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Sagot :
Wavelength observed from Earth = 434nm(λₙ)
Wavelength observed after shift = 510nm(λ₀)
(b) Given, v=HR
R=Distance from Earth to quasar
H=Hubble Constant=22×[tex]10^{-3}m/(s,ly)[/tex]
V=Velocity of quasar
from above V=5.25×[tex]10^{7} m/s[/tex]
∴R=[tex]\frac{V}{H} =\frac{5.25*10^{7} }{22*10^{-3} }=0.24*10^{10} ly[/tex]
R=0.24×[tex]10^{10}ly[/tex], ly=Light year
How did Hubble demonstrate the vast distance between galaxies?
- Hubble's brilliant discovery was that the red shift of galaxies was proportional to their distance from Earth. That meant that objects farther from Earth were moving faster.
- In other words, the universe must be expanding. Hubble discovered Cepheid variable stars in the Andromeda Nebula, a well-known spiral, in 1923.
- Hubble was able to determine the distance of the nebula by using the relationship between the period of the Cepheid fluctuations and its luminosity.
- Surface brightness fluctuations (SBF) and the colour of a galaxy can be used by astronomers to calculate how far away it is from Earth. The majority of galaxies measured in this manner are millions of light years away.
To learn more about Hubble demonstrate the vast distance between galaxies refer to
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