Multi-epoch spectrophotometric characterization of the mini-moon 2024 PT5 in the visible and near-infrared

IF 5.8 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Jin Beniyama, Bryce T. Bolin, Alexey V. Sergeyev, Marco Delbo, Laura-May Abron, Matthew Belyakov, Tomohiko Sekiguchi, Seiko Takagi
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引用次数: 0

Abstract

Context. 2024 PT5 is a tiny (D ≤ 10 m) near-Earth asteroid (NEA) discovered in August 2024. 2024 PT5 was gravitationally bound to the Earth-Moon system from September to November 2024 and classified as a mini-moon. Several quick response observations suggest that 2024 PT5 has a lunar ejecta origin, while the rotation state and albedo, essential properties for investigating its origin, are not well constrained.Aims. We aim to characterize the spectrophotometric properties of 2024 PT5 by ground-based observations to test its taxonomic classification and origin.Methods. We performed visible to near-infrared multicolor photometry of 2024 PT5 from data taken using the TriColor CMOS Camera and Spectrograph (TriCCS) on the Seimei 3.8 m telescope during January 4–10, 2025. The Seimei/TriCCS observations of 2024 PT5 cover phase angles from 14 deg to 27 deg, and were obtained in the ɡ, r, i, and ɀ bands in the Pan-STARRS system. In addition, we analyzed Y, J, H, and K photometry taken with the Multi-Object Spectrograph for Infrared Exploration (MOSFIRE) on the Keck I 10-m telescope on January 16–17, 2025.Results. Our light curves show brightness variations over time periods of several tens of minutes. We infer that 2024 PT5 is in a tumbling state and has a light curve amplitude of about 0.3 mag. Visible and near-infrared color indices of 2024 PT5, ɡr = 0.567 ± 0.044, ri = 0.155 ± 0.009, rɀ = 0.147 ± 0.066, YJ = 0.557 ± 0.046, JH = 0.672 ± 0.078, and HKs = 0.148 ± 0.098, indicate that 2024 PT5 is an S-complex asteroid, largely consistent with previous observations. Using the HG model, we derived an absolute magnitude, HV,HG, of 27.72 ± 0.09 and a slope parameter, GV, of 0.223 ± 0.073 in the V band. A geometric albedo of 2024 PT5 was derived to be 0.26 ± 0.07 from the slope of its photometric phase curve. This albedo value is typical of the S- and Q-type NEAs.Conclusions. Using the albedo and absolute magnitude, the equivalent diameter of 2024 PT5 is estimated to be 7.4 ± 1.0 m. The color properties of 2024 PT5 derived from our observations match the ones of rock samples taken from the lunar surface, which agrees with previous studies.
小卫星2024 PT5的多历元可见光和近红外光谱特征
2024 PT5是2024年8月发现的一颗微小的(直径≤10米)近地小行星(NEA)。2024 PT5于2024年9月至11月被引力绑定在地月系统,被归类为迷你卫星。几项快速响应观测表明,2024 PT5有月球抛射物的起源,而研究其起源的基本属性旋转状态和反照率并没有得到很好的限制。目的通过地面观测表征2024 PT5的分光光度特性,以验证其分类和来源。我们利用晴明3.8 m望远镜上的三色CMOS相机和光谱仪(TriCCS)在2025年1月4日至10日期间拍摄的数据,对2024 PT5进行了可见光到近红外的多色光度测定。2024 PT5的晴明/TriCCS观测覆盖了14 ~ 27°的相位角,在Pan-STARRS系统中获得了j、r、i和z波段的观测数据。此外,我们还分析了Keck I 10米望远镜上的多目标红外探测光谱仪(MOSFIRE)于2025年1月16日至17日拍摄的Y、J、H和K光度。我们的光曲线显示了几十分钟内亮度的变化。我们推断2024 PT5处于下跌状态,光变曲线幅度约0.3杂志。2024 PT5的可见光和近红外的颜色指数,ɡ- r = 0.567±0.044,r - i = 0.155±0.009,0.147±0.066 r -ɀ=,Y - J = 0.557±0.046,J - H = 0.672±0.078,和H - k = 0.148±0.098,表明2024年PT5是一个中心的小行星,很大程度上与以前的观测一致。利用H-G模型,我们得到了V波段的绝对星等HV,HG为27.72±0.09,斜率参数GV为0.223±0.073。根据其光度相曲线斜率,推导出2024 PT5的几何反照率为0.26±0.07。该反照率值是典型的S型和q型nea。利用反照率和绝对星等,估计2024 PT5的等效直径为7.4±1.0 m。从我们的观察中得出的2024 PT5的颜色特性与从月球表面采集的岩石样本的颜色特性相匹配,这与之前的研究一致。
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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