Proba-3 Mission Captures Stunning Views of the Sun's Inner Corona

The Sun’s inner corona, the hottest part of our star's atmosphere, appears faint yellow in this time-lapse made from images taken by the ASPIICS coronagraph aboard Proba-3. The European Space Agency’s Proba-3 mission consists of two spacecraft capable of flying in precisely controlled formation to create artificial solar eclipses in orbit. This animation combines data from Proba-3’s ASPIICS coronagraph (inner solar corona in yellow) and from the Atmospheric Imaging Assembly (AIA) aboard NASA’s Solar Dynamics Observatory (solar disc in dark orange). “The corona is extremely hot, about two hundred times hotter than the Sun's surface,” explains Andrei Zhukov from the Royal Observatory of Belgium, Principal Investigator for ASPIICS. “Sometimes, structures made of relatively cold plasma (charged gas) are observed near the Sun – although these are still around 10 000 degrees, they are much colder than the surrounding million-degree hot corona – creating what we call ‘a prominence’.” Prominences can expand outwards from the Sun and ‘erupt’, breaking up and sending plasma in different directions. This animation resulted from ASPIICS observing the Sun during an active period on 21 September 2025, with one image taken every five minutes, capturing three prominence eruptions in 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,” adds Andrei. The ASPIICS instrument captures the solar corona with several filters, including two different ‘spectral lines’, each line corresponding to a different element contained in the coronal gases. The prominence eruptions seen in this animation were captured in the spectral line emitted by helium atoms, showing the solar atmosphere similarly to how a human eye would see it during a total eclipse through a yellow ASPIICS filter. The AIA image shows the emission in another spectral line produced by helium. The remaining faint yellow glow of the corona is a result of the scattering of visible light from the Sun's surface on coronal electrons.