| Literature DB >> 32457956 |
Brian D Warner1, Vladimir Benishek2, Andrea Ferrero3.
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.Entities:
Year: 2014 PMID： 32457956 PMCID： PMC7249606
Source DB: PubMed Journal: Minor Planet Bull