Description
Transcript: The visible surface and edge of the Sun and the region where sunspots lie is the Sun’s photosphere. Just above the photosphere lies the chromosphere or color layer. This is a slender region of pink gas at a temperature of about ten thousand degrees Kelvin. The pink color comes from emission from hydrogen alpha, the single spectral transition of an excited hydrogen that comes out in the red part of the visible spectrum. The solar chromosphere is best seen during a total eclipse when the moon blocks out the Sun’s light, and the delicate radiation of the chromosphere and its color can clearly be seen. Beyond the chromosphere the Sun fades out into deep space.
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