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Relativistic Doppler effect

What you are seeing: the observed frequency ratio fobs/fsrc=1/(γ(1βcosθ))f_\text{obs}/f_\text{src} = 1 / (\gamma (1 - \beta \cos\theta)) as a function of viewing angle θ\theta at fixed source speed β=v/c\beta = v/c. The polar plot shows the same factor on radial axes: head-on approach (θ=0\theta = 0) gives the maximum blueshift, recession (θ=π\theta = \pi) gives the maximum redshift, and at θ=π/2\theta = \pi/2 there is a pure transverse redshift by 1/γ1/\gamma (no Newtonian analog).

Slide the speed to see the curve sharpen as β1\beta \to 1: the blueshift cone narrows toward forward beaming. The dashed red horizontal at fobs/fsrc=1f_\text{obs}/f_\text{src} = 1 marks where blueshift flips to redshift; it crosses zero at cosθ=(11/γ)/β\cos\theta = (1 - 1/\gamma) / \beta.

Figure 1. Relativistic Doppler fobs/fsrc=1/(γ(1βcosθ))f_\text{obs}/f_\text{src} = 1/(\gamma(1-\beta\cos\theta)) vs angle. Method: closed-form.
beta (v/c)0.500
theta (deg)60

WHAT TO TRY

  • Vary each control and watch the rail readouts respond.
  • Compare the diagnostic plot against the live scene.