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Updated: Dec 20, 2025

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
Published on: May 10, 2020
LIGHTCURVE ANALYSIS OF NEAR-EARTH ASTEROID 2010 TN54
Brian D Warner1, Vladimir Benishek2, Andrea Ferrero3
1Center for Solar System Studies - Palmer Divide Station, 446 Sycamore Ave, Eaton, CO 80615 USA.
Abstract:
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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