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9702 · 25.3

Hubble's law and the Big Bang theory — practice questions

Practice and worked examples for 9702 Hubble's law and the Big Bang theory. Short previews only — attempt the full question in MarkScheme against the official scheme.

Worked example 1

A distant galaxy has a recessional velocity of 4900 km s14900 \text{ km s}^{-1}. If Hubble's constant is taken as 70 km s1Mpc170 \text{ km s}^{-1}\text{Mpc}^{-1}, calculate the distance to this galaxy in megaparsecs (Mpc).

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  1. Identify the given values:
    • Recessional velocity, v=4900 km s1v = 4900 \text{ km s}^{-1}
    • Hubble's constant, H0=70 km s1Mpc1H_0 = 70 \text{ km s}^{-1}\text{Mpc}^{-1}
  2. State Hubble's Law:
    • v=H0dv = H_0 d
  3. Rearrange to solve for distance (dd):
    • d=vH0d = \frac{v}{H_0}
  4. Substitute the values and calculate:
    • d=4900 km s170 km s1Mpc1d = \frac{4900 \text{ km s}^{-1}}{70 \text{ km s}^{-1}\text{Mpc}^{-1}}
    • d=70 Mpcd = 70 \text{ Mpc}

Answer: The distance to the galaxy is 70 Mpc70 \text{ Mpc}.

Worked example 2

A spectral line of hydrogen is observed in a distant galaxy's spectrum at a wavelength of 662.8 nm. The same line measured in a laboratory has a wavelength of 656.3 nm. Using a Hubble constant of H0=72 km s1Mpc1H_0 = 72 \text{ km s}^{-1}\text{Mpc}^{-1}, estimate the distance to this galaxy in Mpc. (Speed of light, c=3.00×108 m s1c = 3.00 \times 10^8 \text{ m s}^{-1}).

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  1. Calculate the change in wavelength (Δλ\Delta \lambda):
    • Δλ=λobservedλoriginal\Delta \lambda = \lambda_{observed} - \lambda_{original}
    • Δλ=662.8 nm656.3 nm=6.5 nm\Delta \lambda = 662.8 \text{ nm} - 656.3 \text{ nm} = 6.5 \text{ nm}
  2. Calculate the redshift (Z):
    • Z=ΔλλoriginalZ = \frac{\Delta \lambda}{\lambda_{original}}
    • Z=6.5 nm656.3 nm=0.009904Z = \frac{6.5 \text{ nm}}{656.3 \text{ nm}} = 0.009904
  3. Calculate the recessional velocity (v):
    • For small redshifts, vZcv \approx Zc
    • v=0.009904×(3.00×108 m s1)=2.9712×106 m s1v = 0.009904 \times (3.00 \times 10^8 \text{ m s}^{-1}) = 2.9712 \times 10^6 \text{ m s}^{-1}
  4. Convert velocity to km s⁻¹:
    • v=(2.9712×106 m s1)/1000=2971.2 km s1v = (2.9712 \times 10^6 \text{ m s}^{-1}) / 1000 = 2971.2 \text{ km s}^{-1}
  5. Use Hubble's Law to find the distance (d):
    • d=vH0d = \frac{v}{H_0}
    • d=2971.2 km s172 km s1Mpc1=41.26... Mpcd = \frac{2971.2 \text{ km s}^{-1}}{72 \text{ km s}^{-1}\text{Mpc}^{-1}} = 41.26... \text{ Mpc}

Answer: The distance to the galaxy is approximately 41 Mpc41 \text{ Mpc} (to 2 s.f.).