Description
Transcript: A parsec is a distance unit appropriate to the study of stars. It’s the distance that produces a parallax shift of one arcsecond. In other words, it’s the distance where the angle subtended by the star as seen from the Earth’s orbit six months apart, spanning the orbit, is one second of arc. One parsec equals 3.26 lightyears, so a parsec is slightly larger than a lightyear. Astronomers also use multiples of the parsec, a thousand parsecs, which is a kiloparsec, and a million parsecs, which is a megaparsec. The most useful thing about the parsec unit is that it corresponds to the typical distances between stars in the Milky Way Galaxy.
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