A series of nuclear reactions is what powers the stars. These reactions produce neutrinos, which are tiny particles with no electrical charge. The existence of neutrinos was predicted in 1930 by early quantum physicist Wolfgang Pauli, in an attempt to explain how beta decay seemed to violate the laws of conservation of energy. But it wasn't until 1942 when a neutrino was actually observed and subsequently described by the physicist who co-discovered them, Frederick Reines, as "the most tiny quantity of reality ever imagined by a human being." Because they are so fast, neutrinos help us study the sun in "real-time," because the light we experience now was produced by the sun thousands of years ago.
Neutrinos Are Insanely Small, Fast, And Everywhere
Neutrinos: Nature's Ghosts?
Key Facts In This Video
If you wanted to stop one neutrino, you would need about four light years of lead. 00:09
The neutrinos made in the sun are detected much quicker than other energy from the sun because very little gets in the way of them. 02:56
We can study how the sun has changed over time by comparing neutrinos (which have left the sun more recently) to other energy (which took many more years to escape the sun). 08:06
Wake up with the smartest email in your inbox.
Our Best Articles Daily