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<p><big>Moons of giant planets</big></p>
<p>Tidal heating is responsible for the geologic activity of the most volcanically active body in the <a href="page.php?w=Solar_System">Solar System</a>: <a href="page.php?w=Io_%28moon%29">Io</a>, a moon of <a href="page.php?w=Jupiter">Jupiter</a>. Io's eccentricity persists as the result of its <a href="page.php?w=Laplace_resonance">orbital resonance</a>s with the <a href="page.php?w=Galilean_moons">Galilean moons</a> <a href="page.php?w=Europa_%28moon%29">Europa</a> and <a href="page.php?w=Ganymede_%28moon%29">Ganymede</a>.</p><p>
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