Description
Transcript: The Sun oscillates or vibrates at many frequencies like a bell. Solar oscillations can be used to study the interior of the Sun just as geologists use seismic waves to study the Earth’s interior. In fact, apart from neutrinos this is the only way to reliably map out conditions inside the Sun. The best known solar oscillation has a five minute period and corresponds to cells near the surface moving up and down by distances of about ten kilometers. This represents the kind of boiling of the solar surface. It can also be measured by the Doppler Effect in the gas motions and the light emitted by cells near the surface. The Sun has highly complex behavior, and solar seismology is a rich field. Hundreds of modes of oscillation have been observed in the Sun, and recently the principles of seismology have begun to be applied to other stars as well.
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