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<p>The study in 2012, utilizing a <a href="page.php?w=Rossiter-McLaughlin_effect">Rossiter-McLaughlin effect</a>, have determined the planetary orbit is probably aligned with the equatorial plane of the star, misalignment equal to °.</p>

<p><big>Physical characteristics</big></p>
<p>The planet is slightly less massive than <a href="page.php?w=Jupiter">Jupiter</a> (0.919 ± 0.073 ) but its diameter is 84% larger. This give TrES-4 an average density of only about a third of a gram per cubic centimetre, approximately the same as <a href="page.php?w=Saturn">Saturn</a>'s</p><p>
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