The Universe Is Expanding — Question 3

Section 44-10 · Physics pages 7476–7477

Question 3 Peculiar velocity biases a nearby Hubble estimate A galaxy has distance 20 Mpc and observed recession velocity 1700 km/s. Its radial peculiar velocity is +300 km/s, where positive means away from the observer. Use the low-redshift additive approximation. vH vpec vobs Schematic; labels, not drawing lengths, specify the data. (a) Find the Hubble-flow velocity and corrected H0. (b) Find the uncorrected estimate and fractional bias.
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Question 3 - Solution Peculiar velocity biases a nearby Hubble estimate vH vpec vobs (a) Method and calculation vobs = H0D + vpec ⇒vH = 1700 −300 = 1400 km/s . H0 = 1400/20 = 70 km s−1 Mpc−1 . (b) Interpretation and further calculation Hnaive = 1700/20 = 85 km s−1 Mpc−1 . (Hnaive −H0)/H0 = 15/70 = .214286 . Physical check At fixed peculiar speed, the fractional bias decreases with distance within the regime where the linear Hubble law applies.

Question 3

Peculiar velocity biases a nearby Hubble estimate

A galaxy has distance 20 Mpc and observed recession velocity 1700 km/s. Its radial peculiar velocity is +300 km/s, where positive means away from the observer. Use the low-redshift additive approximation.

Diagram shown in the original SVG worksheet.

  1. Find the Hubble-flow velocity and corrected H0.

  2. Find the uncorrected estimate and fractional bias.

Question 3 - Solution

Peculiar velocity biases a nearby Hubble estimate

Diagram shown in the original SVG worksheet.

(a) Method and calculation

vobs=H0D+vpec⇒vH=1700−300=1400km/s.v_{\mathrm{obs}}=H_0D+v_{\mathrm{pec}}\Rightarrow\boxed{v_H=1700-300=1400\ {\mathrm{km/s}}}.H0=1400/20=70kms−1Mpc−1.\boxed{H_0=1400/20=70\ {\mathrm{km\,s^{-1}\,Mpc^{-1}}}}.

(b) Interpretation and further calculation

Hnaive=1700/20=85kms−1Mpc−1.\boxed{H_{\mathrm{naive}}=1700/20=85\ {\mathrm{km\,s^{-1}\,Mpc^{-1}}}}.(Hnaive−H0)/H0=15/70=.214286.\boxed{(H_{\mathrm{naive}}-H_0)/H_0=15/70=.214286}.

Physical check

At fixed peculiar speed, the fractional bias decreases with distance within the regime where the linear Hubble law applies.