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<a accesskey="3" href="page.php?w=Cepheid_variable&amp;p=2">3.Next</a>
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<p>A <b>Cepheid variable</b>  is a type of <a href="page.php?w=variable_star">variable star</a> that <a href="page.php?w=Instability_strip">pulsates radially</a>, varying in both diameter and temperature. It changes in brightness, with a well-defined stable <a href="page.php?w=frequency">period</a> (typically 1-100 days) and amplitude. Cepheids are important cosmic benchmarks for scaling <a href="page.php?w=cosmic_distance_ladder">galactic and extragalactic distances</a>; a strong direct <a href="page.php?w=period-luminosity_relation">relationship</a></p><p>
<a accesskey="3" href="page.php?w=Cepheid_variable&amp;p=2">3.Next</a>
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