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<p><a href="page.php?w=Photometry_%28astronomy%29">photometry</a> of Varuna's light curve in 2001 revealed that it displays large brightness variations with an <a href="page.php?w=amplitude">amplitude</a> of about 0.5 <a href="page.php?w=magnitude_%28astronomy%29">magnitude</a>s. The measured rotational light curve of Varuna provided two ambiguous rotation periods of 3.17 and 6.34 hours, for a single-peaked and a double-peaked solution, respectively. Additional possible rotation periods of 2.79 and 3.66 hours were also obtained by Farnham, although</p><p>
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