Description
Transcript: The Sun is the source of all the Earth’s energy, and life could not exist without the Sun. In addition, there’s growing evidence that long term variations in the Sun’s output profoundly affect the Earth’s climate. For example, in the period from 1645 to 1715 sunspots were at a generic minimum called the Maunder Minimum. And in Europe an ice age was experienced with cold temperatures, and this is confirmed by tree rings from the time. From 1540 to the present day there have been many droughts in Africa. Statistical analysis shows that they correlate very well with sunspot minima. Thus, on a period of the solar cycle there’s evidence that the Sun affects the Earth’s climate. In addition, there is less secure evidence that variation in the Sun’s output affects the Earth’s climate on a timescale of hundreds or thousands of years. Earth, for example, experiences mini ice ages every several thousand years. This evidence is less good because evidence of the Sun’s output is indirect over those timescales, as is evidence of the Earth’s temperature.
Transcript: Since light has a finite speed, three hundred thousand kilometers per second, there’s an inevitable consequence called light travel time. In terrestrial environments light essentially travels instantly or appears to travel fast. The finite speed of light, three hundred thousand...
Published 07/24/11
Transcript: Some stars in the sky, somewhat hotter than the Sun with temperatures of 5 thousand to 10 thousand Kelvin, have very low luminosities in the range of one-hundredth to one-thousandth the Sun’s luminosity. Application of the Stephan-Boltzmann Law shows that they must be physically...
Published 07/24/11
Transcript: Certain rare stars in the sky with either red or blue colors are extremely luminous, up to a million times the luminosity of the Sun. Application of the Stephan-Boltzmann Law shows that their sizes must be in the range of ten to a thousand times the size of the Sun. These...
Published 07/24/11