of prominence generation is an ongoing target of scientific research. A typical prominence extends over many thousands of kilometers; the largest on record was estimated at over 800,000 km (500,000 mi) long, roughly of solar radius. Photos taken back in 2022 using my Ha Solar filter and telescope.

Our star

Our beautiful star keeps our planet alive; without it there would be no life. On this warm sunny day the viewing was very nice, with a calm atmosphere and no major turbulence. The view through the eyepiece was fantastic! There was a lot of activity on the solar surface with active areas around sunspots and larger filaments. On the edge of the sun there were fantastic prominences; they were significantly larger than our own planet.

Half-cloudy in the morning and I took the opportunity to look at the sun between the clouds. Quite turbulent atmosphere and a bit poor vision, but tried to photograph the entire solar disk with 5 images then stitched together in Photoshop. The first thing I noticed were all the filaments on the sun and a couple of nice prominences (now it's the same thing but from different angles).

A filament on the sun is a large, winding cloud of hot gas (plasma) that is held above the sun's surface by strong magnetic fields. Since the gas is slightly cooler than the surrounding sun's surface, they look like dark, thread-like structures when you photograph the sun straight ahead.

If the same phenomenon is seen from the side, at the edge of the sun, it is instead called a prominence and looks like a bright, reddish arc that extends into space.

You can see this at the bottom left of the sun where a filament disappears over the edge and a prominence becomes visible.

Otherwise, an active sun with areas of sunspots and a chance for solar storms.

Inverted version

The Sun 2026-05-14

Active regions on the Sun are temporary areas of intense, complex magnetic fields, often thousands of times stronger than the Sun's average magnetic field. They appear as dark sunspots in the photosphere and are the primary source of solar flares, coronal loops, and coronal mass ejections (CMEs)

Current Solar Activity (As of May 2026)As of May 14, 2026, multiple numbered active regions have been observed, including AR4436 and AR4438.Recent activity includes a strong M5.79 flare from region 4436 and associated radio blackouts.

Photos taken at Carpe Noctem Observatory.

Active areas at the sun

Active areas on the Sun are regions with extremely strong magnetic fields, up to 1,000 times stronger than the Sun's average magnetic field. It is from these areas that solar storms, solar flares and coronal mass ejections (CMEs) most often emanate.

Sunspots: Dark, cooler areas in the photosphere where the magnetic field is extra concentrated. The number of sunspots follows a cycle of about 11 years. Plagues (bright areas): Bright, hot regions in the chromosphere surrounding sunspots. Solar flares: Sudden and intense energy discharges that send out radiation. Coronal mass ejections (CMEs): Huge clouds of plasma and magnetic fields that are thrown out from the Sun.

The picture shows AR4425 & 4428, taken through my telescope today.

AR4425

AR4425 (also known as 14425) is an active sunspot region currently located on the Earth-facing side of the Sun in late April and early May 2026. Here is the latest status of the region: Magnetic classification: It has recently been downgraded to a beta (β) configuration after losing its more complex "delta" structure, meaning its potential for powerful solar storms has decreased somewhat.

In recent days, AR4425 has been one of the more prominent regions, contributing to several C-class flares as well as occasional M-class (moderate) flares, including an M2.2 on April 26.

The region is currently moving across the northwestern quadrant of the Sun's disk. Although it has shown signs of decreasing complexity, it is still closely monitored by space weather services such as NOAA as it moves toward the edge of the Sun.

Photo taken through my back yard telescope 2026-05-01

Center of our galaxy

The center of our galaxy rises from the ocean late at night off the east coast of Sweden. The center of the Milky Way is the dense core of the galaxy, located about 25,000–28,000 light-years from Earth in the constellation Sagittarius. At its absolute center is the supermassive black hole Sagittarius A* (not visible in these photos, still under the sealine), which weighs about 4 million solar masses. The area is hidden behind thick space dust and is characterized by an extreme density of stars.