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Volume 587 Issue 7835, 26 November 2020

Catching the rays

The Sun generates the vast majority of its energy from the fusion of hydrogen to form helium in a process called the proton–proton chain. But a small amount of its energy was thought to come from a secondary fusion process catalysed by carbon, nitrogen and oxygen, known as the CNO cycle. In this week’s issue, the Borexino Collaboration presents results that offer the first direct experimental evidence for the CNO cycle occurring in the Sun. The researchers used the Borexino detector (pictured on the cover) at the INFN Gran Sasso National Laboratories near L’Aquila, Italy, to detect neutrinos emitted as a result of the cycle. The results allowed the team to confirm that the CNO cycle contributes to about 1% of the Sun’s energy, and could offer fresh ways to probe the elemental composition of the Sun’s core.

Cover image: Borexino Collaboration.

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