Tag Archives: BepiColombo

BepiColombo Mission Launches in 2026: Unveiling the Secrets of Mercury

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Artist’s Impression of BepiColombo Spacecraft Near Mercury

Source: ESA/ATG Media Lab

In 2026, the highly anticipated BepiColombo spacecraft is set to orbit Mercury, promising to unlock the planet’s long-standing mysteries.

BepiColombo is a collaborative mission involving the European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA). This intricate mission includes the Mercury Planetary Orbiter (MPO) and the Mercury Magnetospheric Orbiter (Mio), tethered to the Mercury Transport Module (MTM).

Since its launch in 2018, the MTM has made six flybys of Mercury, skillfully utilizing the planet’s gravity to facilitate its descent into orbit, a method pioneered by Giuseppe “Bepi” Colombo.

This mission has already gathered crucial scientific insights, including data about the solar wind and high-resolution imagery of Mercury’s surface. However, the MPO’s advanced instruments, including X-ray spectrometers, remain inactive due to obstructions by the MTM.

In September 2026, the MPO and Mio will detach from the MTM, embarking on their final descent into orbit, completing this phase by November when their focus will shift to detailed studies of Mercury.

According to Charlie Feldman, a researcher at the University of Leicester who contributed to the MPO’s instruments, “We’re hopeful that our equipment will function as intended. With the extensive time invested in building it, the excitement comes with a degree of anxiety.”

Alongside capturing intricate details of Mercury’s magnetosphere, the MPO will extensively map and analyze the planet’s surface using its spectrometer and other tools. “This represents the first X-ray imagery of an extraterrestrial surface,” Feldman noted.

Such observations may unravel enigmas surrounding the significant X-ray emissions detected from Mercury’s night side in prior missions. Additionally, the spacecraft will assess X-rays emitted from the sun-facing side, unearthing new insights into Mercury’s geological composition and evolution. “Deciphering how planets formed gives us a broader understanding of solar system dynamics,” Feldman stated.

Exploring Space and Astronomy in Japan: The Land of the Rising Sun

Experience Japan’s unique blend of astronomy and culture, featuring cutting-edge research institutes and breathtaking starry skies. Explore prestigious locations like JAXA Tsukuba Space Center, the Nobeyama Radio Observatory, and the Tanegashima Space Center, while marveling at the celestial beauty above the Japanese Alps and Yakushima.

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Source: www.newscientist.com

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

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The bright and dark part of Mercury's north pole seen from the BepiColombo spacecraft

ESA/BepiColombo/MTM

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.

Mercury's vast volcanic plain known as Borealis Planum

ESA/BepiColombo/MTM

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.

Natal Facula, believed to be the remains of the largest volcanic eruption in Mercury's history, is seen as a bright spot in this image.

ESA/BepiColombo/MTM

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.

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Source: www.newscientist.com

Oxygen and carbon ions detected in Venus’s magnetosphere by BepiColombo

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In August 2021, ESA/JAXA BepiColombo spacecraft bound for Mercury Performed a second flyby of Venus, providing short-term observations of its guided magnetosphere. The spacecraft detected cold oxygen and carbon ions at a distance of about six planet radii, in an area of ​​the magnetosphere that has never been explored before.

Schematic illustration of planetary material escaping through the sides of Venus's magnetic sheath. The red line and arrow indicate the observation region and direction of BepiColombo as the ions escape (C+,oh+,H+) was observed. Image credit: Thibaut Roger / Europlanet 2024 RI / Hadid other.

Venus was similar to Earth in many ways during its formation, including the presence of large amounts of liquid water.

However, Venus eventually underwent a divergent evolution, leading to major differences between the two planets.

Unlike Earth, Venus is currently a very dry planet with no inherent magnetic field.

The continuous influence of the solar wind on the atmospheres of both planets results in significant atmospheric losses.

Venus' atmosphere is primarily composed of carbon dioxide and small amounts of nitrogen and other trace species, and is affected by interactions with the solar wind, leading to significant ion fluxes.

“This is the first time that positively charged carbon ions have been observed to be ejected from Venus's atmosphere,” said Dr. Lina Hadid, a researcher at the Plasma Physics Institute and CNRS.

“These are heavy ions that typically move slowly, so we're still trying to understand the mechanism.”

“An electrostatic 'wind' may be moving them away from Earth, or they may be accelerated by centrifugal action.”

“Unlike Earth, Venus does not generate an intrinsic magnetic field at its core.”

“Nevertheless, interactions between charged particles emitted by the sun (solar wind) and charged particles in Venus' upper atmosphere create a weak, comet-shaped 'induced magnetosphere' around the planet. ”

“Around the magnetosphere there is a region called the 'magnetic sheath' where the solar wind is slowed down and heated.”

On August 10, 2021, BepiColombo passed Venus to slow down and adjust its course towards its final destination, Mercury.

The probe soared up the long tail of the planet's magnetic sheath, emerging from the nose of the magnetic region closest to the sun.

Over a 90-minute observation period, BepiColombo's mass spectrometer (MSA) and mercury ion analyzer (MIA) will measure the number and mass of charged particles encountered, and detect chemical and Captured information about physical processes. magneto sheath.

“Characterizing the loss of heavy ions on Venus and understanding the escape mechanisms will help us understand how Venus's atmosphere evolved,” said Dr. Dominique Delcourt, principal investigator at MSA and researcher at the Plasma Physics Institute. “This is critical to understanding how water is lost.” .

“This result shows a unique result from measurements made during a flyby of a planet, in which the spacecraft may pass through areas that are generally inaccessible to orbiting spacecraft. '' said Dr. Nicolas Andre, a researcher at the Astrophysical and Planetary Institute.

of study It was published in the magazine natural astronomy.

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LZ Hadid other. BepiColombo's observations of cold oxygen and carbon ions on the side of Venus' induced magnetosphere. Nat Astron, published online on April 12, 2024. doi: 10.1038/s41550-024-02247-2

Source: www.sci.news