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CME Tracker

Coronal Mass Ejection Monitoring

NASA DONKI-powered CME detection with WSA-ENLIL modeled arrival times and geomagnetic impact forecasts.

Active CMEs (3d)

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Earth-Directed

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Fastest Speed

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Next Arrival

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WSA-ENLIL Solar Wind Model

Heliospheric CME propagation · Live overlay available

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Recent CME events

NASA DONKI · Last 3 days

How long does a CME take to reach Earth?

A coronal mass ejection is a burst of solar plasma and magnetic field hurled from the Sun's corona. Travel time to Earth depends almost entirely on speed: a fast, powerful CME can cross the roughly 150 million km gap in as little as 15 to 18 hours, while a slower, more typical eruption can take 2 to 4 days. Not every CME is Earth-directed — many erupt away from our planet entirely and never arrive at all.

Fast CME
15–18 hours
Speeds above ~2,000 km/s — capable of triggering strong geomagnetic storms
Typical CME
2–3 days
Most Earth-directed CMEs fall in this range
Slow CME
3–5+ days
Weaker eruptions with limited geomagnetic effect

Once a CME's magnetic field connects with Earth's, it can compress the magnetosphere and drive geomagnetic storms — the same activity that fuels bright aurora. That's why the "Next Arrival" estimate above is one of the most useful numbers on this page: it's an early warning for when to start watching the aurora forecast closely.