Solar Orbiter's widest Sun image

Five years into its mission, Solar Orbiter has captured a stunning new image of the Sun. This detailed view reveals the Sun’s million-degree hot atmosphere, known as the corona, as seen in ultraviolet light.

Solar Orbiter photo of the Sun

The image was created from photos taken by Solar Orbiter’s Extreme Ultraviolet Imager between 13:06 and 17:31 UTC on March 9, 2025, at a wavelength of 17.4 nanometers. At a distance of approximately 77 million km and 11.4° below the equator, the final image measures 12544 x 12544 pixels (6171.6 arc seconds), with the Sun spanning about 7505 pixels. Credit:  ESA & NASA/Solar Orbiter/EUI Team, E. Kraaikamp (ROB)

By ESA/Eyrun Thune
Published Apr. 25, 2025

The Sun appears as a warm yellow sphere with a glowing, chaotic surface. Bright yellow arcs radiate from its equator, while darker regions are noticeable near the south pole. The yellow glow varies in intensity, extending to the edges of the image, where both bright arcs and darker areas are visible.

In this detailed image, you can observe hot plasma—charged particles—interacting within the Sun’s chaotic magnetic field. Look closely to spot the glowing coronal loops surrounding active regions and the darker, cooler filaments and prominences that add to the Sun's intricate tapestry.

The High-Resolution imaging process


Capturing such a detailed image is a remarkable achievement. On March 9, 2025, Solar Orbiter positioned itself 77 million kilometers from the Sun to map the surface using a 5 x 5 grid approach. The Extreme Ultraviolet Imager (EUI) took six high-resolution images and two wide-angle views at each grid point. The final composite image is a stunning assembly of 200 individual photographs, presenting the widest high-resolution view of the Sun to date.

A collaborative effort


Solar Orbiter is the product of an international collaboration between the European Space Agency (ESA) and NASA. The EUI instrument, which played a crucial role in this imaging feat, is led by the Royal Observatory of Belgium.


RoCS's role in the Solar Orbiter mission

The Rosseland Centre for Solar Physics (RoCS) contributes significantly to the Solar Orbiter mission. By developing advanced observational techniques, RoCS enhances the spacecraft's ability to capture high-resolution images of the Sun. Their collaboration with international partners fosters knowledge exchange in solar research, ultimately advancing our understanding of solar phenomena and their impact on space weather.

Tags: Solar Orbiter
Published Apr. 25, 2025 2:17 PM - Last modified Apr. 25, 2025 2:20 PM