Math 2.0

Astronomy and astrophysics Spherical astronomy and astrometry Proposition

Aberration of light

Builds on Celestial sphere

Statement

Let SS be an inertial frame, and let an observer move with constant velocity vv relative to SS. Let cc be the speed of light, and let β=∣v∣/c\beta = \abs{v}/c, with 0≤β<10 \le \beta < 1. Let light from a distant source arrive at the observer. Let θ∈[0,π]\theta \in [0, \pi] be the angle in SS between vv and the direction towards the source. Then the observer sees the source at the angle θ′\theta' from the direction of motion, where cos⁡θ′=cos⁡θ+β1+βcos⁡θ.\cos\theta' = \frac{\cos\theta + \beta}{1 + \beta\cos\theta}. In particular θ′≤θ\theta' \le \theta, with equality only when β=0\beta = 0 or sin⁡θ=0\sin\theta = 0, and θ−θ′=βsin⁡θ+O(β2)\theta - \theta' = \beta\sin\theta + O(\beta^2).

Remarks

The light travels in the direction −n-n, where nn is the unit vector towards the source. Apply the Lorentz transformation to the photon's energy EE and momentum component p∥=−(E/c)cos⁡θp_\parallel = -(E/c)\cos\theta along vv. This gives E′=γE(1+βcos⁡θ)E' = \gamma E (1 + \beta\cos\theta) and c p∥′=−γE(cos⁡θ+β)c\,p'_\parallel = -\gamma E(\cos\theta + \beta), with γ=(1−β2)−1/2\gamma = (1 - \beta^2)^{-1/2}, and the formula follows. So a moving observer sees all sources shifted towards the point on the celestial sphere towards which it moves. Example: the Earth's orbital speed is about 29.829.8 km/s, so β≈9.9×10−5\beta \approx 9.9 \times 10^{-5}. In radians this is about 20.5′′20.5'', the constant of annual aberration. Over a year each star traces a small ellipse of semi-major axis about 20.5′′20.5''.

Going deeper

For a student

The exact formula is the relativistic transformation of directions of light rays between two inertial frames. To first order in β\beta it agrees with the classical picture of adding the observer's velocity to the velocity of light. In astrometry one distinguishes annual aberration, from the orbital motion of the Earth, and diurnal aberration, from its rotation, which is at most about 0.32′′0.32''. Unlike parallax, aberration does not depend on the distance of the star, only on its direction. James Bradley discovered annual aberration while he was looking for stellar parallax.

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  1. Celestial sphere concept
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Further reading

  1. Web https://en.wikipedia.org/wiki/Aberration_(astronomy)
About this page
TagWBCV84VHEH
URIm2://WBCV84VHEH
Kindstatement, proposition
WritingW0 stub
MSC85A04, 83A05
StatusThis copy of the site has no build data. Run m2 status WBCV84VHEH.
AboutCelestial sphere
UsesCelestial sphere
Changed3 November 2026

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