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<p>A star with a planet will move in its own small orbit in response to the planet's gravity. This leads to variations in the speed with which the star moves toward or away from Earth, i.e. the variations are in the <a href="page.php?w=radial_velocity">radial velocity</a> of the star with respect to Earth. The radial velocity can be deduced from the displacement in the parent star's <a href="page.php?w=spectral_line">spectral line</a>s due to the <a href="page.php?w=Doppler_effect">Doppler effect</a>. The radial-velocity method measures these variations</p><p>
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