論文

基本情報

氏名 渡邉 誠
氏名(カナ) ワタナベ マコト
氏名(英語) Watanabe Makoto
所属 理学部 物理学科
職名 准教授
researchmap研究者コード B000222325
researchmap機関 岡山理科大学

題名

Dust Properties of the Interstellar Object 3I/ATLAS Revealed by Optical and Near-Infrared Polarimetry

単著・共著の別

共著

著者

Seungwon Choi, Masateru Ishiguro, Jun Takahashi, Tomoki Saito, Yoonsoo P. Bach, Bumhoo Lim, Hiroyuki Naito, Jooyeon Geem, Sunho Jin, Jinguk Seo, Hyeonwoo Ju, Hiroshi Akitaya, Koji S. Kawabata, Mahito Sasada, Kazuya Doi, Hisayuki Kubota, Seiko Takagi, Makoto Watanabe, Tomohiko Sekiguchi, Myungshin Im

概要

We present independent polarimetric observations of the interstellar object 3I/ATLAS, including the first near-infrared polarimetric measurements. Using imaging polarimeters, we measured the degree of linear polarization from the visible R <sub>C</sub> band (0.64  μ m) to the near-infrared K <sub>s</sub> band (2.25  μ m), and investigated its dependence on solar phase angle (polarization phase curve, PPC) and wavelength (polarization color curve, PCC). We confirm that the PPC of 3I/ATLAS differs significantly from those of typical solar system comets, showing an unusually large polarization amplitude. This PPC shows no significant change in the R <sub>C</sub> band across perihelion passage, despite the perihelion lying within the water snow line. This indicates that the unusual polarimetric behavior of 3I/ATLAS is unlikely to be driven by transient volatile activity, but instead reflects intrinsic optical properties of refractory dust particles. The PCC increases with wavelength over 0.6–1.2  μ m and peaks at 1.5–2.0  μ m, suggesting that the dominant scattering units are dust aggregates composed of submicron-sized monomers, broadly consistent with interstellar dust and solar-system cometary aggregates. Taken together, our results indicate that 3I/ATLAS preserves polarimetric properties characteristic of a primitive cometary planetesimal formed in another planetary system, with a refractory dust composition that differs from that typically observed among solar system comets, despite sharing a similar size scale of the aggregate building blocks.

発表雑誌等の名称

The Astrophysical Journal Letters

出版者

1000

1

開始ページ

L29

終了ページ

発行又は発表の年月

2026/03

査読の有無

有り

招待の有無

無し

記述言語

英語

掲載種別

研究論文(学術雑誌)

ISSN

ID:DOI

10.3847/2041-8213/ae497c

ID:NAID(CiNiiのID)

ID:PMID

URL

JGlobalID

arXiv ID

ORCIDのPut Code

DBLP ID