attofishpi wrote: ↑Wed Aug 31, 2022 12:58 pm
Astro Cat wrote: ↑Wed Aug 31, 2022 10:14 am
For instance here you can see a lot of galaxies that deviate a lot from the Hubble Flow because they're in the Virgo Cluster (the blue oval). There's a lot of gravity there so a lot of "true" motion going on: some towards us, some away.
Hi Astro thanks for the above, but not sure if I made my question rather ambiguous, or I still just don't comprehend.
Let me put it another way.
Let's say there are two identical stars (I know this scenario is totally unlikely), one is 1000 light years from us, and is stationary in relation to us. The other is 1,000,000 light years from us, and is also stationary in relation to us.
Does the wavelength that arrives to us remain identical from both stars? Or does the wavelength of the star that is futher away have a greater wavelength (more "red" shifted)?
The one from the star that's further away is more redshifted, but it is technically
not the Doppler effect: it is a consequence of the peaks and troughs being further and further apart as the space between them expands (and we see radiation with increasing distance between peaks as a redshift).
So, to try to digest your question in the different ways I can think you might be curious about:
1) If you mean that these two test objects are
literally stationary in relation to us (some alien civilization thinks our world is special, and they hold these two stars stationary in relation to us against the expansion of the universe), then with a completely clear path (dust will attenuate light to look like redshift, too) there would not be any redshift from either object.
2) If you mean that these two test objects simply aren't orbiting anything (have no peculiar/true motion) but they do "move" as the universe expands, like two points on an expanding balloon (they're not "moving," but the space around them sweeps them along for the ride), then yes there would be redshift, and the further one would be redshifted more.
So, you originally mentioned someone saying something like that most galaxies aren't moving (I don't remember how you phrased it exactly). What I suspect is probably a case of misinterpretation: there is a distance away from an observer where peculiar motion (think of this like "true" motion: the dots on the balloon are actually moving on the balloon) is completely negligible because the expansion overpowers it.
The closer objects are, the more their peculiar motion matters: Andromeda is blueshifted from our perspective because of its peculiar motion (straight towards us) for instance. Or consider all of those galaxies all over the place on the plot I posted in the Virgo Cluster: they're near enough to us as observers that their peculiar motion matters a lot.
But peculiar motion has an upper speed limit (and we will see that speed limit in galactic clusters, where gravity is the craziest). The expansion (the Hubble flow), however, gets stronger and stronger the further away something is. Since peculiar motion caps out at a few thousand km/s, there is a distance at which peculiar motion becomes completely negligible and all that matters is the Hubble flow.
This is probably what the article you were mentioning is talking about. It's not that galaxies out there aren't moving: they're moving in all sorts of directions, even towards us. It's that the expansion so vastly outstrips their peculiar motion that it's utterly negligible.