You seem to be the only poster on this forum who is not Michael Pearson, besides me. So I wolud like to engage you in a discussion.
First of all you sparked my curiosity about stars acting like locomotives or helocopters. Looking up the subject on the internet, I found one essay that exactly addresses the question of doppler versus space expansion. Space expansion? I'd like to pursue that question but it does not seem apprpriate for this forum.
To summarize the essay of Wiess, he first states that whether redshift(?) is due to doppler or space expansion (what's redshift?) depends on the coordinate system. In one it's due to space expansion, and in the other it's due to doppler. So the two are equivalent(???). That does not seem likely unless they are apples and oranges.
From your posts I presume that redshift means frequency change which probably is what redshift means. If so, then doppler characterizes the measurement and space expansion characterizes the primary cause of the doppler.
Finally, at the end of Wiess's essay he says that if the redshift is large, then it is not equivalent to doppler---whatever that means. But it does seem that space expansion is more fundamental than doppler.
Rawson the clerk
Original by Michael Weiss 1994.
What Causes the Hubble Redshift? Are the light waves "stretched" as the universe expands, or is the light doppler-shifted because distant galaxies are moving away from us?
In a word: yes. In two sentences: the Doppler shift explanation is a linear approximation to the "stretched light" explanation. Switching from one viewpoint to the other amounts to a change of coordinate systems in (curved) spacetime.
A detailed explanation requires looking at Friedmann-Robertson-Walker (FRW) models of spacetime. The famous "expanding balloon speckled with galaxies" provides a visual analogy for one of these; like any analogy, it will mislead you if taken too literally, but handled with caution it can furnish some insight.
Draw a latitude/longitude grid on the balloon. These define comoving coordinates. Imagine a couple of speckles ("galaxies") embedded in the rubber surface. The comoving coordinates of the speckles don't change as the balloon expands, but the distance between the speckles steadily increases. In comoving coordinates, we say that the speckles don't move, but "space itself" stretches between them.
A bug starts crawling from one speckle to the other. A second after the first bug leaves, his brother follows him. (Think of the bugs as two light pulses, or successive wave crests in a beam of light.) Clearly the separation between the bugs will increase during their journey. In comoving coordinates, light is "stretched" during its journey.
Now we switch to a different coordinate system, this one valid only in a neighborhood (but one large enough to cover both speckles). Imagine a clear, flexible, non-stretching patch, attached to the balloon at one speckle. The patch clings to the surface of the balloon, which slides beneath it as the balloon inflates. (The bugs crawl along under the patch.) We draw a coordinate grid on the patch. In the patch coordinates, the second speckle recedes from the first speckle. And so in patch coordinates, we can regard the redshift as a Doppler shift.
Is this visually appealing? I think so. However, this explanation glosses over one crucial point: the time coordinate. FRW spacetimes come fully equipped with a specially distinguished time coordinate (called the comoving or cosmological time). For example, a comoving observer could set her clock by the average density of surrounding speckles, or by the temperature of the Cosmic Background Radiation. (From a purely mathematical standpoint, the comoving time coordinate is singled out by a certain symmetry property.)
We have many choices of time coordinate to go with the space coordinates drawn on our patch. Let's use cosmological time. Notice that this is not the choice usually made in Special Relativity: though the two speckles separate rapidly, their cosmological clocks remain synchronized. Bugs embarking on their journey from the "moving" speckle appear to crawl "upstream" against flowing space as they head towards the "home" speckle. The current diminishes as they approach home. (In other words, bug speed is anisotropic in these coordinates.) These differences from the usual SR picture are symptoms of a deeper fact: besides the obvious "spatial" curvature of the balloon's surface, FRW spacetimes have "temporal" curvature as well. Indeed, not all FRW spacetimes exhibit spatial curvature, but (with one exception) all have temporal curvature.
You can work out the magnitude of the redshift using patch coordinates. I leave this as an exercise, with a couple of hints. (1) Since bug speed is anisotropic far from the home speckle, consider also a patch attached to the "moving" speckle. Compute the initial distance between the bugs (the "wavelength") in both patch coordinate systems, using the standard nonrelativistic Doppler formula for a stationary source, moving receiver. (2) Now think about how the bug distance changes as the bugs journey to the home speckle (this time sticking with home patch coordinates). The bug distance does not propagate unchanged. Consider instead the analog of the period of a light wave: the time between bug crossings of a grid line on the patch. This does propagate almost unchanged, provided the rate of balloon expansion stays pretty much the same throughout the bugs' perilous trek. The final result: the magnitude of the redshift, computed using Doppler's formula, agrees to first order with magnitude computed using the "stretched light" explanation. (To the cognoscenti: the assumptions are that Hx