(3200) Phaethon Polarimetry in the Negative Branch: New Evidence for the Anhydrous Nature of the DESTINY+ Target Asteroid
Authors/Creators
-
Geem, Jooyeon1
- Ishiguro, Masateru1
- Takahashi, Jun2
- Akitaya, Hiroshi3
- Kawabata, Koji S.4
- Nakaoka, Tatsuya4
- Imazawa, Ryo4
- Mori, Fumiki4
- Jin, Sunho1
- Bach, Yoonsoo P.1
- Jo, Hangbin1
- Kuroda, Daisuke5
- Hasegawa, Sunao6
- Yoshida, Fumi3
- Ishibashi, Ko3
- Sekiguchi, Tomohiko7
- Beniyama, Jin8
- Arai, Tomoko3
- Ikeda, Yuji9
- Shinnaka, Yoshiharu9
- Granvik, Mikael10
- Siltala, Lauri10
- Djupvik, Anlaug A.11
- Kasikov, Anni11
- Pinter, Viktoria11
- Knudstrup, Emil11
- 1. Seoul National University
- 2. University of Hyogo
- 3. Chiba Institute of Technology
- 4. Hiroshima University
- 5. Kyoto University
- 6. Japan Aerospace Exploration Agency
- 7. Hokkaido University of Education
- 8. The University of Tokyo
- 9. Kyoto Sangyo University
- 10. University of Helsinki
- 11. Nordic Optical Telescope
Description
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, \(\alpha=8.8-32.4^\circ\)) from 2021 October to 2022 January.
Here, we offer the polarimetric data (FITS files) taken by 1) the Hiroshima Optical and Near-InfraRed camera (HONIR; Akitaya et al. 2014) on the 1.5-m Kanata Telescope at the Higashi-Hiroshima Observatory, 2) the Wide Field Grism Spectrograph 2 (WFGS2; Kawakami et al. 2022) on the 2.0-m Nayuta telescope at the Nishi-Harima Astronomical Observatory, and 3) the Andalucia Faint Object Spectrograph and Camera (ALFOSC) with the FAPOL polarimeter on the 2.56-m Nordic Optical Telescope at the Observatorio del Roque de Los Muchachos, La Palma. All data is preprocessed (i.e., bias, dark and flat corrections are done).
Please contact Jooyeon Geem (geem@astro.snu.ac.kr) or Masateru Ishiguro (ishiguro@snu.ac.kr), if you have any questions.
Notes
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