Description
Transcript: We can’t see into the Sun. The Sun is opaque like a frosted pane of glass. Opacity or optical depth is the degree to which a material transmits light. If a material transmits all of the light incident on it, it is transparent, and its opacity or optical depth is zero. If it transmits none of the light it’s opaque, and its opacity or optical depth is high. In the Sun, radiation suffers collisions with atoms or ions that exist there at high temperature and very high density. The frequent collisions make a high opacity which means the radiation cannot travel freely. It’s the difference between having a town square where you walk across it freely because no one else is there and a town square full of a crowd of people where you would have to jostle your way through colliding many times before you could cross the square. In one case the opacity is zero. In the other case the opacity is high. In the Sun the opacity is high enough that we cannot see inside the surface’s few thousandths of a kilometer.
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