The Redshift of Light Emitted by Nearby and Distant Galaxies
However, the ultraviolet surface brightness data of nearby and distant galaxies, over a very wide redshift range imply that the observable Universe is the non-expanding (Euclidean) Universe (NEEU) [1, and references therein]. Moreover, a detailed analysis of the gamma-ray burst sources performed by Sanejouand {2} suggests that this Universe has been Euclidean and static over the last 12 Gy. To explain the redshift, Premović {3} hypothesized that the speed of light emitted by nearby and distant galaxies in NEEU is superluminal.
In
general, we can assume that the measured wavelength, λG, of nearby and distant
galaxies, comprises two parts: the first one, λBB, which results from the Big Bang
Universe (hereinafter BBU) expansion and the second one, λAC, arises from another cause. So, we write that the measured wavelength
λG = λBB + λAC … (1).
There are three possible cases: (a) there is no additional cause λAC = 0 or its contribution to the measured wavelength λG is negligible, then the observable universe is the Big Bang type; (b) a contribution of the BBU expansion λBB to the measured wavelength λG is negligible or equal zero, then the observable universe is NEEU; and, (c) though the BBU expansion contributes predominantly to the measured wavelength λG the wavelength contribution of another cause is not negligible.
Since we cannot separate these wavelength or redshift contributions of nearby and distant galaxies to their corresponding total counterparts (λG and zG), we do not know if the observable Universe: BBU or not.
Hubble’s law states that a distance DG
from Earth to nearby galaxies in BBU or NEEU is linearly related to its
redshift zG {3}. It can be written as
DG = zGc/H0 … (3).
where c (≈ 3×108 m sec-1) is the speed of light and H0 is the Hubble constant. The value is still uncertain and ranges from 50 km sec-1 (Mpc)-1 – 100 km sec-1 (Mpc)-1). This law is valid for nearby galaxies. As we noted previously, once zG becomes ≥ 0.1 and we are dealing with distant galaxies[1], this relationship is no longer linear and becomes dependent on the particular cosmological model.
For example, the galaxy NGC 6264 with zG = 0.03384, the farthest “megamaser” galaxy, is at a distance 447 Mly {3, and references therein}. Using eqn. (3) and the Hubble length c/H0 = 72 km sec-1 we calculate zG = DGH0/c = 447 Mly/13.65 Gly = 0.03275. The difference is 0.03384 – 0.03275 = 0.00109 or the percentage difference is about 3 %.
[1] We will define nearby galaxies as those whose redshift zG is from 0.001 to 0.1 (or 0.001 ≤ zG ≤ 0.1) and distant galaxies with zG > 0.1. Of course, there is no sharp boundary between nearby and distant galaxies.
[2] Of course, λG and zG are related to each other.
[3] Contribution of their peculiar
motion to the redshift is negligible [3].
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