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Relativistic Beaming

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When a star or other light-emitting object is moving close to the speed of light relative to an observer, it exhibits something called "beaming". Even though an observer moving the same speed as the star would see light emitted in all directions, if the star is moving, the light gets more focused in the direction of motion.
This animation shows relativistic beaming for a star moving to the right, relative to an observer (us). Each second of the animation increases the star's relative velocity by 10% of light-speed, ending when the star is moving 99% of the speed of light. I also included a (highly inaccurate) depiction of the Doppler effect, wherein observers will see the light's wavelength decrease - blueshift - if the star is moving toward them, while if the star is moving away, they will see a redshift.
This animation shows relativistic beaming for a star moving to the right, relative to an observer (us). Each second of the animation increases the star's relative velocity by 10% of light-speed, ending when the star is moving 99% of the speed of light. I also included a (highly inaccurate) depiction of the Doppler effect, wherein observers will see the light's wavelength decrease - blueshift - if the star is moving toward them, while if the star is moving away, they will see a redshift.
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