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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 10.

Figure shows the fitting of our derived shape model to the observational data obtained on 2014 May 2. Since the 2014 data were collected during the active period, and the pole orientation and rotation period differ from those derived in 2025, we adopted the updated pole orientation and related parameters.

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