The threat from the Sun: should we be worrying about coronal mass ejections?

Scientists have real concerns that extreme weather on the Sun’s surface could unleash a catastrophe on humanity

Telescopic photo of a coronal mass ejection
Telescopic photo of a coronal mass ejection

How is solar weather created?

The surface of the Sun is blisteringly hot, with a temperature of 10,000°F – but the aura of plasma (electrically charged gas) that surrounds it, known as the corona, is far hotter, and in a state of constant turbulence. The corona is so hot that the Sun’s gravitational field can’t hold it, and particles are regularly flung off into space, travelling in every direction through the solar system at millions of miles per hour. This constant flow of particles is called the solar wind. But there are also larger-scale events known as coronal mass ejections (CMEs): huge eruptions caused by magnetic storms on the Sun’s surface, which shoot out billions of tonnes of plasma into space. These vast globs of charged particles regularly hit the Earth.

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