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

被引:3
作者
Beniyama, Jin [1 ,2 ]
Sekiguchi, Tomohiko [3 ]
Kuroda, Daisuke [4 ,5 ]
Arai, Tomoko [6 ]
Ishibashi, Ko [6 ]
Ishiguro, Masateru [7 ,8 ]
Yoshida, Fumi [6 ,9 ]
Senshu, Hiroki [6 ]
Ootsubo, Takafumi [10 ]
Sako, Shigeyuki [1 ,11 ,12 ]
Ohsawa, Ryou [10 ]
Takita, Satoshi [1 ]
Geem, Jooyeon [7 ,8 ]
Bach, Yoonsoo P. [7 ,8 ]
机构
[1] Univ Tokyo, Inst Astron, Grad Sch Sci, 2-21-1 Osawa, Mitaka, Tokyo 1810015, Japan
[2] Univ Tokyo, Grad Sch Sci, Dept Astron, 7-3-1 Hongo,Bunkyo Ku, Tokyo 1130033, Japan
[3] Hokkaido Univ, Asahikawa Campus,Hokumon 9, Asahikawa, Hokkaido 0708621, Japan
[4] Kyoto Univ, Okayama Observ, 3037-5 Honjo,Kamogata Cho, Asakuchi, Okayama 7190232, Japan
[5] Japan Spaceguard Assoc, Bisei Spaceguard Ctr, 1716-3 Okura, Ibara, Okayama 7141411, Japan
[6] Chiba Inst Technol, Planetary Explorat Res Ctr, 2-17-1 Tsudanuma, Narashino, Chiba 2750016, Japan
[7] Seoul Natl Univ, Dept Phys & Astron, 1 Gwanak Ro, Seoul 08826, South Korea
[8] Seoul Natl Univ, SNU Astron Res Ctr, 1 Gwanak Ro, Seoul 08826, South Korea
[9] Univ Occupat & Environm Hlth, Sch Med, Dept Basic Sci, 1-1 Iseigaoka, Yahata, Kitakyusyu 8078555, Japan
[10] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
[11] Univ Tokyo, UTokyo Org Planetary Space Sci, 7-3-1 Hongo,Bunkyo Ku, Tokyo 1130033, Japan
[12] Univ Tokyo, Collaborat Res Org Space Sci & Technol, 7-3-1 Hongo,Bunkyo Ku, Tokyo 1130033, Japan
关键词
methods; observational - minor planets; asteroids; individual (Phaethon)-techniques; photometric; 2005; UD; SURFACE HETEROGENEITY; STREAM;
D O I
10.1093/pasj/psac109
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 similar to 9? with the H-G model. Using the HVvalue 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.
引用
收藏
页码:297 / 310
页数:14
相关论文
共 61 条
[1]   REFINED ROTATIONAL PERIOD, POLE SOLUTION, AND SHAPE MODEL FOR (3200) PHAETHON [J].
Ansdell, Megan ;
Meech, Karen J. ;
Hainaut, Olivier ;
Buie, Marc W. ;
Kaluna, Heather ;
Bauer, James ;
Dundon, Luke .
ASTROPHYSICAL JOURNAL, 2014, 793 (01)
[2]  
Arai T., 2018, LPI, V2083, P2570
[3]  
Arai T., 2022, LUNAR PLANET I CONTR, V2678, P2916
[4]   Video observations of tiny near-Earth objects with Tomo-e Gozen [J].
Beniyama, Jin ;
Sako, Shigeyuki ;
Ohsawa, Ryou ;
Takita, Satoshi ;
Kobayashi, Naoto ;
Okumura, Shin-ichiro ;
Urakawa, Seitaro ;
Yoshikawa, Makoto ;
Usui, Fumihiko ;
Yoshida, Fumi ;
Doi, Mamoru ;
Niino, Yuu ;
Shigeyama, Toshikazu ;
Tanaka, Masaomi ;
Tominaga, Nozomu ;
Aoki, Tsutomu ;
Arima, Noriaki ;
Arimatsu, Ko ;
Kasuga, Toshihiro ;
Kondo, Sohei ;
Mori, Yuki ;
Takahashi, Hidenori ;
Watanabe, Jun-ichi .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2022, 74 (04) :877-903
[5]   SExtractor: Software for source extraction [J].
Bertin, E ;
Arnouts, S .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1996, 117 (02) :393-404
[6]   Rotational variation of the linear polarization of the asteroid (3200) Phaethon as evidence for inhomogeneity in its surface properties [J].
Borisov, G. ;
Devogele, M. ;
Cellino, A. ;
Bagnulo, S. ;
Christou, A. ;
Bendjoya, Ph. ;
Rivet, J. -P. ;
Abe, L. ;
Vernet, D. ;
Donchev, Z. ;
Krugly, Yu. ;
Belskaya, I. ;
Bonev, T. ;
Steeghs, D. ;
Galloway, D. ;
Dhillon, V. ;
O'Brien, P. ;
Pollacco, D. ;
Poshyachinda, S. ;
Ramsay, G. ;
Thrane, E. ;
Ackley, K. ;
Rol, E. ;
Ulaczyk, K. ;
Cutter, R. ;
Dyer, M. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2018, 480 (01) :L131-L135
[7]  
BOWELL E, 1989, ASTEROIDS II, P524
[8]  
Bus S. J., 1999, THESIS MIT
[9]   Phase II of the Small Main-belt Asteroid Spectroscopic Survey - A feature-based taxonomy [J].
Bus, SJ ;
Binzel, RP .
ICARUS, 2002, 158 (01) :146-177
[10]  
Chambers K. C., 2016, ARXIV