A neutrino produced by nuclear reactions in the Sun's core.Solar neutrinos are ghostly subatomic particles produced in the nuclear fusion reactions that power the Sun. They stream out of the solar core in enormous numbers, passing through matter almost undisturbed. Because they interact so weakly, they carry information directly from the Sun's heart, offering a unique window into the nuclear processes that keep our star shining.
The solar neutrino problem—a deficit of detected neutrinos compared to theoretical predictions—was first observed in the 1960s by Ray Davis's Homestake experiment. It was resolved in 2001 by the Sudbury Neutrino Observatory, which showed that neutrinos change flavor in transit.
In the Sun's core, protons fuse into helium, releasing neutrinos as byproducts. These neutrinos escape the Sun almost instantly, traveling at near light speed. To catch them, detectors use massive volumes of heavy water, gallium, or liquid scintillator, waiting for the rare moment when a neutrino interacts with an atomic nucleus, producing a detectable flash or a new particle.
Solar neutrino detectors are used to monitor the Sun's nuclear activity in real time and to study neutrino properties, including oscillations and mass differences.
About 100 billion solar neutrinos pass through every square centimeter of your body each second, yet you never feel a thing.


