To calculate the measured wavelength of the Lβ line for hydrogen considering the redshift, we can use the relativistic Doppler effect formula:
λ_observed = λ_rest * sqrt((1 + v/c) / (1 - v/c))
Where:
λ_observed is the observed wavelength
λ_rest is the rest wavelength
v is the velocity of the starlike object
c is the speed of light in vacuum
The rest wavelength of the Lβ line for hydrogen is approximately 102.57 nm.
Now let's calculate the observed wavelength:
v = 75000 km/s = 75000 * 1000 m/s = 7.5 * 10^7 m/s
c = 3 * 10^8 m/s
λ_observed = 102.57 nm * sqrt((1 + 7.5 * 10^7 / (3 * 10^8)) / (1 - 7.5 * 10^7 / (3 * 10^8)))
Calculating the above expression, we find:
λ_observed ≈ 102.57 nm * sqrt(1.4083333)
λ_observed ≈ 102.57 nm * 1.1865502
λ_observed ≈ 121.77 nm
Therefore, the measured wavelength of the Lβ line for hydrogen, considering the redshift, is approximately 121.77 nm.