Design of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX)

The JAXA’s Martian Moons Exploration (MMX) mission is planned to reveal the origin of Phobos and Deimos. It will remotely observe both moons and return a sample from Phobos. The nominal instruments include the TElescopic Nadir imager for GeOmOrphology (TENGOO) and Optical RadiOmeter composed of CHro...
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Autor*in:	Kameda, Shingo [verfasserIn] Ozaki, Masanobu Enya, Keigo Fuse, Ryota Kouyama, Toru Sakatani, Naoya Suzuki, Hidehiko Osada, Naoya Kato, Hiroki Miyamoto, Hideaki Yamazaki, Atsushi Nakamura, Tomoki Okamoto, Takaya Ishimaru, Takahiro Hong, Peng Ishibashi, Ko Takashima, Takeshi Ishigami, Ryoya Kuo, Cheng-Ling Abe, Shinsuke Goda, Yuya Murao, Hajime Fujishima, Saori Aoyama, Tsubasa Hagiwara, Keiji Mizumoto, Satoko Tanaka, Noriko Murakami, Kousuke Matsumoto, Miho Tanaka, Kenji Sakuta, Hironobu

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2021

Schlagwörter:	MMX TENGOO OROCHI Imager Phobos Deimos Mars

Anmerkung:	© The Author(s) 2021

Übergeordnetes Werk:	Enthalten in: Earth, planets and space - Heidelberg : Springer, 1998, 73(2021), 1 vom: 14. Dez.
Übergeordnetes Werk:	volume:73 ; year:2021 ; number:1 ; day:14 ; month:12

Links:	Volltext

DOI / URN:	10.1186/s40623-021-01462-9

Katalog-ID:	SPR045792917

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Indexfelder

author_variant	s k sk m o mo k e ke r f rf t k tk n s ns h s hs n o no h k hk h m hm a y ay t n tn t o to t i ti p h ph k i ki t t tt r i ri c l k clk s a sa y g yg h m hm s f sf t a ta k h kh s m sm n t nt k m km m m mm k t kt h s hs
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allfields	10.1186/s40623-021-01462-9 doi (DE-627)SPR045792917 (SPR)s40623-021-01462-9-e DE-627 ger DE-627 rakwb eng Kameda, Shingo verfasserin (orcid)0000-0001-9084-2858 aut Design of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX) 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2021 The JAXA’s Martian Moons Exploration (MMX) mission is planned to reveal the origin of Phobos and Deimos. It will remotely observe both moons and return a sample from Phobos. The nominal instruments include the TElescopic Nadir imager for GeOmOrphology (TENGOO) and Optical RadiOmeter composed of CHromatic Imagers (OROCHI). The scientific objective of TENGOO is to obtain the geomorphological features of Phobos and Deimos. The spatial resolution of TENGOO is 0.3 m at an altitude of 25 km in the quasi-satellite orbit. The scientific objective of OROCHI is to obtain material distribution using spectral mapping. OROCHI possesses seven wide-angle bandpass imagers without a filter wheel and one monochromatic imager dedicated to the observation during the landing phase. Using these two instruments, we plan to select landing sites and obtain information that supports the analysis of return samples. Graphical Abstract MMX (dpeaa)DE-He213 TENGOO (dpeaa)DE-He213 OROCHI (dpeaa)DE-He213 Imager (dpeaa)DE-He213 Phobos (dpeaa)DE-He213 Deimos (dpeaa)DE-He213 Mars (dpeaa)DE-He213 Ozaki, Masanobu aut Enya, Keigo aut Fuse, Ryota aut Kouyama, Toru aut Sakatani, Naoya aut Suzuki, Hidehiko aut Osada, Naoya aut Kato, Hiroki aut Miyamoto, Hideaki aut Yamazaki, Atsushi aut Nakamura, Tomoki aut Okamoto, Takaya aut Ishimaru, Takahiro aut Hong, Peng aut Ishibashi, Ko aut Takashima, Takeshi aut Ishigami, Ryoya aut Kuo, Cheng-Ling aut Abe, Shinsuke aut Goda, Yuya aut Murao, Hajime aut Fujishima, Saori aut Aoyama, Tsubasa aut Hagiwara, Keiji aut Mizumoto, Satoko aut Tanaka, Noriko aut Murakami, Kousuke aut Matsumoto, Miho aut Tanaka, Kenji aut Sakuta, Hironobu aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 73(2021), 1 vom: 14. Dez. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:73 year:2021 number:1 day:14 month:12 https://dx.doi.org/10.1186/s40623-021-01462-9 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 73 2021 1 14 12
spelling	10.1186/s40623-021-01462-9 doi (DE-627)SPR045792917 (SPR)s40623-021-01462-9-e DE-627 ger DE-627 rakwb eng Kameda, Shingo verfasserin (orcid)0000-0001-9084-2858 aut Design of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX) 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2021 The JAXA’s Martian Moons Exploration (MMX) mission is planned to reveal the origin of Phobos and Deimos. It will remotely observe both moons and return a sample from Phobos. The nominal instruments include the TElescopic Nadir imager for GeOmOrphology (TENGOO) and Optical RadiOmeter composed of CHromatic Imagers (OROCHI). The scientific objective of TENGOO is to obtain the geomorphological features of Phobos and Deimos. The spatial resolution of TENGOO is 0.3 m at an altitude of 25 km in the quasi-satellite orbit. The scientific objective of OROCHI is to obtain material distribution using spectral mapping. OROCHI possesses seven wide-angle bandpass imagers without a filter wheel and one monochromatic imager dedicated to the observation during the landing phase. Using these two instruments, we plan to select landing sites and obtain information that supports the analysis of return samples. Graphical Abstract MMX (dpeaa)DE-He213 TENGOO (dpeaa)DE-He213 OROCHI (dpeaa)DE-He213 Imager (dpeaa)DE-He213 Phobos (dpeaa)DE-He213 Deimos (dpeaa)DE-He213 Mars (dpeaa)DE-He213 Ozaki, Masanobu aut Enya, Keigo aut Fuse, Ryota aut Kouyama, Toru aut Sakatani, Naoya aut Suzuki, Hidehiko aut Osada, Naoya aut Kato, Hiroki aut Miyamoto, Hideaki aut Yamazaki, Atsushi aut Nakamura, Tomoki aut Okamoto, Takaya aut Ishimaru, Takahiro aut Hong, Peng aut Ishibashi, Ko aut Takashima, Takeshi aut Ishigami, Ryoya aut Kuo, Cheng-Ling aut Abe, Shinsuke aut Goda, Yuya aut Murao, Hajime aut Fujishima, Saori aut Aoyama, Tsubasa aut Hagiwara, Keiji aut Mizumoto, Satoko aut Tanaka, Noriko aut Murakami, Kousuke aut Matsumoto, Miho aut Tanaka, Kenji aut Sakuta, Hironobu aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 73(2021), 1 vom: 14. Dez. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:73 year:2021 number:1 day:14 month:12 https://dx.doi.org/10.1186/s40623-021-01462-9 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 73 2021 1 14 12
allfields_unstemmed	10.1186/s40623-021-01462-9 doi (DE-627)SPR045792917 (SPR)s40623-021-01462-9-e DE-627 ger DE-627 rakwb eng Kameda, Shingo verfasserin (orcid)0000-0001-9084-2858 aut Design of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX) 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2021 The JAXA’s Martian Moons Exploration (MMX) mission is planned to reveal the origin of Phobos and Deimos. It will remotely observe both moons and return a sample from Phobos. The nominal instruments include the TElescopic Nadir imager for GeOmOrphology (TENGOO) and Optical RadiOmeter composed of CHromatic Imagers (OROCHI). The scientific objective of TENGOO is to obtain the geomorphological features of Phobos and Deimos. The spatial resolution of TENGOO is 0.3 m at an altitude of 25 km in the quasi-satellite orbit. The scientific objective of OROCHI is to obtain material distribution using spectral mapping. OROCHI possesses seven wide-angle bandpass imagers without a filter wheel and one monochromatic imager dedicated to the observation during the landing phase. Using these two instruments, we plan to select landing sites and obtain information that supports the analysis of return samples. Graphical Abstract MMX (dpeaa)DE-He213 TENGOO (dpeaa)DE-He213 OROCHI (dpeaa)DE-He213 Imager (dpeaa)DE-He213 Phobos (dpeaa)DE-He213 Deimos (dpeaa)DE-He213 Mars (dpeaa)DE-He213 Ozaki, Masanobu aut Enya, Keigo aut Fuse, Ryota aut Kouyama, Toru aut Sakatani, Naoya aut Suzuki, Hidehiko aut Osada, Naoya aut Kato, Hiroki aut Miyamoto, Hideaki aut Yamazaki, Atsushi aut Nakamura, Tomoki aut Okamoto, Takaya aut Ishimaru, Takahiro aut Hong, Peng aut Ishibashi, Ko aut Takashima, Takeshi aut Ishigami, Ryoya aut Kuo, Cheng-Ling aut Abe, Shinsuke aut Goda, Yuya aut Murao, Hajime aut Fujishima, Saori aut Aoyama, Tsubasa aut Hagiwara, Keiji aut Mizumoto, Satoko aut Tanaka, Noriko aut Murakami, Kousuke aut Matsumoto, Miho aut Tanaka, Kenji aut Sakuta, Hironobu aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 73(2021), 1 vom: 14. Dez. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:73 year:2021 number:1 day:14 month:12 https://dx.doi.org/10.1186/s40623-021-01462-9 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 73 2021 1 14 12
allfieldsGer	10.1186/s40623-021-01462-9 doi (DE-627)SPR045792917 (SPR)s40623-021-01462-9-e DE-627 ger DE-627 rakwb eng Kameda, Shingo verfasserin (orcid)0000-0001-9084-2858 aut Design of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX) 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2021 The JAXA’s Martian Moons Exploration (MMX) mission is planned to reveal the origin of Phobos and Deimos. It will remotely observe both moons and return a sample from Phobos. The nominal instruments include the TElescopic Nadir imager for GeOmOrphology (TENGOO) and Optical RadiOmeter composed of CHromatic Imagers (OROCHI). The scientific objective of TENGOO is to obtain the geomorphological features of Phobos and Deimos. The spatial resolution of TENGOO is 0.3 m at an altitude of 25 km in the quasi-satellite orbit. The scientific objective of OROCHI is to obtain material distribution using spectral mapping. OROCHI possesses seven wide-angle bandpass imagers without a filter wheel and one monochromatic imager dedicated to the observation during the landing phase. Using these two instruments, we plan to select landing sites and obtain information that supports the analysis of return samples. Graphical Abstract MMX (dpeaa)DE-He213 TENGOO (dpeaa)DE-He213 OROCHI (dpeaa)DE-He213 Imager (dpeaa)DE-He213 Phobos (dpeaa)DE-He213 Deimos (dpeaa)DE-He213 Mars (dpeaa)DE-He213 Ozaki, Masanobu aut Enya, Keigo aut Fuse, Ryota aut Kouyama, Toru aut Sakatani, Naoya aut Suzuki, Hidehiko aut Osada, Naoya aut Kato, Hiroki aut Miyamoto, Hideaki aut Yamazaki, Atsushi aut Nakamura, Tomoki aut Okamoto, Takaya aut Ishimaru, Takahiro aut Hong, Peng aut Ishibashi, Ko aut Takashima, Takeshi aut Ishigami, Ryoya aut Kuo, Cheng-Ling aut Abe, Shinsuke aut Goda, Yuya aut Murao, Hajime aut Fujishima, Saori aut Aoyama, Tsubasa aut Hagiwara, Keiji aut Mizumoto, Satoko aut Tanaka, Noriko aut Murakami, Kousuke aut Matsumoto, Miho aut Tanaka, Kenji aut Sakuta, Hironobu aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 73(2021), 1 vom: 14. Dez. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:73 year:2021 number:1 day:14 month:12 https://dx.doi.org/10.1186/s40623-021-01462-9 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 73 2021 1 14 12
allfieldsSound	10.1186/s40623-021-01462-9 doi (DE-627)SPR045792917 (SPR)s40623-021-01462-9-e DE-627 ger DE-627 rakwb eng Kameda, Shingo verfasserin (orcid)0000-0001-9084-2858 aut Design of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX) 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2021 The JAXA’s Martian Moons Exploration (MMX) mission is planned to reveal the origin of Phobos and Deimos. It will remotely observe both moons and return a sample from Phobos. The nominal instruments include the TElescopic Nadir imager for GeOmOrphology (TENGOO) and Optical RadiOmeter composed of CHromatic Imagers (OROCHI). The scientific objective of TENGOO is to obtain the geomorphological features of Phobos and Deimos. The spatial resolution of TENGOO is 0.3 m at an altitude of 25 km in the quasi-satellite orbit. The scientific objective of OROCHI is to obtain material distribution using spectral mapping. OROCHI possesses seven wide-angle bandpass imagers without a filter wheel and one monochromatic imager dedicated to the observation during the landing phase. Using these two instruments, we plan to select landing sites and obtain information that supports the analysis of return samples. Graphical Abstract MMX (dpeaa)DE-He213 TENGOO (dpeaa)DE-He213 OROCHI (dpeaa)DE-He213 Imager (dpeaa)DE-He213 Phobos (dpeaa)DE-He213 Deimos (dpeaa)DE-He213 Mars (dpeaa)DE-He213 Ozaki, Masanobu aut Enya, Keigo aut Fuse, Ryota aut Kouyama, Toru aut Sakatani, Naoya aut Suzuki, Hidehiko aut Osada, Naoya aut Kato, Hiroki aut Miyamoto, Hideaki aut Yamazaki, Atsushi aut Nakamura, Tomoki aut Okamoto, Takaya aut Ishimaru, Takahiro aut Hong, Peng aut Ishibashi, Ko aut Takashima, Takeshi aut Ishigami, Ryoya aut Kuo, Cheng-Ling aut Abe, Shinsuke aut Goda, Yuya aut Murao, Hajime aut Fujishima, Saori aut Aoyama, Tsubasa aut Hagiwara, Keiji aut Mizumoto, Satoko aut Tanaka, Noriko aut Murakami, Kousuke aut Matsumoto, Miho aut Tanaka, Kenji aut Sakuta, Hironobu aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 73(2021), 1 vom: 14. Dez. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:73 year:2021 number:1 day:14 month:12 https://dx.doi.org/10.1186/s40623-021-01462-9 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 73 2021 1 14 12
language	English
source	Enthalten in Earth, planets and space 73(2021), 1 vom: 14. Dez. volume:73 year:2021 number:1 day:14 month:12
sourceStr	Enthalten in Earth, planets and space 73(2021), 1 vom: 14. Dez. volume:73 year:2021 number:1 day:14 month:12
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	MMX TENGOO OROCHI Imager Phobos Deimos Mars
isfreeaccess_bool	true
container_title	Earth, planets and space
authorswithroles_txt_mv	Kameda, Shingo @@aut@@ Ozaki, Masanobu @@aut@@ Enya, Keigo @@aut@@ Fuse, Ryota @@aut@@ Kouyama, Toru @@aut@@ Sakatani, Naoya @@aut@@ Suzuki, Hidehiko @@aut@@ Osada, Naoya @@aut@@ Kato, Hiroki @@aut@@ Miyamoto, Hideaki @@aut@@ Yamazaki, Atsushi @@aut@@ Nakamura, Tomoki @@aut@@ Okamoto, Takaya @@aut@@ Ishimaru, Takahiro @@aut@@ Hong, Peng @@aut@@ Ishibashi, Ko @@aut@@ Takashima, Takeshi @@aut@@ Ishigami, Ryoya @@aut@@ Kuo, Cheng-Ling @@aut@@ Abe, Shinsuke @@aut@@ Goda, Yuya @@aut@@ Murao, Hajime @@aut@@ Fujishima, Saori @@aut@@ Aoyama, Tsubasa @@aut@@ Hagiwara, Keiji @@aut@@ Mizumoto, Satoko @@aut@@ Tanaka, Noriko @@aut@@ Murakami, Kousuke @@aut@@ Matsumoto, Miho @@aut@@ Tanaka, Kenji @@aut@@ Sakuta, Hironobu @@aut@@
publishDateDaySort_date	2021-12-14T00:00:00Z
hierarchy_top_id	353898597
id	SPR045792917
language_de	englisch
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author	Kameda, Shingo
spellingShingle	Kameda, Shingo misc MMX misc TENGOO misc OROCHI misc Imager misc Phobos misc Deimos misc Mars Design of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX)
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topic_title	Design of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX) MMX (dpeaa)DE-He213 TENGOO (dpeaa)DE-He213 OROCHI (dpeaa)DE-He213 Imager (dpeaa)DE-He213 Phobos (dpeaa)DE-He213 Deimos (dpeaa)DE-He213 Mars (dpeaa)DE-He213
topic	misc MMX misc TENGOO misc OROCHI misc Imager misc Phobos misc Deimos misc Mars
topic_unstemmed	misc MMX misc TENGOO misc OROCHI misc Imager misc Phobos misc Deimos misc Mars
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format_facet	Elektronische Aufsätze Aufsätze Elektronische Ressource
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title	Design of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX)
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title_full	Design of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX)
author_sort	Kameda, Shingo
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author_browse	Kameda, Shingo Ozaki, Masanobu Enya, Keigo Fuse, Ryota Kouyama, Toru Sakatani, Naoya Suzuki, Hidehiko Osada, Naoya Kato, Hiroki Miyamoto, Hideaki Yamazaki, Atsushi Nakamura, Tomoki Okamoto, Takaya Ishimaru, Takahiro Hong, Peng Ishibashi, Ko Takashima, Takeshi Ishigami, Ryoya Kuo, Cheng-Ling Abe, Shinsuke Goda, Yuya Murao, Hajime Fujishima, Saori Aoyama, Tsubasa Hagiwara, Keiji Mizumoto, Satoko Tanaka, Noriko Murakami, Kousuke Matsumoto, Miho Tanaka, Kenji Sakuta, Hironobu
container_volume	73
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author-letter	Kameda, Shingo
doi_str_mv	10.1186/s40623-021-01462-9
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title_sort	design of telescopic nadir imager for geomorphology (tengoo) and observation of surface reflectance by optical chromatic imager (orochi) for the martian moons exploration (mmx)
title_auth	Design of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX)
abstract	The JAXA’s Martian Moons Exploration (MMX) mission is planned to reveal the origin of Phobos and Deimos. It will remotely observe both moons and return a sample from Phobos. The nominal instruments include the TElescopic Nadir imager for GeOmOrphology (TENGOO) and Optical RadiOmeter composed of CHromatic Imagers (OROCHI). The scientific objective of TENGOO is to obtain the geomorphological features of Phobos and Deimos. The spatial resolution of TENGOO is 0.3 m at an altitude of 25 km in the quasi-satellite orbit. The scientific objective of OROCHI is to obtain material distribution using spectral mapping. OROCHI possesses seven wide-angle bandpass imagers without a filter wheel and one monochromatic imager dedicated to the observation during the landing phase. Using these two instruments, we plan to select landing sites and obtain information that supports the analysis of return samples. Graphical Abstract © The Author(s) 2021
abstractGer	The JAXA’s Martian Moons Exploration (MMX) mission is planned to reveal the origin of Phobos and Deimos. It will remotely observe both moons and return a sample from Phobos. The nominal instruments include the TElescopic Nadir imager for GeOmOrphology (TENGOO) and Optical RadiOmeter composed of CHromatic Imagers (OROCHI). The scientific objective of TENGOO is to obtain the geomorphological features of Phobos and Deimos. The spatial resolution of TENGOO is 0.3 m at an altitude of 25 km in the quasi-satellite orbit. The scientific objective of OROCHI is to obtain material distribution using spectral mapping. OROCHI possesses seven wide-angle bandpass imagers without a filter wheel and one monochromatic imager dedicated to the observation during the landing phase. Using these two instruments, we plan to select landing sites and obtain information that supports the analysis of return samples. Graphical Abstract © The Author(s) 2021
abstract_unstemmed	The JAXA’s Martian Moons Exploration (MMX) mission is planned to reveal the origin of Phobos and Deimos. It will remotely observe both moons and return a sample from Phobos. The nominal instruments include the TElescopic Nadir imager for GeOmOrphology (TENGOO) and Optical RadiOmeter composed of CHromatic Imagers (OROCHI). The scientific objective of TENGOO is to obtain the geomorphological features of Phobos and Deimos. The spatial resolution of TENGOO is 0.3 m at an altitude of 25 km in the quasi-satellite orbit. The scientific objective of OROCHI is to obtain material distribution using spectral mapping. OROCHI possesses seven wide-angle bandpass imagers without a filter wheel and one monochromatic imager dedicated to the observation during the landing phase. Using these two instruments, we plan to select landing sites and obtain information that supports the analysis of return samples. Graphical Abstract © The Author(s) 2021
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container_issue	1
title_short	Design of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX)
url	https://dx.doi.org/10.1186/s40623-021-01462-9
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author2	Ozaki, Masanobu Enya, Keigo Fuse, Ryota Kouyama, Toru Sakatani, Naoya Suzuki, Hidehiko Osada, Naoya Kato, Hiroki Miyamoto, Hideaki Yamazaki, Atsushi Nakamura, Tomoki Okamoto, Takaya Ishimaru, Takahiro Hong, Peng Ishibashi, Ko Takashima, Takeshi Ishigami, Ryoya Kuo, Cheng-Ling Abe, Shinsuke Goda, Yuya Murao, Hajime Fujishima, Saori Aoyama, Tsubasa Hagiwara, Keiji Mizumoto, Satoko Tanaka, Noriko Murakami, Kousuke Matsumoto, Miho Tanaka, Kenji Sakuta, Hironobu
author2Str	Ozaki, Masanobu Enya, Keigo Fuse, Ryota Kouyama, Toru Sakatani, Naoya Suzuki, Hidehiko Osada, Naoya Kato, Hiroki Miyamoto, Hideaki Yamazaki, Atsushi Nakamura, Tomoki Okamoto, Takaya Ishimaru, Takahiro Hong, Peng Ishibashi, Ko Takashima, Takeshi Ishigami, Ryoya Kuo, Cheng-Ling Abe, Shinsuke Goda, Yuya Murao, Hajime Fujishima, Saori Aoyama, Tsubasa Hagiwara, Keiji Mizumoto, Satoko Tanaka, Noriko Murakami, Kousuke Matsumoto, Miho Tanaka, Kenji Sakuta, Hironobu
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up_date	2024-07-03T18:19:40.163Z
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Design of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX)

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