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arXiv 2212.09323astro-ph.EP
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DESTINY $^{+}$目标小行星(3200)Phaethon的同时多色Photometry

Simultaneous Multicolor Photometry of the DESTINY$^{+}$ target asteroid (3200) Phaethon

Jin Beniyama, Tomohiko Sekiguchi, Daisuke Kuroda, Tomoko Arai, Ko Ishibashi, Masateru Ishiguro, Fumi Yoshida, Hiroaki Senshu, Takafumi Ootsubo, Shigeyuki Sako, … 展开作者

Jin Beniyama, Tomohiko Sekiguchi, Daisuke Kuroda, Tomoko Arai, Ko Ishibashi, Masateru Ishiguro, Fumi Yoshida, Hiroaki Senshu, Takafumi Ootsubo, Shigeyuki Sako, Ryou Ohsawa, Satoshi Takita, Jooyeon Geem, Yoonsoo P. Bach

摘要:

精确估计(3200)Phaethon的亮度直到较低的相位角对于DESTINY $^{+}$飞行任务的机载照相机的规划是必不可少的。我们于2021年10月和11月在Seimei 3.8 m望远镜上使用TriCCS相机对Phaethon进行了光学波长($g$,$r$和$i$)的密集观测。我们利用$H$-$G$模型,从多次测光观测(包括低相角观测到$\sim$ 9 $^{\circ}$)中导出了法厄同的绝对星等$H_\mathrm{V}$和斜率参数$G$,分别为$H_\mathrm{V}=14.23\pm0.02$和$G=0.040\pm0.008$.利用$H_\mathrm{V}$值和以往偏振研究中导出的Phaethon的几何参数,我们估计Phaethon的直径在5.22 ~ 6.74 km之间,这与雷达和掩星观测结果是一致的。利用线性模型,我们导出了$H_\mathrm{V}=14.65\pm0.02$,它对应于4.30 - 5.56 km的直径范围。我们的同步三色光变曲线表明,没有旋转光谱变化大于0.018和0.020等的g-r和r-i的颜色,可能与表面材料和/或结构的不均匀性,被认为是在2021年的幻影。

英文摘要:

Accurate estimation of brightness of (3200) Phaethon up to lower phase angles are essential for planning of the on-board camera of the DESTINY$^{+}$ mission. We have carried out intensive observations of Phaethon in the optical wavelength ($g$, $r$, and $i$) with the TriCCS camera on the Seimei 3.8 m telescope in October and November, 2021. We derived the absolute magnitude $H_\mathrm{V}$ and the slope parameter $G$ of Phaethon as $H_\mathrm{V}=14.23\pm0.02$ and $G=0.040\pm0.008$ from multiple photometric observations including lower phase angles down to $\sim$9$^{\circ}$ with the $H$-$G$ model. Using the $H_\mathrm{V}$ value and the geometric albedo of Phaethon derived in previous polarimetric studies, we estimated that the Phaethon's diameter is within a range of 5.22 to 6.74 km, which is consistent with radar and occultation observations. With the linear model, we derived $H_\mathrm{V}=14.65\pm0.02$, which corresponds to a diameter range of 4.30 to 5.56 km. Our simultaneous tricolor lightcurves of Phaethon indicate that no rotational spectral variations larger than 0.018 and 0.020 mag in the g-r and r-i colors, possibly related to inhomogeneity of the surface material and/or structure, are seen at the 2021 apparition.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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