<?xml version="1.0" encoding='utf-8'?>
<!DOCTYPE wml PUBLIC "-//WAPFORUM//DTD WML 1.1//EN" "http://www.wapforum.org/DTD/wml_1.1.xml">
<wml>
<card id="card1" title="Doppler spectroscopy - Page 3 - Wikipedia">
<p>
<a accesskey="1" href="page.php?w=Doppler_spectroscopy&amp;p=2">1.Previous</a><br />
<a accesskey="3" href="page.php?w=Doppler_spectroscopy&amp;p=4">3.Next</a>
</p>
<p>orbit around their center of mass. He predicted that the small Doppler shifts to the light emitted by the star, caused by its continuously varying radial velocity, would be detectable by the most sensitive spectrographs as tiny <a href="page.php?w=redshift">redshift</a>s and <a href="page.php?w=blueshift">blueshift</a>s in the star's emission. However, the technology of the time produced radial-velocity measurements with errors of 1,000&nbsp;<a href="page.php?w=Metre_per_second">m/s</a> or more, making them useless for the detection of orbiting</p><p>
<a accesskey="1" href="page.php?w=Doppler_spectroscopy&amp;p=2">1.Previous</a><br />
<a accesskey="3" href="page.php?w=Doppler_spectroscopy&amp;p=4">3.Next</a>
</p>

<do type="prev" label="Search">
        <go href="search.wml"/>
</do>

</card>
</wml>
