Mechanisms behind aurora may be universal in the Solar System

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Observations by Mio/BepiColombo during its first Mercury flyby of electrons precipitating towards Mercury’s surface, in correlation with the anticipated locations of X-ray aurorae reported by the MESSENGER mission. Credit: Sae AIZAWA
Observations by Mio/BepiColombo during its first Mercury flyby of electrons precipitating towards Mercury’s surface, in correlation with the anticipated locations of X-ray aurorae reported by the MESSENGER mission. Credit: Sae AIZAWA

Mercury's magnetic field generates aurorae just like Earth's northern and southern lights, according to international researchers, who say that the mechanisms behind how aurorae are formed may be universal in the Solar System. The team used data from a flyby mission of Mercury and found that the planet's southern magnetosphere aurorae are similar to those seen on Earth and Mars. The magnetosphere is the region around the planet dominated by its magnetic field and is known to experience rapid reconfigurations, which happen following interactions with the solar wind and often result in aurorae similar to those observed around Earth, Jupiter, Saturn, and Uranus.

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From: Springer Nature

Astronomy: Auroral mechanisms may be universal in the Solar System 

The mechanism that generates aurorae in planetary magnetospheres may be universal throughout the Solar System, according to a Nature Communications paper. The study reports data from the BepiColombo mission’s first flyby of Mercury and reveals that Mercury’s southern magnetosphere aurorae are similar to those seen on Earth and Mars.

Mercury’s magnetosphere — the region around the planet dominated by the planet's magnetic field — is known to experience rapid reconfigurations, which happen following magnetic reconnection with solar wind, and processes similar to those observed around Earth, Jupiter, Saturn and Uranus. However, our knowledge about reconfiguration cycles has been limited to spacecraft observations of Mercury’s northern magnetosphere, by the type of particles, and by the energy range detected.

Sae Aizawa and colleagues analysed simultaneous measurements of low-energy electrons (less than 30 kiloelectron volts) and ions during the BepiColombo mission’s first flyby of Mercury in October 2021. They found direct evidence that energetic electrons are accelerated in the near-tail region of Mercury's magnetosphere, drift rapidly toward the dayside, and are subsequently injected onto closed magnetic field lines on the planetary nightside. This process is observed as X-ray aurorae.

The authors suggest that, despite differences in the structure and dynamics of the planetary magnetospheres, electron injections and subsequent energy-dependent drift are a universal mechanism observed throughout our Solar System.

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Funder: S.A., N.A., D.D., J.-A. S., A.B., A.F., E.P., M.P., Q.N., M.R., L.Z.H., D.F., and B.K. acknowledge the support of Centre National d’Etudes Spatiales (CNES, France) to the BepiColombo mission. BepiColombo is a joint space mission between the European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA). MPPE is funded by JAXA, CNES, the Centre National de la Recherche Scientifique (CNRS, France), the Italian Space Agency (ASI), and the Swedish National Space Agency (SNSA). S.A. was funded by the French National Research Agency (ANR) for the TEMPETE (Temporal Evolution of Magnetized Planetary Environments during exTreme Events) project at the time of this work. The part of this work carried by S.A. is supported by JSPS KAKENHI number 22J01606. M.P. is funded by the European Union’s Horizon 2020 program under grant agreement No 871149 for Europlanet 2024 RI. M.F. and N.K. are supported by the German Space Agency DLR under grant 50QW2101.
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