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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 3.

After the solar color has been removed, the spectral slope of the asteroid is shown in the figure. The data of 2014 were taken from the S. S. Sheppard & C. Trujillo (2015), and corresponding color is ﹩{g}^{{\prime} }-{r}^{{\prime} }=0.43\pm 0.02﹩, ﹩{r}^{{\prime} }-{i}^{{\prime} }=0.14\pm 0.02﹩, ﹩{i}^{{\prime} }-{z}^{{\prime} }﹩ = –0.01 ± 0.02. The relatively flat spectral slope indicates that 2000 SY178 is a C-type asteroid.

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