Doppler Effect for Light — Question 10

Section 37-9 · Physics pages 6210–6211

Question 10 Shortened arrival intervals can produce apparent superluminal transverse motion A moving emitter has speed v = βc and approaches a distant stationary observer at angle α between velocity and the line of sight toward that observer. Across a short interval the direction is effectively constant. Its transverse displacement is v sin α ∆t. observer v α Schematic; labels, not drawing lengths, specify the data. (a) Derive the apparent transverse speed using reception-time separation. (b) For β = 0.80 and cos α = 0.80, find that speed and the received-to-proper pulse-frequency ratio.
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Question 10 - Solution Shortened arrival intervals can produce apparent superluminal transverse motion observer v α (a) Method and calculation ∆tR = ∆t −v cos α ∆t/c = ∆t(1 −β cos α). vapp/c = β sin α 1 −β cos α . (b) Interpretation and further calculation vapp/c = .80(.60) 1 −.80(.80) = 4/3 . fR/f0 = 1 γ(1 −β cos α) = 5/3 . Physical check The apparent speed uses reception times, not simultaneous source positions. The actual emitter speed remains 0.80c.

Question 10

Shortened arrival intervals can produce apparent superluminal transverse motion

A moving emitter has speed v=βcv=\beta c and approaches a distant stationary observer at angle α\alpha between velocity and the line of sight toward that observer. Across a short interval the direction is effectively constant. Its transverse displacement is vsin⁡αΔtv\sin\alpha\,\Delta t.

Diagram shown in the original SVG worksheet.

  1. Derive the apparent transverse speed using reception-time separation.

  2. For β=0.80\beta=0.80 and cos⁡α=0.80\cos\alpha=0.80, find that speed and the received-to-proper pulse-frequency ratio.

Question 10 - Solution

Shortened arrival intervals can produce apparent superluminal transverse motion

Diagram shown in the original SVG worksheet.

(a) Method and calculation

ΔtR=Δt−vcos⁡αΔt/c=Δt(1−βcos⁡α).\Delta t_R=\Delta t-v\cos\alpha\,\Delta t/c=\Delta t(1-\beta\cos\alpha).vapp/c=βsin⁡α1−βcos⁡α.\boxed{v_{\mathrm{app}}/c=\frac{\beta\sin\alpha}{1-\beta\cos\alpha}}.

(b) Interpretation and further calculation

vapp/c=.80(.60)1−.80(.80)=4/3.\boxed{v_{\mathrm{app}}/c=\frac{.80(.60)}{1-.80(.80)}=4/3}.fR/f0=1γ(1−βcos⁡α)=5/3.\boxed{f_R/f_0=\frac1{\gamma(1-\beta\cos\alpha)}=5/3}.

Physical check

The apparent speed uses reception times, not simultaneous source positions. The actual emitter speed remains 0.80c.