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When a Solar Superstorm Rocked Mars: Eyewitness Accounts from Orbit

ESA's Orbiters Caught a Monster Solar Storm Stripping Mars's Atmosphere

Discover how a massive solar superstorm in 2017 offered an unprecedented look at Mars's atmospheric loss and radiation hazards, thanks to simultaneous observations from ESA's Mars Express and ExoMars TGO.

Imagine a colossal solar superstorm, far more powerful than anything we usually experience on Earth, hurtling through space and slamming right into a planet. That's exactly what happened to Mars in September 2017, and thankfully, two of Europe's watchful eyes in orbit were perfectly positioned to witness the whole dramatic spectacle unfold. It was a truly unique opportunity to study the Red Planet under extreme conditions.

This wasn't just any solar flare; we're talking about a massive coronal mass ejection (CME) that erupted from the Sun, sending a torrent of energetic particles and magnetic fields racing towards Mars. For scientists, it was like a cosmic gift, providing an unparalleled chance to see how such powerful space weather truly impacts a planet with a tenuous atmosphere and no global magnetic field to speak of. We got to see, in real-time, the Red Planet getting pummeled.

Hovering above, ESA's venerable Mars Express, which has been orbiting since 2003, and the then-relatively new ExoMars Trace Gas Orbiter (TGO), launched in 2016, both sprang into action. They offered a combined, simultaneous vantage point that had never been possible before. Mars Express, with its SPICAM instrument, picked up on a huge spike in ozone levels, a clear indicator of significant atmospheric shifts. Even more dramatically, its ASPERA-3 instrument was practically watching Mars's upper atmosphere being stripped away, as it measured an intense outflow of particles escaping into space. It was a live demonstration of how Mars likely lost much of its once-thicker atmosphere over billions of years.

Meanwhile, the TGO, still getting acquainted with its new home, provided crucial insights into the radiation environment. Its FREND (Fine Resolution Epithermal Neutron Detector) instrument registered a significant surge in radiation at the Martian surface and just below it. This data is absolutely vital for understanding the very real dangers future human explorers will face when they eventually venture to Mars. Think about it – a sudden blast like that could be catastrophic for unprotected astronauts.

And if all that wasn't enough, both orbiters also detected something truly beautiful and awe-inspiring: auroras! Yes, despite Mars lacking a global magnetic field like Earth's, these brilliant light shows appeared. They occur when the solar wind interacts with localized, remnant crustal magnetic fields, primarily in the southern hemisphere. Imagine seeing those shimmering lights from the Martian surface – a stark reminder of the dynamic, sometimes violent, interaction between a planet and its star.

The coordinated observations from Mars Express and TGO have given us an incredible treasure trove of data. They're helping scientists piece together the puzzle of Mars's atmospheric evolution, understand the processes of planetary atmospheric loss, and critically, assess the hazards posed by space weather for any future crewed missions. It’s a vivid lesson in just how vulnerable planets can be to the Sun's tempestuous nature, and a testament to the incredible scientific instruments we send out to watch these cosmic dramas unfold.

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