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<p>Likewise, although an object with mass above approximately 0.013 solar masses will be able to <a href="page.php?w=deuterium_burning">fuse deuterium</a> for a time, this source of energy will be exhausted in approximately 100million years. Apart from these sources, the radiation of an isolated substellar object comes only from the release of its <a href="page.php?w=gravitational_potential_energy">gravitational potential energy</a>, which causes it to gradually cool and shrink. A substellar object in <a href="page.php?w=orbit">orbit</a> around</p><p>
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