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Math & science since 1843

The Sun has an eleven-year heartbeat

Two images of the Sun side by side: on the left, labelled Solar minimum, a clean orange disc; on the right, labelled Solar maximum, the same disc dotted with dark sunspots
The Sun at solar minimum (December 2019) and at solar maximum (August 2024), seen by NASA’s Solar Dynamics Observatory. Image: NASA/SDO, public domain, via Wikimedia Commons

Count the dark spots on the face of the Sun over the years and they rise and fall: many, then few, then many again. One full round takes about eleven years, and astronomers call it the solar cycle.

It was found by Heinrich Schwabe, a pharmacist from Dessau in Germany, who won his first telescope in a lottery in 1825. He was hunting for Vulcan, a planet that some believed hid inside the orbit of Mercury, and hoped to catch it crossing the face of the Sun. For 17 years, on every clear day, he recorded the Sun’s spots. No planet turned up, but in 1843 he noticed that the spots came and went in a rhythm. He put it at about ten years; longer records have since settled on about eleven.

Near the peak of each cycle the Sun’s magnetic field flips, north becoming south, so the Sun needs two cycles, about 22 years, to get back to where it started.

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