by alter-ego » Thu Sep 11, 2014 4:27 am
DougStern wrote:So if everything is migrating to the centre of the supercluster, what happens at the super cluster centre eventually?
What is at the "center" is not known. It's not clear that anything different happens if the center is reached. Keep in mind, the Laniakea watershed model displays boundaries as streamlines with cosmic expansion removed. While the animation shows streamline arrowheads all colliding and disappearing, nothing like that is occurring or will occur. Like a globular cluster, stars are orbiting and passing through the center without special events for the most part. On the scale of a supergalactic cluster, the dynamics are probably similar for galaxies (at least the ones that are already in the attractor "valley". Unlike globular clusters, whose spherical size is not affected by cosmic expansion, Laniakea will expand, changing the galactic density and times it takes for a specific member to reach a "center".
I think Laniakea's shape and size will change on the cosmic time scale, galaxies will get further apart on average, and what galaxies do swing through the attractor, things not change much. For static-sized Laniakea 160Mpc, a maximum member velocity ~15000km/sec, the one-way time to reach the center from the edge ~5 billion years, or about 1/3 the age of the universe.
You can see that the convergent streamlines that come to a sudden end in the animations don't correctly give you insight into the galactic dynamics of the cosmic future.
[quote="DougStern"]So if everything is migrating to the centre of the supercluster, what happens at the super cluster centre eventually?[/quote]
What is at the "center" is not known. It's not clear that anything different happens if the center is reached. Keep in mind, the Laniakea watershed model displays boundaries as streamlines with cosmic expansion removed. While the animation shows streamline arrowheads all colliding and disappearing, nothing like that is occurring or will occur. Like a globular cluster, stars are orbiting and passing through the center without special events for the most part. On the scale of a supergalactic cluster, the dynamics are probably similar for galaxies (at least the ones that are already in the attractor "valley". Unlike globular clusters, whose spherical size is not affected by cosmic expansion, Laniakea will expand, changing the galactic density and times it takes for a specific member to reach a "center".
I think Laniakea's shape and size will change on the cosmic time scale, galaxies will get further apart on average, and what galaxies do swing through the attractor, things not change much. For static-sized Laniakea 160Mpc, a maximum member velocity ~15000km/sec, the one-way time to reach the center from the edge ~5 billion years, or about 1/3 the age of the universe.
You can see that the convergent streamlines that come to a sudden end in the animations don't correctly give you insight into the galactic dynamics of the cosmic future.