Description
Transcript: The three basic types of radioactive decay are called alpha, beta, and gamma decay. In the alpha process an atom spontaneously emits a helium nucleus. Helium nucleus contains two protons and two neutrons so alpha decay reduces the atomic number by two. In beta decay a neutron decays into a proton, an electron, and a neutrino. A neutron is only stable when bound in an atomic nucleus. Free neutrons will decay radioactively. The final type of emission is called gamma radiation. Gamma rays are high energy photons released spontaneously by radioactive atoms.
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