论文标题

命运的同时多色光度法

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

论文作者

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

论文摘要

(3200)phaethon到较低角度的亮度的准确估计对于计划命运$^{+} $任务的板载摄像头至关重要。我们已经在2021年10月和11月的Seimei 3.8 m望远镜上使用TRICCS摄像头进行了光波长($ g $,$ r $ $ $ $ $ $ $ $ $ $和$ i $)的Phaethon的密集观察。我们得出了绝对的幅度$ h_ \ Mathrm {v} $和slope parame $ g $ g $ g $ g $ $ H_ \ MATHRM {V} = 14.23 \ PM0.02 $和$ G = 0.040 \ PM0.008 $,来自多个光度观测值,包括$ h $ g $型号,包括较低相角,降低至$ \ sim $ 9 $^{\ sim $ 9 $^{\ circ} $。使用$ h_ \ mathrm {v} $值和先前偏光研究中衍生的phaethon的几何反照率,我们估计,Phaethon的直径在5.22至6.74 km的范围内,这与雷达和掩盖观察值一致。使用线性模型,我们得出了$ H_ \ Mathrm {V} = 14.65 \ PM0.02 $,这对应于4.30至5.56 km的直径范围。我们同时的phaethon的三色灯弯曲表明,在2021年的幻影下,G-R和R-I颜色中没有旋转光谱变化大于0.018和0.020 mag,可能与表面材料和/或结构的不均匀性有关。

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.

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