NIRS3: The Near Infrared Spectrometer on Hayabusa2
NIRS3: The Near Infrared Spectrometer is installed on the Hayabusa2 spacecraft to observe the target C-type asteroid 162173 Ryugu at near infrared wavelengths of 1.8 to 3.2 μm. It aims to obtain reflectance spectra in order to detect absorption bands of hydrated and hydroxide minerals in the 3 μm-ba...
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| Veröffentlicht in: | Space science reviews 2017-07, Vol.208 (1-4), p.317-337 |
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| creator | Iwata, Takahiro Kitazato, Kohei Abe, Masanao Ohtake, Makiko Arai, Takehiko Arai, Tomoko Hirata, Naru Hiroi, Takahiro Honda, Chikatoshi Imae, Naoya Komatsu, Mutsumi Matsunaga, Tsuneo Matsuoka, Moe Matsuura, Shuji Nakamura, Tomoki Nakato, Aiko Nakauchi, Yusuke Osawa, Takahito Senshu, Hiroki Takagi, Yasuhiko Tsumura, Kohji Takato, Naruhisa Watanabe, Sei-ichiro Barucci, Maria Antonietta Palomba, Ernesto Ozaki, Masanobu |
| description | NIRS3: The Near Infrared Spectrometer is installed on the Hayabusa2 spacecraft to observe the target C-type asteroid 162173 Ryugu at near infrared wavelengths of 1.8 to 3.2 μm. It aims to obtain reflectance spectra in order to detect absorption bands of hydrated and hydroxide minerals in the 3 μm-band. We adopted a linear-image sensor with indium arsenide (InAs) photo diodes and a cooling system with a passive radiator to achieve an optics temperature of 188 K (
−
85
∘
C
), which enables to retaining sufficient sensitivity and noise level in the 3 μm wavelength region. We conducted ground performance tests for the NIRS3 flight model (FM) to confirm its baseline specifications. The results imply that the properties such as the signal-to-noise ratio (SNR) conform to scientific requirements to determine the degree of aqueous alteration, such as CM or CI chondrite, and the stage of thermal metamorphism on the asteroid surface. |
| doi_str_mv | 10.1007/s11214-017-0341-0 |
| format | Article |
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−
85
∘
C
), which enables to retaining sufficient sensitivity and noise level in the 3 μm wavelength region. We conducted ground performance tests for the NIRS3 flight model (FM) to confirm its baseline specifications. The results imply that the properties such as the signal-to-noise ratio (SNR) conform to scientific requirements to determine the degree of aqueous alteration, such as CM or CI chondrite, and the stage of thermal metamorphism on the asteroid surface.</description><identifier>ISSN: 0038-6308</identifier><identifier>EISSN: 1572-9672</identifier><identifier>DOI: 10.1007/s11214-017-0341-0</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Absorption bands ; Absorption spectra ; Aerospace Technology and Astronautics ; Asteroids ; Astrophysics ; Astrophysics and Astroparticles ; Cooling systems ; Indium arsenides ; Infrared spectrometers ; Japanese spacecraft ; Metamorphism ; Minerals ; Near infrared radiation ; Noise levels ; Noise sensitivity ; Optics ; Performance tests ; Physics ; Physics and Astronomy ; Planetology ; Radiators ; Reflectance ; Signal to noise ratio ; Solar system ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Spacecraft ; Spectrum analysis ; Water transportation ; Wavelengths</subject><ispartof>Space science reviews, 2017-07, Vol.208 (1-4), p.317-337</ispartof><rights>Springer Science+Business Media Dordrecht 2017</rights><rights>Springer Science+Business Media Dordrecht 2017.</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c462t-99ab61412ce8b094ca1056a958f59628ac148a6250a332d4bd058b8cd3c4ccef3</citedby><cites>FETCH-LOGICAL-c462t-99ab61412ce8b094ca1056a958f59628ac148a6250a332d4bd058b8cd3c4ccef3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11214-017-0341-0$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11214-017-0341-0$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>230,314,776,780,881,27901,27902,41464,42533,51294</link.rule.ids><backlink>$$Uhttps://hal-obspm.ccsd.cnrs.fr/obspm-02194499$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Iwata, Takahiro</creatorcontrib><creatorcontrib>Kitazato, Kohei</creatorcontrib><creatorcontrib>Abe, Masanao</creatorcontrib><creatorcontrib>Ohtake, Makiko</creatorcontrib><creatorcontrib>Arai, Takehiko</creatorcontrib><creatorcontrib>Arai, Tomoko</creatorcontrib><creatorcontrib>Hirata, Naru</creatorcontrib><creatorcontrib>Hiroi, Takahiro</creatorcontrib><creatorcontrib>Honda, Chikatoshi</creatorcontrib><creatorcontrib>Imae, Naoya</creatorcontrib><creatorcontrib>Komatsu, Mutsumi</creatorcontrib><creatorcontrib>Matsunaga, Tsuneo</creatorcontrib><creatorcontrib>Matsuoka, Moe</creatorcontrib><creatorcontrib>Matsuura, Shuji</creatorcontrib><creatorcontrib>Nakamura, Tomoki</creatorcontrib><creatorcontrib>Nakato, Aiko</creatorcontrib><creatorcontrib>Nakauchi, Yusuke</creatorcontrib><creatorcontrib>Osawa, Takahito</creatorcontrib><creatorcontrib>Senshu, Hiroki</creatorcontrib><creatorcontrib>Takagi, Yasuhiko</creatorcontrib><creatorcontrib>Tsumura, Kohji</creatorcontrib><creatorcontrib>Takato, Naruhisa</creatorcontrib><creatorcontrib>Watanabe, Sei-ichiro</creatorcontrib><creatorcontrib>Barucci, Maria Antonietta</creatorcontrib><creatorcontrib>Palomba, Ernesto</creatorcontrib><creatorcontrib>Ozaki, Masanobu</creatorcontrib><title>NIRS3: The Near Infrared Spectrometer on Hayabusa2</title><title>Space science reviews</title><addtitle>Space Sci Rev</addtitle><description>NIRS3: The Near Infrared Spectrometer is installed on the Hayabusa2 spacecraft to observe the target C-type asteroid 162173 Ryugu at near infrared wavelengths of 1.8 to 3.2 μm. It aims to obtain reflectance spectra in order to detect absorption bands of hydrated and hydroxide minerals in the 3 μm-band. We adopted a linear-image sensor with indium arsenide (InAs) photo diodes and a cooling system with a passive radiator to achieve an optics temperature of 188 K (
−
85
∘
C
), which enables to retaining sufficient sensitivity and noise level in the 3 μm wavelength region. We conducted ground performance tests for the NIRS3 flight model (FM) to confirm its baseline specifications. The results imply that the properties such as the signal-to-noise ratio (SNR) conform to scientific requirements to determine the degree of aqueous alteration, such as CM or CI chondrite, and the stage of thermal metamorphism on the asteroid surface.</description><subject>Absorption bands</subject><subject>Absorption spectra</subject><subject>Aerospace Technology and Astronautics</subject><subject>Asteroids</subject><subject>Astrophysics</subject><subject>Astrophysics and Astroparticles</subject><subject>Cooling systems</subject><subject>Indium arsenides</subject><subject>Infrared spectrometers</subject><subject>Japanese spacecraft</subject><subject>Metamorphism</subject><subject>Minerals</subject><subject>Near infrared radiation</subject><subject>Noise levels</subject><subject>Noise sensitivity</subject><subject>Optics</subject><subject>Performance tests</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Planetology</subject><subject>Radiators</subject><subject>Reflectance</subject><subject>Signal to noise ratio</subject><subject>Solar system</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Spacecraft</subject><subject>Spectrum analysis</subject><subject>Water 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Nakamura, Tomoki ; Nakato, Aiko ; Nakauchi, Yusuke ; Osawa, Takahito ; Senshu, Hiroki ; Takagi, Yasuhiko ; Tsumura, Kohji ; Takato, Naruhisa ; Watanabe, Sei-ichiro ; Barucci, Maria Antonietta ; Palomba, Ernesto ; Ozaki, Masanobu</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c462t-99ab61412ce8b094ca1056a958f59628ac148a6250a332d4bd058b8cd3c4ccef3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Absorption bands</topic><topic>Absorption spectra</topic><topic>Aerospace Technology and Astronautics</topic><topic>Asteroids</topic><topic>Astrophysics</topic><topic>Astrophysics and Astroparticles</topic><topic>Cooling systems</topic><topic>Indium arsenides</topic><topic>Infrared spectrometers</topic><topic>Japanese spacecraft</topic><topic>Metamorphism</topic><topic>Minerals</topic><topic>Near infrared radiation</topic><topic>Noise levels</topic><topic>Noise 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Chikatoshi</au><au>Imae, Naoya</au><au>Komatsu, Mutsumi</au><au>Matsunaga, Tsuneo</au><au>Matsuoka, Moe</au><au>Matsuura, Shuji</au><au>Nakamura, Tomoki</au><au>Nakato, Aiko</au><au>Nakauchi, Yusuke</au><au>Osawa, Takahito</au><au>Senshu, Hiroki</au><au>Takagi, Yasuhiko</au><au>Tsumura, Kohji</au><au>Takato, Naruhisa</au><au>Watanabe, Sei-ichiro</au><au>Barucci, Maria Antonietta</au><au>Palomba, Ernesto</au><au>Ozaki, Masanobu</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>NIRS3: The Near Infrared Spectrometer on Hayabusa2</atitle><jtitle>Space science reviews</jtitle><stitle>Space Sci Rev</stitle><date>2017-07-01</date><risdate>2017</risdate><volume>208</volume><issue>1-4</issue><spage>317</spage><epage>337</epage><pages>317-337</pages><issn>0038-6308</issn><eissn>1572-9672</eissn><abstract>NIRS3: The Near Infrared Spectrometer is installed on the Hayabusa2 spacecraft to observe the target C-type asteroid 162173 Ryugu at near infrared wavelengths of 1.8 to 3.2 μm. It aims to obtain reflectance spectra in order to detect absorption bands of hydrated and hydroxide minerals in the 3 μm-band. We adopted a linear-image sensor with indium arsenide (InAs) photo diodes and a cooling system with a passive radiator to achieve an optics temperature of 188 K (
−
85
∘
C
), which enables to retaining sufficient sensitivity and noise level in the 3 μm wavelength region. We conducted ground performance tests for the NIRS3 flight model (FM) to confirm its baseline specifications. The results imply that the properties such as the signal-to-noise ratio (SNR) conform to scientific requirements to determine the degree of aqueous alteration, such as CM or CI chondrite, and the stage of thermal metamorphism on the asteroid surface.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s11214-017-0341-0</doi><tpages>21</tpages></addata></record> |
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| subjects | Absorption bands Absorption spectra Aerospace Technology and Astronautics Asteroids Astrophysics Astrophysics and Astroparticles Cooling systems Indium arsenides Infrared spectrometers Japanese spacecraft Metamorphism Minerals Near infrared radiation Noise levels Noise sensitivity Optics Performance tests Physics Physics and Astronomy Planetology Radiators Reflectance Signal to noise ratio Solar system Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Spacecraft Spectrum analysis Water transportation Wavelengths |
| title | NIRS3: The Near Infrared Spectrometer on Hayabusa2 |
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