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Stellar aberration of light

What you are seeing: star positions as they appear to an observer moving at velocity βc\beta c along the +x+x axis, compared to their rest-frame positions. The Lorentz aberration formula cosθobs=(cosθrest+β)/(1+βcosθrest)\cos\theta_\text{obs} = (\cos\theta_\text{rest} + \beta) / (1 + \beta \cos\theta_\text{rest}) pulls every star toward the forward direction (relativistic beaming in geometry). For Earth's annual orbital aberration (β104\beta \approx 10^{-4}), the maximum shift is the classical constant of aberration 20.5"\approx 20.5".

Rest-frame stars are drawn at uniform angles around the observer (cyan dots); their observed positions cluster forward (orange dots). Connecting lines show the shift; the maximum-shift line is highlighted in accent. As β1\beta \to 1 the entire visible sphere concentrates into a forward cone.

Figure 1. Stellar aberration: rest vs observed positions on a polar plot. Method: closed-form Lorentz aberration.
log10 beta-4.00

WHAT TO TRY

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