CCD photometry observations of the near-Earth asteroid (NEA) 2010 TN 54 indicates a period of either 6.14 h or 12.12 h, depending on whether a monomodal or bimodal lightcurve is adopted. The amplitude was only 0.07 ± 0.01 mag, which - along with the period being nearly commensurate with an Earth day - made finding a definitive solution difficult, despite being observed from locations in North America and Europe.
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| http://www.ncbi.nlm.nih.gov/pmc/articles/PMC7249606 | PMC |
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