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Photometric Observations and Analysis of Active Asteroid (62412) 2000 SY178

  • Authors: Xiangyu Fan, Xiliang Zhang, Xiaomeng Xu, Ling Wang

Xiangyu Fan et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 5.

Phased best fit double-peaked period for 2000 SY178 of 3.3282 hr. Fitting adopted a 6th Fourier series and the order is determined by F-test. The maximum peak-to-peak amplitude is 0.56 ± 0.02. The two lower peaks have a difference of about 0.08 mag, showing 2000 SY178 has an elongated irregular shape and a light curve dominated by shape rather than albedo effects.

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