Thermal Infrared Imaging Experiments of C-Type Asteroid 162173 Ryugu on Hayabusa2

被引:0
作者
Tatsuaki Okada
Tetsuya Fukuhara
Satoshi Tanaka
Makoto Taguchi
Takeshi Imamura
Takehiko Arai
Hiroki Senshu
Yoshiko Ogawa
Hirohide Demura
Kohei Kitazato
Ryosuke Nakamura
Toru Kouyama
Tomohiko Sekiguchi
Sunao Hasegawa
Tsuneo Matsunaga
Takehiko Wada
Jun Takita
Naoya Sakatani
Yamato Horikawa
Ken Endo
Jörn Helbert
Thomas G. Müller
Axel Hagermann
机构
[1] Japan Aerospace Exploration Agency,Institute of Space and Astronautical Science
[2] The University of Tokyo,Graduate School of Science
[3] Rikkyo University,Graduate School of Frontiers Sciences
[4] The University of Tokyo,Planetary Exploration Research Center
[5] Chiba Institute of Technology,Center for Advanced Information Science and Technology
[6] University of Aizu,Center for Global Environmental Research
[7] National Institute for Advanced Industrial Science and Technology,Department of Space and Astronautical Science, School of Physical Sciences
[8] Hokkaido University of Education,Institute of Planetary Research
[9] National Institute for Environmental Studies,undefined
[10] Graduate University for Advanced Studies,undefined
[11] German Aerospace Center (DLR),undefined
[12] Max-Planck Institute for Extraterrestrial Physics,undefined
[13] The Open University,undefined
来源
Space Science Reviews | 2017年 / 208卷
关键词
Thermography; Thermal inertia; Temperature; Near-Earth asteroid; Planetary exploration;
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学科分类号
摘要
The thermal infrared imager TIR onboard Hayabusa2 has been developed to investigate thermo-physical properties of C-type, near-Earth asteroid 162173 Ryugu. TIR is one of the remote science instruments on Hayabusa2 designed to understand the nature of a volatile-rich solar system small body, but it also has significant mission objectives to provide information on surface physical properties and conditions for sampling site selection as well as the assessment of safe landing operations. TIR is based on a two-dimensional uncooled micro-bolometer array inherited from the Longwave Infrared Camera LIR on Akatsuki (Fukuhara et al., 2011). TIR takes images of thermal infrared emission in 8 to 12 μm with a field of view of 16×12∘\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$16 \times 12^{\circ}$\end{document} and a spatial resolution of 0.05∘\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$0.05^{\circ}$\end{document} per pixel. TIR covers the temperature range from 150 to 460 K, including the well calibrated range from 230 to 420 K. Temperature accuracy is within 2 K or better for summed images, and the relative accuracy or noise equivalent temperature difference (NETD) at each of pixels is 0.4 K or lower for the well-calibrated temperature range. TIR takes a couple of images with shutter open and closed, the corresponding dark frame, and provides a true thermal image by dark frame subtraction. Data processing involves summation of multiple images, image processing including the StarPixel compression (Hihara et al., 2014), and transfer to the data recorder in the spacecraft digital electronics (DE). We report the scientific and mission objectives of TIR, the requirements and constraints for the instrument specifications, the designed instrumentation and the pre-flight and in-flight performances of TIR, as well as its observation plan during the Hayabusa2 mission.
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页码:255 / 286
页数:31
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