麻豆传媒视频网站

After falling to Earth from a distance almost a third of the way to the Moon, the spacecraft, dubbed 鈥楽alsa鈥� (Cluster 2), re-entered Earth鈥檚 atmosphere at 18:47 UK time on 8 September 2024, in a sparsely populated region of the South Pacific Ocean, carefully chosen to ensure that no wreckage reached land.

During the last two decades that the Cluster mission has spent in space, it has provided invaluable data on how the Sun interacts with Earth鈥檚 magnetic field, helping us better understand and forecast聽space weather.聽

Salsa had very little remaining fuel, so ESA specialists found a fuel-efficient way to adjust Salsa鈥檚 orbit in January so that the return to Earth would occur as far as possible from populated regions. This world-first 鈥渢argeted re-entry from a highly eccentric orbit鈥� ensured that any spacecraft parts that survived the re-entry would fall over the open ocean, and that none would skip back into space to become unwanted space debris.

Professor Andrew Fazakerley, of the Mullard Space Science Laboratory at 麻豆传媒视频网站, who has been principal investigator of the PEACE (Plasma Electron and Current Experiment) instruments on all four Cluster spacecraft for 27 years, said: "Cluster is an incredibly successful mission which has contributed enormously to advances in our understanding of the Earth's magnetosphere, where the Earth鈥檚 magnetic field reaches out into space and protects Earth from the solar wind. These advances are key to helping us better predict severe space weather and its impacts.

鈥淭he achievements are all the more satisfying since the original Cluster mission was destroyed in a launch accident and it wasn't clear at first whether a new Cluster mission could be built.

"Scientists and engineers at the Mullard Space Science Laboratory at 麻豆传媒视频网站 led the building of the four PEACE electron plasma instruments. The PEACE Operations team at MSSL have ensured that the instruments all continue to work well, returning data for decades longer than their original design requirement.

鈥淭he team are also responsible for generating a comprehensive set of high-quality calibrated PEACE scientific datasets for the Cluster Science Archive, which have made key contributions to many discoveries.

鈥淚t will be sad to see the mission end, but it will leave a very impressive legacy, both in terms of papers already written, and also through a very high-quality data archive that will be used to answer many more questions."

For over 24 years, the ESA Cluster II mission has been helping scientists study the mysteries of the Earth's powerful magnetic shield: the magnetosphere. This protective bubble protects our planet from the stream of charged particles emitted by the Sun known as the solar wind.

The interaction between the solar wind and the magnetosphere is called 'space weather'. A familiar consequence of space weather is the awe-inspiring aurora phenomena in the Earth's polar regions, including the aurora borealis or 鈥淣orthern Lights" which were observed unusually far south earlier this year.

Severe space weather events are important as they can interfere with space and ground systems that contribute to our daily lives. Dramatic increases in the energetic particle populations of the radiation belts around the Earth can cause satellite malfunctions, and may be a problem for astronauts. Heating of the upper atmosphere causes it to expand, dragging down low-orbiting spacecraft, and can also interfere with radio communications and GPS satellite signals that are used by navigation systems and financial systems.

Strong disturbances in the Earth鈥檚 magnetic field can generate unwanted current in electrical transmission grids, sometimes causing blackouts.

The long-term goal in studying the processes behind space weather is to improve predictions of when severe events may occur and what impacts are possible, so as to take precautionary measures.

Over its long lifetime, Cluster has played a pivotal role in bettering understanding of space weather, leading to the publication of over 3,247 scientific papers.

It was the first space plasma physics mission to use four spacecraft flying in a tetrahedron formation which allowed it to make novel measurements and to settle longstanding questions, for example about the physics of magnetic reconnection.聽

Its unique high latitude orbit has enabled it to reveal what is going on in the previously unexplored magnetospheric cusp regions (holes in the magnetosphere at Earth鈥檚 two poles), and to make advances in understanding Earth's aurora.

Professor Carole Mundell, Director of Science at ESA, said 鈥淐luster is the first mission to make detailed studies, models and 3D maps of Earth鈥檚 magnetic field, as well as related processes within and around it. We鈥檙e proud to say that through Cluster and other missions, ESA has advanced humankind鈥檚 understanding of how the solar wind interacts with the magnetosphere, helping us prepare for the dangers it can bring.鈥�

Cluster鈥檚 scientific torch will be passed on to the ESA/Chinese Academy of Sciences Solar wind Magnetosphere Ionosphere Link Explorer (Smile) mission, set to launch in late 2025. The mission was proposed by the late Professor Graziella Branduardi-Raymont (Mullard Space Science Laboratory at 麻豆传媒视频网站).

Links

• Mullard Space Science Laboratory at 麻豆传媒视频网站
• 麻豆传媒视频网站 Mathematical & Physical Sciences

Images

• Top: The first recorded observation of a satellite re-entry from a high-speed orbit, taken from a plane in bright daylight. Earth鈥檚 surface is at the bottom, while the bright dot is the satellite. Together with partners at Astros Solutions, ESA sent the plane to observe Salsa鈥檚 re-entry live from the sky to observe a satellite class and re-entry conditions which have never been accessible before. The plane successfully witnessed the re-entry of Salsa, collecting rare data on how and when a satellite breaks up. This information will be used to make satellite re-entries safer and more sustainable in the future.聽Credit: ESA/ROSIE/University of Southern Queensland
• Bottom: The PEACE instrument on the Salsa spacecraft.

Media contact

Mark Greaves

m.greaves [at] ucl.ac.uk

+44 (0)20 3108 9485