"Redshift (and blue shift) are characterized by the relative difference between the observed and emitted wavelengths of the light from an object. The key here is the emitted wavelength as we can only ever assume this figure, based on our observations and assumptions. In astronomy, redshift is defined by the quality known as z, where z = (observed wavelength - emitted wavelength) / emitted wavelength."<br /><br />There is something very important missing in this paragraph. How does any astronomer know, including Hubble, how much red shifted the light was? What's the standard? There seems to be a key element missing here.<br /><br />There are NO essential assumptions being listed as your post missed the key element in measuring redshift. Thus the post is mistaken on this point.<br /><br />Further, with greater & greater distances, the light fuzzes up and blurs. It's assumed due to interceding dust, gas and such, but not proven to be so. With the existence of dark matter, the whole or part of the redshift might well be found to be a good deal more complicated than once thought.<br /><br />Masses(dark matter) which are at least 6 times greater than visible mass in the universe might have a serious effect upon light moving past such enormous gravity collections, such as dark matter. The fact that normal light is NOT diffused or lensed by such 'dark matter' means very clearly that dark matter is NOT concentrated, it's diffuse, and it doesn't interact very much with light.<br /><br />But the long range gravitational effects would still be there & thus alone could shift light into the red wavelengths, more or less. This means the red shifts might well need to be adjusted.<br /><br />& due to varying concentrations of dark matter, would give some differences in red shifts, as well. These issues are not addressed. Nor is there any necessity that a universe expand linearly, as almost all of the universe is not linear at all. It could pulse, speed up, slow down, or any other o