Spectral Type and Geometric Albedo of (98943) 2001 CC21, the Hayabusa2# Mission Target
Creators
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Geem, Jooyeon1
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Ishiguro, Masateru1
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Granvik, Mikael2
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Naito, Hiroyuki3
- Akitaya, Hiroshi4
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Sekiguch, Tomohiko5
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Hasegawa, Sunao6
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Kuroda, Daisuke7
- Oono, Tatsuharu8
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Bach, Yoonsoo P.1
- Jin, Sunho1
- Imazawa, Ryo9
- Kawabata, Koji S.9
- Takagi, Seiko8
- Yoshikawa, Makoto7
- Djupvik, Anlaug A.10
- Gadeberg, Julie Thiim10
- Pursimo, Tapio10
- Pedros, Oliver Durfeldt10
- Thomsen, Jeppe Sinkbaek10
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Gray, Zuri10
- 1. Seoul National University
- 2. University of Helsinki
- 3. Nayoro Observatory
- 4. Chiba Institute of Technology
- 5. Hokkaido University of Education
- 6. Japan Aerospace Exploration Agency
- 7. Japan Spaceguard Association
- 8. Hokkaido University
- 9. Hiroshima University
- 10. Nordic Optical Telescope
Description
We conducted optical polarimetry and near-infrared spectroscopy of JAXA's Hayabusa2# mission target, (98943) 2001 CC21, in early 2023. Our new observations indicate that this asteroid has a polarimetric inversion angle of ~20\(^\circ\), absorption bands around 0.9 and 1.9 \(\mu\)m, and a geometric albedo of 0.23\(\pm\)0.04. All these features are consistent with those of S-types but inconsistent with L-types. Based on this evidence, we conclude that JAXA's Hayabusa2# spacecraft will explore an S-type asteroid (more specifically, an L or LL chondrite-like object) with albedo and size (0.44-0.53 km when we assume the absolute magnitude of 18.8) similar to (25143) Itokawa.
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Description
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This ‘data’ directory contains the polarimetric and spectroscopic data of 2001 CC21
used to derive the results in Geem et al. MNRAS Letter 2023
(https://doi.org/10.48550/arXiv.2304.02917).
See the published papers by Geem et al. (MNRAS Letter 2023)
If you need any questions, please contact Jooyeon Geem via her mail (ksky0422@snu.ac.kr).
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Directory tree structure
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/data
├──/polarimetry
│ └──/Instrument (FAPOL, HONIR and, MSI)
│ └──/Observation Date
│ └──/Filter (V or R)
│ ├── *.fits (Preprocessed image in FITS format)
│ ├── mask_*.fits (Masking image in FITS format)
│ └── *.mag.1 (IRAF Phot file containing target's center info.)
│
└──/spectroscopy
└──/Observation Date (230206 and 230205)
├── obslog.txt (Observation log file)
└── *.fits (The extracted spectra using Spextool)
Files
data.zip
Files
(1.0 GB)
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