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(3200) Phaethon polarimetry in the negative branch: new evidence for the anhydrous nature of the DESTINY+ target asteroid
Department of Physics and Astronomy, Seoul National University , 1 Gwanak-ro, Gwanak-gu, Seoul 08826, Republic of Korea; SNU Astronomy Research Center, Seoul National University , 1 Gwanak-ro, Gwanak-gu, Seoul 08826, Republic of Korea.
Department of Physics and Astronomy, Seoul National University , 1 Gwanak-ro, Gwanak-gu, Seoul 08826, Republic of Korea; SNU Astronomy Research Center, Seoul National University , 1 Gwanak-ro, Gwanak-gu, Seoul 08826, Republic of Korea.ORCID iD: 0000-0002-7332-2479
Center for Astronomy, University of Hyogo , 407-2 Nishigaichi, Sayo, Hyogo 679-5313, Japan.
Planetary Exploration Research Center, Chiba Institute of Technology , 2-17-1 Tsudanuma, Narashino, Chiba 275-0016, Japan.ORCID iD: 0000-0001-6156-238X
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2022 (English)In: Monthly Notices of the Royal Astronomical Society: Letters, ISSN 1745-3925, Vol. 516, no 1, p. L53-L57Article in journal (Refereed) Published
Abstract [en]

We report on the first polarimetric study of (3200) Phaethon, the target of JAXA’s DESTINY+ mission, in the negative branch to ensure its anhydrous nature and to derive an accurate geometric albedo. We conducted observations at low phase angles (Sun-target-observer angle, α = 8.8–32.4°) from 2021 October to 2022 January and found that Phaethon has a minimum polarization degree Pmin = −1.3 ± 0.1  per cent, a polarimetric slope h = 0.22 ± 0.02  per cent deg−1, and an inversion angle α0 = 19.9 ± 0.3°. The derived geometric albedo is pV = 0.11 (in the range of 0.08–0.13). These polarimetric properties are consistent with anhydrous chondrites, contradict hydrous chondrites, and typical cometary nuclei.

Place, publisher, year, edition, pages
Oxford University Press, 2022. Vol. 516, no 1, p. L53-L57
Keywords [en]
techniques: polarimetric, minor planets, asteroids: individual: (3200) Phaethon
National Category
Astronomy, Astrophysics and Cosmology
Research subject
Onboard space systems
Identifiers
URN: urn:nbn:se:ltu:diva-92520DOI: 10.1093/mnrasl/slac072ISI: 000934001900010Scopus ID: 2-s2.0-85144853670OAI: oai:DiVA.org:ltu-92520DiVA, id: diva2:1688040
Note

Validerad;2022;Nivå 1;2022-12-02 (sofila);

Funder: National Research Foundation of Korea (grant no.  2018R1D1A1A09084105); the Optical & Near- Infrared Astronomy Inter-University Cooperation Program, MEXT, of Japan; Hypervelocity Impact Facility, ISAS; Japan Aerospace Exploration Agency. JAXA; Japan Society for the Promotion of Science (JSPS) KAKENHI (grant no. 20K14541)

Available from: 2022-08-17 Created: 2022-08-17 Last updated: 2025-10-21Bibliographically approved

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Granvik, Mikael

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Ishiguro, MasateruAkitaya, HiroshiKawabata, Koji SHasegawa, SunaoBeniyama, JinGranvik, MikaelKasikov, AnniKnudstrup, Emil
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