Changes

::::::::::::::And that's 31.7 billion light years comoving distance, 13.2 billion light years in light travel distance. Meaning, we see it as it was, billions of years ago, and it is WAY farther away by now. [[User:RachelW|RachelW]] 21:25, 30 January 2012 (EST)

::::::::::::::And that's 31.7 billion light years comoving distance, 13.2 billion light years in light travel distance. Meaning, we see it as it was, billions of years ago, and it is WAY farther away by now. [[User:RachelW|RachelW]] 21:25, 30 January 2012 (EST)

Aschlafly has "numerous references" to stars 39 billion light years away. I have an open mind about this, and I trust that as an educator he will want to share them. [[User:ScottDG|ScottDG]] [[User talk:ScottDG|Talk]] <b>2 billion lightyears ago...wait, what?  </b> 21:28, 30 January 2012 (EST)

Aschlafly has "numerous references" to stars 39 billion light years away. I have an open mind about this, and I trust that as an educator he will want to share them. [[User:ScottDG|ScottDG]] [[User talk:ScottDG|Talk]] <b>2 billion lightyears ago...wait, what?  </b> 21:28, 30 January 2012 (EST)

Rob, I posted on your talk page that the rate of expansion is very small, considering the distances involved. Two objects that are  relatively strongly bound gravitationally don't experience the expansion because gravity resists the very small force driving them apart. However, between two objects far enough away for gravity to be very weak, the expansion is more noticeable. [[User:RachelW|RachelW]] 22:06, 30 January 2012 (EST)

:Rob, I posted on your talk page that the rate of expansion is very small, considering the distances involved. Two objects that are  relatively strongly bound gravitationally don't experience the expansion because gravity resists the very small force driving them apart. However, between two objects far enough away for gravity to be very weak, the expansion is more noticeable. [[User:RachelW|RachelW]] 22:06, 30 January 2012 (EST)