H
heyo
Guest
An interesting article in the new SciAm about the expansion of the universe, and it clued me in to some things that I thought I understood but was off on.<br /><br />One thing is, I thought that the redshift of distant galaxies was due to an effect similar to the doppler shift of sound here on Earth, and that is the analogy that is commonly used.<br /><br />Not so however, because the galaxy's local motion relative to it's local spacetime is relatively low compared to the speed of the expansion of the universe. Most of the redshift is actually caused by space strrrreeetching out while the light waves are en-route over all those billions of years, thereby making them longer.<br /><br />Draw a picture of a light wave on a rubber band, then stretch the rubber band. I think that's a good analogy.<br /><br />Also, we know that astronomers can look about about 14 billion light years or so, and are therefore looking back about 14 billion years, but what the article said (which makes sense) is that we see those galaxies where they were at that time, and that the actual current radius of the observable universe is about 46 billion light years, extrapolating out to where those galaxies would be today.<br /><br />Also, we know that objects can't move at speeds greater than C, but the expansion can proceed at />C. But, I did not know that galaxies with a redshift of only 1.5 (which IIRC means the light is stretched to 2.5 times it's original wavelength) are already receding from us at >C.<br /><br />It is a neat article. I reccomend checking it out.<br /><br />Heyo