{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1360011142934340992.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1007/978-94-024-1538-4_19"}},{"identifier":{"@type":"URI","@value":"http://link.springer.com/content/pdf/10.1007/978-94-024-1538-4_19"}},{"identifier":{"@type":"DOI","@value":"10.1007/s11214-016-0263-2"}},{"identifier":{"@type":"URI","@value":"http://link.springer.com/article/10.1007/s11214-016-0263-2/fulltext.html"}},{"identifier":{"@type":"URI","@value":"http://link.springer.com/content/pdf/10.1007/s11214-016-0263-2.pdf"}},{"identifier":{"@type":"URI","@value":"http://link.springer.com/content/pdf/10.1007/s11214-016-0263-2"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"The Camera of the MASCOT Asteroid Lander on Board Hayabusa 2"}],"description":[{"notation":[{"@value":"The MASCOT Camera (MasCam) is part of the Mobile Asteroid Surface Scout (MASCOT) lander’s science payload. MASCOT has been launched to asteroid (162173) Ryugu onboard JAXA’s Hayabusa 2 asteroid sample return mission on Dec 3rd, 2014. It is scheduled to arrive at Ryugu in 2018, and return samples to Earth by 2020. MasCam was designed and built by DLR’s Institute of Planetary Research, together with Airbus-DS Germany. The scientific goals of the MasCam investigation are to provide ground truth for the orbiter’s remote sensing observations, provide context for measurements by the other lander instruments (radiometer, spectrometer and magnetometer), the orbiter sampling experiment, and characterize the geological context, compositional variations and physical properties of the surface (e.g. rock and regolith particle size distributions). During daytime, clear filter images will be acquired. During night, illumination of the dark surface is performed by an LED array, equipped with                                                                                                                                   $4\\times36$                  monochromatic light-emitting diodes (LEDs) working in four spectral bands. Color imaging will allow the identification of spectrally distinct surface units. Continued imaging during the surface mission phase and the acquisition of image series at different sun angles over the course of an asteroid day will contribute to the physical characterization of the surface and also allow the investigation of time-dependent processes and to determine the photometric properties of the regolith. The MasCam observations, combined with the MASCOT hyperspectral microscope (MMEGA) and radiometer (MARA) thermal observations, will cover a wide range of observational scales and serve as a strong tie point between Hayabusa 2’s remote-sensing scales (                                                                                                                                   $10^{3}$                 –                                                                                                                                   $10^{-3}\\mbox{ m}$                 ) and sample scales (                                                                                                                                   $10^{-3}$                 –                                                                                                                                   $10^{-6}\\mbox{ m}$                 ). The descent sequence and the close-up images will reveal the surface features over a broad range of scales, allowing an assessment of the surface’s diversity and close the gap between the orbital observations and those made by the in-situ measurements. The MasCam is mounted inside the lander slightly tilted, such that the center of its 54.8° square field-of-view is directed towards the surface at an angle of 22° with respect to the surface plane. This is to ensure that both the surface close to the lander and the horizon are observable. The camera optics is designed according to the Scheimpflug principle, thus that the entire scene along the camera’s depth of field (150 mm to infinity) is in focus. The camera utilizes a                                                                                                                                   $1024\\times1024$                  pixel CMOS sensor sensitive in the 400–1000 nm wavelength range, peaking at 600–700 nm. Together with the f-16 optics, this yields a nominal ground resolution of 150 micron/px at 150 mm distance (diffraction limited). The camera flight model has undergone standard radiometric and geometric calibration both at the component and system (lander) level. MasCam relies on the use of wavelet compression to maximize data return within stringent mission downlink limits. All calibration and flight data products will be generated and archived in the Planetary Data System in PDS image format."}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004236854307971","@type":"Researcher","foaf:name":[{"@value":"R. Jaumann"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340868","@type":"Researcher","foaf:name":[{"@value":"N. Schmitz"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340872","@type":"Researcher","foaf:name":[{"@value":"A. Koncz"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340995","@type":"Researcher","foaf:name":[{"@value":"H. Michaelis"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340873","@type":"Researcher","foaf:name":[{"@value":"S. E. Schroeder"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340992","@type":"Researcher","foaf:name":[{"@value":"S. Mottola"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340998","@type":"Researcher","foaf:name":[{"@value":"F. Trauthan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340878","@type":"Researcher","foaf:name":[{"@value":"H. Hoffmann"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340879","@type":"Researcher","foaf:name":[{"@value":"T. Roatsch"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340884","@type":"Researcher","foaf:name":[{"@value":"D. Jobs"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340871","@type":"Researcher","foaf:name":[{"@value":"J. Kachlicki"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340865","@type":"Researcher","foaf:name":[{"@value":"B. Pforte"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340870","@type":"Researcher","foaf:name":[{"@value":"R. Terzer"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340877","@type":"Researcher","foaf:name":[{"@value":"M. Tschentscher"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340999","@type":"Researcher","foaf:name":[{"@value":"S. Weisse"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340875","@type":"Researcher","foaf:name":[{"@value":"U. Mueller"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340866","@type":"Researcher","foaf:name":[{"@value":"L. Perez-Prieto"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340876","@type":"Researcher","foaf:name":[{"@value":"B. Broll"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340867","@type":"Researcher","foaf:name":[{"@value":"A. Kruselburger"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340880","@type":"Researcher","foaf:name":[{"@value":"T.-M. Ho"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340993","@type":"Researcher","foaf:name":[{"@value":"J. Biele"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340996","@type":"Researcher","foaf:name":[{"@value":"S. Ulamec"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340874","@type":"Researcher","foaf:name":[{"@value":"C. Krause"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340997","@type":"Researcher","foaf:name":[{"@value":"M. Grott"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340881","@type":"Researcher","foaf:name":[{"@value":"J.-P. Bibring"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340864","@type":"Researcher","foaf:name":[{"@value":"S. Watanabe"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340883","@type":"Researcher","foaf:name":[{"@value":"S. Sugita"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340994","@type":"Researcher","foaf:name":[{"@value":"T. Okada"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340882","@type":"Researcher","foaf:name":[{"@value":"M. Yoshikawa"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142934340885","@type":"Researcher","foaf:name":[{"@value":"H. Yabuta"}]}],"publication":{"publicationIdentifier":[{"@type":"ISBN","@value":"9789402415377"},{"@type":"ISBN","@value":"9789402415384"},{"@type":"PISSN","@value":"00386308"},{"@type":"EISSN","@value":"15729672"}],"prism:publicationName":[{"@value":"Hayabusa2"}],"dc:publisher":[{"@value":"Springer Netherlands"}],"prism:publicationDate":"2016","prism:volume":"208","prism:number":"1-4","prism:startingPage":"375","prism:endingPage":"400"},"reviewed":"false","dc:rights":["http://www.springer.com/tdm"],"url":[{"@id":"http://link.springer.com/content/pdf/10.1007/978-94-024-1538-4_19"},{"@id":"http://link.springer.com/article/10.1007/s11214-016-0263-2/fulltext.html"},{"@id":"http://link.springer.com/content/pdf/10.1007/s11214-016-0263-2.pdf"},{"@id":"http://link.springer.com/content/pdf/10.1007/s11214-016-0263-2"}],"createdAt":"2018-08-27","modifiedAt":"2022-08-30","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=Hayabusa%202","dc:title":"Hayabusa 2"},{"@id":"https://cir.nii.ac.jp/all?q=Asteroiden%20und%20Kometen","dc:title":"Asteroiden und Kometen"},{"@id":"https://cir.nii.ac.jp/all?q=Asteroid%20Lander","dc:title":"Asteroid Lander"},{"@id":"https://cir.nii.ac.jp/all?q=Institut%20f%C3%BCr%20Planetenforschung","dc:title":"Institut für Planetenforschung"},{"@id":"https://cir.nii.ac.jp/all?q=Systementwicklung%20und%20Projektb%C3%BCro","dc:title":"Systementwicklung und Projektbüro"},{"@id":"https://cir.nii.ac.jp/all?q=Nutzerzentrum%20f%C3%BCr%20Weltraumexperimente%20(MUSC)","dc:title":"Nutzerzentrum für Weltraumexperimente (MUSC)"},{"@id":"https://cir.nii.ac.jp/all?q=Planetengeologie","dc:title":"Planetengeologie"},{"@id":"https://cir.nii.ac.jp/all?q=Planetenphysik","dc:title":"Planetenphysik"},{"@id":"https://cir.nii.ac.jp/all?q=Planetare%20Sensorsysteme","dc:title":"Planetare Sensorsysteme"},{"@id":"https://cir.nii.ac.jp/all?q=Mascot","dc:title":"Mascot"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040282256936477440","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17H06459"},{"@type":"JGN","@value":"JP17H06459"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PLANNED-17H06459/"}],"notation":[{"@language":"ja","@value":"水惑星学創成に向けた太陽系探査"},{"@language":"en","@value":"Solar System Exploration for Aqua-planetology"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050012570393147008","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Asteroid Ryugu before the Hayabusa2 encounter"},{"@value":"International regolith science group (IRSG) in Hayabusa2 project, asteroid ryugu before the hayabusa2 encounter"}]},{"@id":"https://cir.nii.ac.jp/crid/1050845763736009600","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Hayabusa2 Mission Overview"}]},{"@id":"https://cir.nii.ac.jp/crid/1050856995322809088","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Effects of dust layers on thermal emission from airless bodies"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004231938765696","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Hayabusa2-Ryugu proximity operation planning and landing site selection"}]},{"@id":"https://cir.nii.ac.jp/crid/1360005518594412672","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The descent and bouncing path of the Hayabusa2 lander MASCOT at asteroid (162173) Ryugu"}]},{"@id":"https://cir.nii.ac.jp/crid/1360009142567432448","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Spectrophotometric Analysis of the Ryugu Rock Seen by MASCOT: Searching for a Carbonaceous Chondrite Analog"}]},{"@id":"https://cir.nii.ac.jp/crid/1360009581503733120","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Preliminary analysis of the Hayabusa2 samples returned from C-type asteroid Ryugu"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011142934336128","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Phase II of the Small Main-Belt Asteroid Spectroscopic Survey The Observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011142934668928","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Thermo-physical properties of 162173 (1999 JU3), a potential flyby and rendezvous target for interplanetary missions"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011142935641728","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Rubble-Pile Asteroid Itokawa as Observed by Hayabusa"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011142937637376","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The MASCOT Magnetometer"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011142938000640","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"SPECTRAL CHARACTERISTICS OF HAYABUSA 2 NEAR-EARTH ASTEROID TARGETS 162173 1999 JU3 AND 2001 QC34"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011142938925184","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Near-Infrared Spectral Results of Asteroid Itokawa from the Hayabusa Spacecraft"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011142940079232","@type":"Article","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The MASCOT Radiometer MARA for the Hayabusa 2 Mission"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285710933540736","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Hayabusa2 arrives at the carbonaceous asteroid 162173 Ryugu—A spinning top–shaped rubble pile"}]},{"@id":"https://cir.nii.ac.jp/crid/1360288370532341248","@type":"Article","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The MicrOmega Investigation Onboard Hayabusa2"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292617911905024","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Rolis Experiment on the Rosetta Lander"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292617913117184","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Albedo, Size, and Surface Characteristics of Hayabusa-2 Sample-Return Target 162173 1999 JU3 from AKARI and Subaru Observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292617913527296","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Phase II of the Small Main-Belt Asteroid Spectroscopic Survey A Feature-Based Taxonomy"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292617917120384","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE ORIGIN OF ASTEROID 162173 (1999 JU<sub>3</sub>)"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643708395008","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Spectral and Petrographic Properties of Inclusions in Carbonaceous Chondrites and Comparison with In Situ Images from Asteroid Ryugu"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298754831415040","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"MASCOT’s in situ analysis of asteroid Ryugu in the context of regolith samples and remote sensing data returned by Hayabusa2"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298755600588160","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"MASCOT—A Mobile Lander On-board the Hayabusa2 Spacecraft—Operations on Ryugu"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565165385799936","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"MASCOT—The Mobile Asteroid Surface Scout Onboard the Hayabusa2 Mission"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567182418934272","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Science exploration and instrumentation of the OKEANOS mission to a Jupiter Trojan asteroid using the solar power sail"}]},{"@id":"https://cir.nii.ac.jp/crid/1360568468547834496","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The Hayabusa2 lander MASCOT on the surface of asteroid (162173) Ryugu – Stereo-photogrammetric analysis of MASCam image data"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574092886085376","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Landing on small bodies: From the Rosetta Lander to MASCOT and beyond"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574092886361216","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Optical observations of NEA 162173 (1999 JU3) during the 2011-2012 apparition"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574092887240832","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Rotational spectra of (162173) 1999 JU3, the target of the Hayabusa2 mission"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574092890831232","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Physical Properties of Near-Earth Objects"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118700349824","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Numerical modeling of lander interaction with a low-gravity asteroid regolith surface"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576120878550912","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The MASCOT lander aboard Hayabusa2: The in-situ exploration of NEA (162173) Ryugu"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580229783308416","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Characterization of the MASCOT landing area by Hayabusa2"}]},{"@id":"https://cir.nii.ac.jp/crid/1360853567712223744","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Surface roughness of asteroid (162173) Ryugu and comet 67P/Churyumov–Gerasimenko inferred from<i>in situ</i>observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855567868593152","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Spectral Properties of Near-Earth Objects: Palomar and IRTF Results for 48 Objects Including Spacecraft Targets (9969) Braille and (10302) 1989 ML"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855567869705856","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Spitzer observations of spacecraft target 162173 (1999 JU3)"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855567869860864","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Detailed Images of Asteroid 25143 Itokawa from Hayabusa"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593676475136","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Hayabusa2 extended mission: New voyage to rendezvous with a small asteroid rotating with a short period"}]},{"@id":"https://cir.nii.ac.jp/crid/1361131420873645312","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Images from the surface of asteroid Ryugu show rocks similar to carbonaceous chondrite meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1390282679531397888","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Hayabusa2: Scientific importance of samples returned from C-type near-Earth asteroid (162173) 1999 JU<sub>3</sub>"},{"@value":"Hayabusa2 : Scientific importance of samples returned from C-type near-Earth asteroid (162173) 1999 JU₃"},{"@value":"Hayabusa2: Scientific importance of samples returned from near-Earth C-type asteroid 1999 JU3"},{"@value":"Hayabusa2: scientific importance of samples 1027 returned from C-type near-Earth asteroid (162173) 1999 JU3"}]},{"@id":"https://cir.nii.ac.jp/crid/1460288370504919424","@type":"Dataset","resourceType":"データセット(Dataset)","relationType":["isPartOf","isRelatedTo"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Hayabusa2 Mission Bundle: Document Collection"}]},{"@id":"https://cir.nii.ac.jp/crid/2120026414383529728","@type":"OtherWorks","resourceType":"学術雑誌論文(journal article)","relationType":["isIdenticalTo"],"jpcoar:relatedTitle":[{"@language":"en","@value":"The Camera of the MASCOT Asteroid Lander on Board Hayabusa 2"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1007/978-94-024-1538-4_19"},{"@type":"CROSSREF","@value":"10.1007/s11214-016-0263-2"},{"@type":"KAKEN","@value":"PRODUCT-22518249"},{"@type":"OPENAIRE","@value":"doi_dedup___::f65aa461ebdb6688e1e60b20e0dc5f7d"},{"@type":"JALC","@value":"oai:japanlinkcenter.org:2008499193_hasPart_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"IRDB","@value":"oai:irdb.nii.ac.jp:01332:0004477198_isIdenticalTo_DOI_SCE7EVeBMB63XtOsHLFT8UfDhBr"},{"@type":"CROSSREF","@value":"10.1186/s40645-018-0237-y_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/201936757_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1186/s40645-019-0291-0_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.3847/psj/abbb97_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1038/s41550-021-01550-6_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1007/s11214-017-0377-1_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1126/science.aav8032_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1007/s11214-017-0335-y_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1126/science.aaw8627_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.3847/psj/ac034b_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1186/s40623-023-01805-8_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1007/978-3-030-94628-9_25_references_DOI_OBFu7x27pVXdoezVcjvWuzdFyJP"},{"@type":"CROSSREF","@value":"10.1016/j.pss.2021.105200_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1007/s11214-016-0251-6_references_DOI_OBFu7x27pVXdoezVcjvWuzdFyJP"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/201936760_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1007/s11214-016-0272-1_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/201936128_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/202244059_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1016/j.actaastro.2018.05.032_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1093/mnras/staa3314_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1016/j.asr.2021.03.030_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"},{"@type":"CROSSREF","@value":"10.1016/j.pss.2018.06.020_references_DOI_Pqd5Vwt3BTECX9UuRjtZATVrcBH"}]}