Description
Transcript: The energy source of the Sun is the conversion by fusion of hydrogen into helium in a three step process called the proton-proton chain. In the first step protons fuse to form deuterium, a nucleus with a proton and a neutron. The release products are a positron, the antiparticle of the electron, and a neutrino, a tiny nearly massless particle. In the second step of the process deuterium has another proton added to form tritium, two protons and a neutron bound together with the release of gamma rays or radiant energy. In the third step of the process two tritium nuclei combine to form a helium nucleus, two protons and two neutrons, with two free protons left over to participate in fusion products further. At each of the three steps in the process energy is released, and the result of all this energy release is the power from the Sun.
Transcript: Physicists in the nineteenth century made various estimates of the age of the Sun, but they were fundamentally unaware of the most efficient energy source known. Early in the twentieth century physicists Rutherford and Becquerel began a systematic study of the phenomenon of...
Published 07/24/11
Transcript: Chemical energy cannot power the Sun, so what is the energy source? Inspired by an idea by the German physicist Hermann von Helmholtz the English physicist Lord Kelvin explored the idea of gravitational contraction. In this mechanism the Sun is slowly shrinking and gravitational...
Published 07/24/11
Transcript: Above the solar chromosphere is the corona, a diffuse outer layer of gas at the amazing temperature of two million degrees Kelvin. Both the chromosphere and the corona have higher temperatures than the photosphere. How can this be? One way for gas to become hot is pressure. Higher...
Published 07/24/11