Doppler effect
In the absorption spectrum, we see that blue shift (the spectrum lines appear at bluer side) happens when a star is approaching us. We see a red shift when it’s receding us.
When the observer and source of a wave is moving, the frequency of wave observed changes.
Now tweet the formula a bit: f’/f = (v+uo)/(v+us), for EM wave v = c, c/λ=f, then
λ/λ’ = 1 + Δλ/λ = (c+uo)/(c+us) = 1 + vr/(c+us) ≈ 1 + vr/(c) (since c>>us), therefore we get
Δλ/λ = vr/c
Δλ/λ is called the fractional shift in wavelength. uo-us is the relative velocity between Earth and the star, but being an observer on the Earth (which is not an inertial frame), we may imagine the star being the only moving object. vr turns to be the radial velocity (the component parallel to the line linking star and the Earth) between the star and the Earth. Considering the sign, when the star is approaching us, radial velocity is negative then there’s a negative change in wavelength, causing a blue shift.
Application
1) Expansion of a star (red giants; supernova)
When θ is small, the radius can be given by R=Dθ, ΔR = D(Δθ). ΔR = vt = |Δλ/λ|tc, then
D =ΔR/Δθ = |Δλ|tc/λΔθ. t can be measured in a year [in the same period with Δθ], also note that Δθ in arcsecond should be converted into radian.
Dark matter (as well as dark energy), occupies 95% of matter in the universe, and they do not interact with any known physical phenomena except gravity.
The dark matter leads to the expansion of universe, and a red shift from distant galaxy is observed. The more distant galaxy, the faster recession velocity.
Hubble’s law states that the recession velocity of a galaxy is directly proportional to its distance. Mathematically, v = Hd, where recession velocity is measured in km s-1, d is measured in Mpc and H is the Hubble constant = 73.5 km s-1 Mpc-1.
Note:
1) 73.5 is an approximated value. Up to now this constant are not precisely measured and have a percentage error of 3%.
2) This applies to distant and large enough galaxies only. Otherwise the recession velocity can’t dominant from gravitational pull between galaxies. For example, some small galaxies approach Milky Way Galaxy under gravitational pull.


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