BepiColombo captures images of Mercury’s shadowed craters and volcanic lands

These images illustrate the pockmarked surface of Mercury and are a preview of what to expect as the BepiColombo mission enters orbit around the innermost region of our solar system in late 2026.

Since its launch in 2018, the joint Japan-Europe spacecraft BepiColombo has made six flybys of Mercury, gradually decelerating with each pass to fine-tune its trajectory for orbital insertion. While the mission’s primary scientific instruments are yet to be utilized, the spacecraft’s cameras have already provided detailed images of the planet.

The European Space Agency (ESA) recently released three striking images captured during BepiColombo’s latest flyby on January 8, taken from an altitude of around 300 kilometers above Mercury’s north pole and northern regions.

David Rothery, from the Open University, UK, shared his excitement about the images, saying, “We had to wake up early to see these close-ups, and they exceeded our expectations based on simulated views we studied beforehand.”

The image above showcasing Mercury’s north pole reveals the sharp contrast between light and darkness on the planet, known as the terminator line. This region shows extreme temperature variations, with some areas exposed to scorching sunlight while others remain perpetually shaded within craters.

Notably, shadowed regions containing potential frozen water deposits can be observed along the terminator line in the image. Rothery further highlights the fascinating details visible, such as the sunlit peak inside Tolkien Crater, providing key insights for the mission’s scientific objectives.

Scientific investigations suggest that these shadowed crater areas may harbor frozen water, a key aspect of BepiColombo’s mission to uncover the presence and extent of water on Mercury.

Mesmerizing images from BepiColombo’s mission highlight Mercury’s expansive volcanic plain known as Borealis Planitia, formed over 3 billion years ago from massive lava flows that engulfed existing craters, some of which are visible in the image. While most of these plains are relatively smooth, more recent impact craters provide intriguing targets for scientific study.

Spanning 1,500 kilometers, the Caloris Basin is the largest crater on Mercury, appearing as a semicircular light-colored feature on the planet’s surface. Once BepiColombo enters orbit, researchers aim to investigate the relationships between the Caloris Basin, Borealis Planitia, and the solidified lava flows connecting them.

The illuminated region at the top of the planet, known as Natal Facula, is believed to be the aftermath of Mercury’s most significant volcanic eruption. The presence of a central crater, approximately 40 kilometers wide, indicates multiple eruptions that scattered volcanic material over hundreds of kilometers.

Rothery expresses eagerness for future observations of Natal Facula by BepiColombo’s instruments, emphasizing its scientific importance in understanding Mercury’s volcanic history. Discovering the reasons behind Mercury’s enduring volcanic activity remains a key goal of the mission.