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clock-iconPUBLISHEDJanuary 23, 2026
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Watch As ESA's Artificial Eclipse Maker Catches 3 Solar Prominences Erupting One After Another

The incredible observations are possible thanks to the formation flying of Proba-3.

Dr. Alfredo Carpineti headshot

Dr. Alfredo Carpineti

Alfredo has a PhD in Astrophysics and a Master's in Quantum Fields and Fundamental Forces from Imperial College London.

Space & Physics Editor

Alfredo has a PhD in Astrophysics and a Master's in Quantum Fields and Fundamental Forces from Imperial College London.View full profile

Alfredo has a PhD in Astrophysics and a Master's in Quantum Fields and Fundamental Forces from Imperial College London.

View full profile
EditedbyHolly Large
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Holly Large

Copy Editor & Staff Writer

Holly has a degree in Medical Biochemistry from the University of Leicester. Her scientific interests include genomics, personalized medicine, and bioethics.

Against a dark background, the Sun’s disc is shown in dark orange, as captured by NASA’s Solar Dynamics Observatory. A thin halo of yellow light surrounds the Sun, giving it a luminous outline against the dark background of space. This yellow outline shows the Sun’s inner corona, as captured by Proba-3. Also in yellow a large proinence has just emerged from the solar disc.

One of the prominences caught in the act.

Image credit: ESA/Proba-3/ASPIICS, NASA/SDO/AIA


The European Space Agency’s Proba-3 is a marvel of engineering. Two spacecraft fly in formation to observe the Sun. Well, not exactly the Sun, but its atmosphere: the corona. The two spacecraft get into an alignment so that the one that is Sun-side blocks the solar disk as it happens during a solar eclipse, while the one behind instead looks at the emission of the corona.

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In observations collected on September 21, 2025, the spacecraft snapped not one but multiple eruptions in the solar corona. Matching Proba-3 observations with NASA’s Atmospheric Imaging Assembly (AIA) aboard NASA’s Solar Dynamics Observatory, we can now see the process as a whole.

This is a gif animation made up of false-colour images taken by ESA’s Proba-3 mission and NASA’s Solar Dynamics Observatory. Against a dark background, the Sun’s disc is shown in dark orange, as captured by NASA’s Solar Dynamics Observatory. A thin halo of yellow light surrounds the Sun, giving it a luminous outline against the dark background of space. This yellow outline shows the Sun’s inner corona, as captured by Proba-3. Also in yellow, three solar prominence eruptions are visible, resembling bright yellow wave-like outburst extending outwards from the Sun. First, we can see a smaller one in the top right corner, followed by a larger one in the top left and a third one in the bottom right. The whole animation lasts about 4 seconds and plays in a loop
Five hours of Proba-3 and SDO sped up to a few seconds show a lot of activity.
Image credit: ESA/Proba-3/ASPIICS, NASA/SDO/AIA

“The corona is extremely hot, about two hundred times hotter than the Sun's surface,” Andrei Zhukov from the Royal Observatory of Belgium, Principal Investigator for the ASPIICS coronagraph aboard Proba-3, said in a statement.

“Sometimes, structures made of relatively cold plasma (charged gas) are observed near the Sun – although these are still around 10 000 degrees Celsius, they are much colder than the surrounding million-degree hot corona – creating what we call ‘a prominence’.”

Due to the formation flying, Proba-3 is not always under “eclipse” mode. The observations window this time was five hours, with images collected every five minutes. Still, it was a surprisingly exciting five hours.

“Seeing so many prominence eruptions in such a short timeframe is rare, so I’m very happy we managed to capture them so clearly during our observation window,” added Zhukov.

Proba-3 will observe the Sun during the total solar eclipse happening between Iceland and Spain this coming summer, and the results will be compared. A natural eclipse can get a lot more detail, but clearly, Proba-3 is doing some pretty good work.


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