Standard Solar Model
Listen now
Description
Transcript: Knowing the size, composition, and energy source of the Sun, astronomers can calculate the physical conditions at any point within its volume. This is called the standard solar model. Fusion occurs within the core, the inner quarter of the Sun’s radius. The temperature at the very center is fifteen million Kelvin. One quarter of the radius out has dropped to ten million, the edge of the fusion zone, and at half the radius is down to about five million Kelvin. The density at the core is ten to the fifth kilograms per cubic meter. This drops by a factor of two out to the edge of the fusion core and then down to about ten to the three kilograms per cubic meter halfway out the Sun. The fusion core, one quarter of the radius, one sixty-fourth of the volume, contains half the Sun’s mass and generates ninety-nine percent of its energy. Remember that these statements are based on a model of the Sun’s behavior. We cannot see directly into the Sun’s core.
More Episodes
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