 Angular size under a collinear relativistic boost

Let an observer move towards the centre of a small distant source with velocity $\beta c$, where $c$ is the speed of light. For source-direction angle $\theta$, the photon arrives with longitudinal momentum $-E\cos \theta /c$. A Lorentz transformation gives $E^{\prime }=\gamma E(1+\beta \cos \theta )$ and therefore the relativistic aberration lawwhere $\eta =\mathrm{artanh}\beta$ is the rapidity. For a small angular diameter $\Theta$, the displayed angular-size ratio follows by linearizing at $\theta =0$. Two momentarily coincident observers can consequently measure different angular sizes without any change in their observation event. If their diameter ratio is $q\ge 1$, their relative speed is $c(q^2-1)/(q^2+1)$.