Multi-chord observation of stellar occultation by the near-Earth asteroid (3200) Phaethon on 2021 October 3 (UTC) with very high accuracy. (20th December 2022)
- Record Type:
- Journal Article
- Title:
- Multi-chord observation of stellar occultation by the near-Earth asteroid (3200) Phaethon on 2021 October 3 (UTC) with very high accuracy. (20th December 2022)
- Main Title:
- Multi-chord observation of stellar occultation by the near-Earth asteroid (3200) Phaethon on 2021 October 3 (UTC) with very high accuracy
- Authors:
- Yoshida, Fumi
Hayamizu, Tsutomu
Miyashita, Kazuhisa
Watanabe, Hiroyuki
Yamamura, Hidehito
Akitaya, Hiroshi
Asai, Akira
Fujiwara, Yasunori
Goto, Tateki
Hashimoto, George L
Hatanaka, Akitoshi
Horaguchi, Toshihiro
Ida, Miyoshi
Imamura, Kazuyoshi
Isobe, Ken
Ishiguro, Masateru
Kaizuka, Noboru
Kasebe, Hisashi
Kawasaki, Yohei
Kim, Taewoo
Kitazaki, Katsuhiko
Manago, Norihiro
Matsumura, Masafumi
Matsushita, Hiroshi
Matsuura, Shuji
Nakamura, Takahiro
Nagata, Toshihiro
Noda, Hirotomo
Ogawa, Masaaki
Ohshima, Osamu
Owada, Minoru
Saitou, Kazuyuki
Tsumura, Mitsunori
Ueyama, Yoshihiro
Watanabe, Hayato
Yamamoto, Masa-yuki
Yoshihara, Hideki
Fujiwara, Takao
Haraguchi, Miyu
Hayashi, Hironori
Hitotsuda, Tomoya
Horikawa, Toshihiro
Ishida, Kai
Ito, Tadashi
Jin, Sunho
Kang, Wonseok
Katayama, Toshihiko
Kawabata, Koji S
Kawasaki, Ryosuke
Kim, Kihyeon
Kita, Masayuki
Kitazaki, Naoko
Kurisu, Hiroya
Matsushima, Makoto
Matsumi, Chika
Mihari, Ayami
Naka, Masaru
Nakaoka, Tatsuya
Nishihama, Reiko
Nishiyama, Yukio
Nukui, Sadao
Oba, Masahiko
Okamoto, Takaya
Omori, Yujiro
Seo, Jinguk
Shirakawa, Hiroki
Sugino, Tomoshi
Tani, Yuki
Takagaki, Kazuhiko
Ueda, Yukikazu
Urakawa, Seitaro
Watanabe, Masanari
Yamashita, Kouhei
Yamashita, Misato
Sato, Isao
Murayama, Shosaku
Arai, Tomoko
Herald, David
Higuchi, Arika
… (more) - Abstract:
- Abstract: We observed a stellar occultation by (3200) Phaethon, which occurred in western Japan on 2021 October 3 (UTC). This observation was requested by the DESTINY + mission team, which plans to conduct a flyby of asteroid Phaethon in 2028. Overall, this research effort contributes towards a large-scale observation campaign with a total of 72 observers observing from western Japan to southern Korea. 36 stations were established, and stellar occultation by the asteroid Phaethon was detected in 18 of them. This is the first time that this many multiple chord observations have been made for such a small asteroid (it has a diameter of 5–6 km). Observational reductions show that the apparent cross-section of Phaethon at the time of the occultation could be approximated using an ellipse with a major diameter of 6.12 ± 0.07 km and a minor diameter of 4.14 ± 0.07 km, and a position angle of 117.°4 ± 1.°5. As can be seen from the small error bars of the fitted ellipse, we have succeeded in estimating the shape and size of the asteroid with an extremely high degree of accuracy. Our observation results, together with other observations, will be used to create a 3D model of Phaethon and to improve its orbit. The instruments that we used for this observation are commonly used by many amateur astronomers in Japan for occultation observations and are not difficult to obtain. This paper describes the method and results of our observations using a CMOS camera and a GPS module, so thatAbstract: We observed a stellar occultation by (3200) Phaethon, which occurred in western Japan on 2021 October 3 (UTC). This observation was requested by the DESTINY + mission team, which plans to conduct a flyby of asteroid Phaethon in 2028. Overall, this research effort contributes towards a large-scale observation campaign with a total of 72 observers observing from western Japan to southern Korea. 36 stations were established, and stellar occultation by the asteroid Phaethon was detected in 18 of them. This is the first time that this many multiple chord observations have been made for such a small asteroid (it has a diameter of 5–6 km). Observational reductions show that the apparent cross-section of Phaethon at the time of the occultation could be approximated using an ellipse with a major diameter of 6.12 ± 0.07 km and a minor diameter of 4.14 ± 0.07 km, and a position angle of 117.°4 ± 1.°5. As can be seen from the small error bars of the fitted ellipse, we have succeeded in estimating the shape and size of the asteroid with an extremely high degree of accuracy. Our observation results, together with other observations, will be used to create a 3D model of Phaethon and to improve its orbit. The instruments that we used for this observation are commonly used by many amateur astronomers in Japan for occultation observations and are not difficult to obtain. This paper describes the method and results of our observations using a CMOS camera and a GPS module, so that many people can participate in occultation observations in the future. … (more)
- Is Part Of:
- Publications of the Astronomical Society of Japan. Volume 75:Number 1(2023)
- Journal:
- Publications of the Astronomical Society of Japan
- Issue:
- Volume 75:Number 1(2023)
- Issue Display:
- Volume 75, Issue 1 (2023)
- Year:
- 2023
- Volume:
- 75
- Issue:
- 1
- Issue Sort Value:
- 2023-0075-0001-0000
- Page Start:
- 153
- Page End:
- 168
- Publication Date:
- 2022-12-20
- Subjects:
- asteroids: individual ((3200) Phaethon) -- minor planets -- occultations -- methods: observational -- techniques: image processing -- techniques: photometric
Astronomy -- Periodicals
520.5 - Journal URLs:
- http://pasj.asj.or.jp/ ↗
http://pasj.oxfordjournals.org/ ↗
http://www.oxfordjournals.org/ ↗ - DOI:
- 10.1093/pasj/psac096 ↗
- Languages:
- English
- ISSNs:
- 0004-6264
- Deposit Type:
- Legaldeposit
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- British Library DSC - 7029.000000
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