Description
Transcript: Classification is often an important first step towards physical understanding. Imagine you lived in a small town and did a survey where you gathered information on every inhabitant, three pieces of information: their age, their height, and their weight. If you plotted height against weight you would notice an obvious trend, height and weight are correlated. Most people would fall on a particular track in a diagram of height plotted against weight. Some combinations are never seen; you would not have someone who is 3 feet high and 300 pounds nor someone who is 6 feet high and 60 pounds. The pattern will be telling you something. In this case the pattern reveals age because babies obviously grow into children who grow into larger people, and so height and weight are correlated with age. In the case of stars, a similar situation is applied because astronomers did not know the fundamental nature of stars when they first started observing them, and they used stellar classification to get a start.
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