Simultaneous multicolor photometry of the DESTINY+ target asteroid (3200) Phaethon

Author:

Beniyama Jin12ORCID,Sekiguchi Tomohiko3ORCID,Kuroda Daisuke45ORCID,Arai Tomoko6ORCID,Ishibashi Ko6,Ishiguro Masateru78ORCID,Yoshida Fumi69ORCID,Senshu Hiroki6,Ootsubo Takafumi10,Sako Shigeyuki11112ORCID,Ohsawa Ryou10ORCID,Takita Satoshi1,Geem Jooyeon78ORCID,Bach Yoonsoo P78ORCID

Affiliation:

1. Institute of Astronomy, Graduate School of Science, The University of Tokyo , 2-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan

2. Department of Astronomy, Graduate School of Science, The University of Tokyo , 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

3. Asahikawa Campus, Hokkaido University of Education , Hokumon 9, Asahikawa, Hokkaido 070-8621, Japan

4. Okayama Observatory, Kyoto University , 3037-5 Honjo, Kamogata-cho, Asakuchi, Okayama 719-0232, Japan

5. Bisei Spaceguard Center, Japan Spaceguard Association , 1716-3 Okura, Bisei, Ibara, Okayama 714-1411, Japan

6. Planetary Exploration Research Center, Chiba Institute of Technology , 2-17-1 Tsudanuma, Narashino, Chiba 275–0016, Japan

7. Department of Physics and Astronomy, Seoul National University , 1 Gwanak-ro, Gwanak-gu, Seoul 08826, Republic of Korea

8. SNU Astronomy Research Center, Seoul National University , 1 Gwanak-ro, Gwanak-gu, Seoul 08826, Republic of Korea

9. School of Medicine, Department of Basic Sciences, University of Occupational and Environmental Health , 1-1 Iseigaoka, Yahata, Kitakyusyu 807-8555, Japan

10. National Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

11. UTokyo Organization for Planetary Space Science, The University of Tokyo , 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

12. Collaborative Research Organization for Space Science and Technology, The University of Tokyo , 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

Abstract

Abstract Accurate estimations of the brightness of (3200) Phaethon up to lower phase angles are essential for the planning of the on-board camera for the DESTINY+ mission. We 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 2021 October and November. We derived the absolute magnitude HV and the slope parameter G of Phaethon as HV = 14.23 ± 0.02 and G = 0.040 ± 0.008 from multiple photometric observations including lower phase angles down to ∼9° with the H–G model. Using the HV value and the geometric albedo of Phaethon derived in previous polarimetric studies, we estimated that Phaethon’s diameter is within a range of 5.22–6.74 km, which is consistent with radar and occultation observations. With the linear model, we derived HV = 14.65 ± 0.02, which corresponds to a diameter range of 4.30–5.56 km. Our simultaneous tricolor light curves 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.

Funder

Iwadare Scholarship Foundation

Ministry of Education, Culture, Sports, Science and Technology

JSPS

NAOJ

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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