by rstevenson » Sun Oct 28, 2012 2:42 pm
Hi Ernie. I hope you don't mind me butting in here.
Your geometrical construction works as you described it, but it does not properly represent the expansion of space. Try this instead...
Draw a circle in the sky, encompassing a portion of your view of the universe at that point in time. Pick two points on the circle, p1 and p2, being the locations of a couple of galaxies perhaps. Draw radii to them from the origin 0, which is where you are in the universe. Now wait several billion years while space expands.
Draw a second circle, centered on the origin (you're at the centre of your observable universe so you haven't moved) and touching the same two galaxies. It may have faded over time, so you may need to redraw the first circle at its original radius just as a reminder of how big it was. Extend the radii that you drew before to p1 and p2 until they intersect the second circle at p3 and p4. You'll find that p3 and p4 are where the galaxies are now. Or do it the other way 'round. Find your two galaxies and draw radii from them to the origin. You'll find each new radius lies along the old radius exactly.
Note 1: real galaxies may well have some proper motion which would cause them to appear slightly offset from our idealized situation. For example, the Milky Way and Andromeda are gradually getting closer to each other. But that proper motion has nothing to do with the expansion of space.
Note 2: this is, of course, vastly simplified. As Chris has pointed out we can only see "now" and must infer the rest. But geometrically speaking the above analogy is reasonable.
Rob
Hi Ernie. I hope you don't mind me butting in here.
Your geometrical construction works as you described it, but it does not properly represent the expansion of space. Try this instead...
Draw a circle in the sky, encompassing a portion of your view of the universe at that point in time. Pick two points on the circle, p1 and p2, being the locations of a couple of galaxies perhaps. Draw radii to them from the origin 0, which is where you are in the universe. Now wait several billion years while space expands.
Draw a second circle, centered on the origin (you're at the centre of your observable universe so you haven't moved) and touching the same two galaxies. It may have faded over time, so you may need to redraw the first circle at its original radius just as a reminder of how big it was. Extend the radii that you drew before to p1 and p2 until they intersect the second circle at p3 and p4. You'll find that p3 and p4 are where the galaxies are now. Or do it the other way 'round. Find your two galaxies and draw radii from them to the origin. You'll find each new radius lies along the old radius exactly.
Note 1: real galaxies may well have some proper motion which would cause them to appear slightly offset from our idealized situation. For example, the Milky Way and Andromeda are gradually getting closer to each other. But that proper motion has nothing to do with the expansion of space.
Note 2: this is, of course, vastly simplified. As Chris has pointed out we can only see "now" and must infer the rest. But geometrically speaking the above analogy is reasonable.
Rob