Energy

20,000km/s

speed of the electrons that paint the aurora

The northern lights are caused by particles hitting the air at 7% of the speed of light

The aurora drifts gently across the sky, but the electrons causing it slam into the upper atmosphere at around 20,000 km/s — nearly 7% of the speed of light, about 100 km above your head.

18 May 2026 · 3 min

20,000 km/s — speed of auroral electrons hitting the atmosphere, ~7% of light speed

Wow Moments

20,000 km/sspeed of auroral electrons hitting the atmosphere, ~7% of light speed
44M mphthe same number in imperial, for scale
2–4 dayshow long the solar wind takes to travel from the Sun
100 kmaltitude where most green aurora forms, above your head
1M tonnes/secplasma the Sun sheds as solar wind, continuously

Watch a timelapse of the aurora and it looks calm. Sheets of green light folding and drifting like a slow curtain in a breeze. Gentle. Patient. The opposite of violent.

It is one of the most violent things you can see with the naked eye.

The light you are watching is made by electrons crashing into the upper atmosphere at roughly 20,000 kilometres per second. That is about 7% of the speed of light — around 44 million mph. Each particle covers the distance from Johannesburg to Cape Town in under a tenth of a second. You are watching a particle storm moving so fast that "fast" stops being a useful word for it.

The energy behind them starts on the Sun. The Sun continuously sheds about a million tonnes of charged plasma every second — the solar wind. It streams outward across roughly 150 million km (93 million miles) of empty space, taking two to four days to reach us depending on its speed. Earth's magnetic field catches most of it and funnels it toward the poles.

The solar wind itself is far too slow to light the sky. The speed comes later: inside Earth's magnetosphere — much of it in the long magnetic tail on the night side — electrons are accelerated to around 20,000 km/s. When they finally slam into oxygen and nitrogen atoms about 100 km (60 miles) above the ground, they dump their energy. The atoms absorb it, become briefly "excited", and then release it as a flick of coloured light. Green from oxygen lower down. Red from oxygen higher up. Blue and purple from nitrogen. Every shimmer you see is billions of those tiny energy releases happening at once.

For comparison, here is how aurora speed stacks up against things we normally call fast:

  • Auroral electrons: ~20,000 km/s
  • A coronal mass ejection: up to 3,000 km/s
  • The solar wind (average): ~400 km/s
  • The fastest crewed spacecraft (Apollo 10): ~11 km/s
  • A rifle bullet: ~1 km/s

The aurora is not a gentle light in the sky. It is the visible bruise left where the Sun's particle storm, two to four days in transit, drives electrons into the top of our atmosphere at 7% of the speed of light — and our planet's magnetic field turns the impact into something beautiful instead of something lethal.

Next time the forecast says the lights might be visible, remember you are not watching weather. You are watching the Sun touch the Earth.

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