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<p>stars can be calculated using accurate orbital parameters. Both members of the spectroscopic binary Delta Velorum A are slightly <a href="page.php?w=stellar_evolution">evolved</a> stars that are still on the <a href="page.php?w=main_sequence">main sequence</a>. Component Aa has 2.5 times the <a href="page.php?w=mass_of_the_Sun">mass of the Sun</a>, 2.6 times the <a href="page.php?w=Sun%27s_radius">Sun's radius</a>, and is radiating 56 times the <a href="page.php?w=luminosity_of_the_Sun">luminosity of the Sun</a> at an <a href="page.php?w=effective_temperature">effective temperature</a></p><p>
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