{"@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/1360004239674689792.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.3847/1538-4357/aaa23e"}},{"identifier":{"@type":"URI","@value":"http://stacks.iop.org/0004-637X/853/i=2/a=118/pdf"}},{"identifier":{"@type":"URI","@value":"http://stacks.iop.org/0004-637X/853/i=2/a=118?key=crossref.cb970045f0430f3036683fcd1d26dbbd"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/1538-4357/aaa23e"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/1538-4357/aaa23e/pdf"}},{"identifier":{"@type":"DOI","@value":"10.48550/arxiv.1712.05154"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"On the Impact Origin of Phobos and Deimos. III. Resulting Composition from Different Impactors"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title>\n               <jats:p>The origin of Phobos and Deimos in a giant impact-generated disk is gaining larger attention. Although this scenario has been the subject of many studies, an evaluation of the chemical composition of the Mars’s moons in this framework is missing. The chemical composition of Phobos and Deimos is unconstrained. The large uncertainties about the origin of the mid-infrared features; the lack of absorption bands in the visible and near-infrared spectra; and the effects of secondary processes on the moons’ surfaces make the determination of their composition very difficult using remote sensing data. Simulations suggest a formation of a disk made of gas and melt with their composition linked to the nature of the impactor and Mars. Using thermodynamic equilibrium, we investigate the composition of dust (condensates from gas) and solids (from a cooling melt) that result from different types of Mars impactors (Mars-, CI-, CV-, EH-, and comet-like). Our calculations show a wide range of possible chemical compositions and noticeable differences between dust and solids, depending on the considered impactors. Assuming that Phobos and Deimos resulted from the accretion and mixing of dust and solids, we find that the derived assemblage (dust-rich in metallic iron, sulfides and/or carbon, and quenched solids rich in silicates) can be compatible with the observations. The JAXA’s Martian Moons eXploration (MMX) mission will investigate the physical and chemical properties of Phobos and Deimos, especially sampling from Phobos, before returning to Earth. Our results could be then used to disentangle the origin and chemical composition of the pristine body that hit Mars and suggest guidelines for helping in the analysis of the returned samples.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004239674689795","@type":"Researcher","foaf:name":[{"@value":"Francesco C. Pignatale"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004239674689664","@type":"Researcher","foaf:name":[{"@value":"Sébastien Charnoz"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004239674689668","@type":"Researcher","foaf:name":[{"@value":"Pascal Rosenblatt"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004239674689669","@type":"Researcher","foaf:name":[{"@value":"Ryuki Hyodo"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004239674689797","@type":"Researcher","foaf:name":[{"@value":"Tomoki Nakamura"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004239674689665","@type":"Researcher","foaf:name":[{"@value":"Hidenori Genda"}]}],"contributor":[{"@id":"https://cir.nii.ac.jp/crid/1890583642969262721","@type":"Researcher","foaf:name":[{"@value":"Université Paris Diderot - Paris 7 (UPD7)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890583642969262729","@type":"Researcher","foaf:name":[{"@value":"Institut de Physique du Globe de Paris (IPGP (UMR_7154)) ; Institut national des sciences de l'Univers (INSU - CNRS)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890583642969262731","@type":"Researcher","foaf:name":[{"@value":"Earth-Life Science Institute [Tokyo] (ELSI) ; Tokyo Institute of Technology [Tokyo] (TITECH)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890583642969262850","@type":"Researcher","foaf:name":[{"@value":"Belgian PRODEX programme    Belgian Federal Science Policy Office   JSPS-MAEDI bilateral joint research project (SAKURA program)    Ministry of Education, Culture, Sports, Science and Technology, Japan (MEXT)  Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research (KAKENHI)  JP17H02990 JP17H06457"}]},{"@id":"https://cir.nii.ac.jp/crid/1891710641041704962","@type":"Researcher","foaf:name":[{"@value":"Institut de Physique du Globe de Paris (IPGP (UMR_7154))"}]},{"@id":"https://cir.nii.ac.jp/crid/1891710641041704961","@type":"Researcher","foaf:name":[{"@value":"Institut national des sciences de l'Univers (INSU - CNRS)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)"}]},{"@id":"https://cir.nii.ac.jp/crid/1891710641041704965","@type":"Researcher","foaf:name":[{"@value":"Royal Observatory of Belgium Brussels (ROB)"}]},{"@id":"https://cir.nii.ac.jp/crid/1891710641041704963","@type":"Researcher","foaf:name":[{"@value":"Tokyo Institute of Technology Tokyo (TITECH)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890583642969262733","@type":"Researcher","foaf:name":[{"@value":"Belgian PRODEX programme Belgian Federal Science Policy Office JSPS-MAEDI bilateral joint research project (SAKURA program) Ministry of Education, Culture, Sports, Science and Technology, Japan (MEXT) Japan Society for the Promotion of Science Grants-in-Aid for Scientific Research (KAKENHI) JP17H02990 JP17H06457"}]},{"@id":"https://cir.nii.ac.jp/crid/1890583642969262725","@type":"Researcher","foaf:name":[{"@value":"Commissariat à l'énergie atomique et aux énergies alternatives (CEA)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890583642969262732","@type":"Researcher","foaf:name":[{"@value":"Royal Observatory of Belgium = Observatoire Royal de Belgique (ROB)"}]},{"@id":"https://cir.nii.ac.jp/crid/1891710641041704964","@type":"Researcher","foaf:name":[{"@value":"Tohoku University Sendai"}]},{"@id":"https://cir.nii.ac.jp/crid/1891710641041704960","@type":"Researcher","foaf:name":[{"@value":"Earth-Life Science Institute Tokyo (ELSI)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890583642969262724","@type":"Researcher","foaf:name":[{"@value":"Institut de Physique du Globe de Paris (IPGP) ; Institut national des sciences de l'Univers (INSU - CNRS)-IPG PARIS-Université de La Réunion (UR)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890583642969262730","@type":"Researcher","foaf:name":[{"@value":"Analytic and Computational Research, Inc. - Earth Sciences (ACRI-ST)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890583642969262722","@type":"Researcher","foaf:name":[{"@value":"ANR-10-LABX-0023,UnivEarthS,Earth - Planets - Universe: observation, modeling, transfer(2010)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890583642969262852","@type":"Researcher","foaf:name":[{"@value":"Tohoku University [Sendai]"}]},{"@id":"https://cir.nii.ac.jp/crid/1890583642969262728","@type":"Researcher","foaf:name":[{"@value":"Royal Observatory of Belgium [Brussels] (ROB)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890583642969262726","@type":"Researcher","foaf:name":[{"@value":"ANR-11-IDEX-0005,USPC,Université Sorbonne Paris Cité(2011)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890583642969262720","@type":"Researcher","foaf:name":[{"@value":"Tokyo Institute of Technology [Tokyo] (TITECH)"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"0004637X"},{"@type":"EISSN","@value":"15384357"}],"prism:publicationName":[{"@value":"The Astrophysical Journal"}],"dc:publisher":[{"@value":"American Astronomical Society"}],"prism:publicationDate":"2018-01-30","prism:volume":"853","prism:number":"2","prism:startingPage":"118"},"reviewed":"false","dc:rights":["https://iopscience.iop.org/page/copyright","https://iopscience.iop.org/info/page/text-and-data-mining"],"url":[{"@id":"http://stacks.iop.org/0004-637X/853/i=2/a=118/pdf"},{"@id":"http://stacks.iop.org/0004-637X/853/i=2/a=118?key=crossref.cb970045f0430f3036683fcd1d26dbbd"},{"@id":"https://iopscience.iop.org/article/10.3847/1538-4357/aaa23e"},{"@id":"https://iopscience.iop.org/article/10.3847/1538-4357/aaa23e/pdf"}],"createdAt":"2018-01-30","modifiedAt":"2024-01-10","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=Earth%20and%20Planetary%20Astrophysics%20(astro-ph.EP)","dc:title":"Earth and Planetary Astrophysics (astro-ph.EP)"},{"@id":"https://cir.nii.ac.jp/all?q=%5BSDU.ASTR%5DSciences%20of%20the%20Universe%20%5Bphysics%5D/Astrophysics%20%5Bastro-ph%5D","dc:title":"[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]"},{"@id":"https://cir.nii.ac.jp/all?q=planets%20and%20satellites:%20individual%20(Phobos%20Deimos)","dc:title":"planets and satellites: individual (Phobos Deimos)"},{"@id":"https://cir.nii.ac.jp/all?q=planets%20and%20satellites:%20composition","dc:title":"planets and satellites: composition"},{"@id":"https://cir.nii.ac.jp/all?q=planets%20and%20satellites:%20formation","dc:title":"planets and satellites: formation"},{"@id":"https://cir.nii.ac.jp/all?q=FOS:%20Physical%20sciences","dc:title":"FOS: Physical sciences"},{"@id":"https://cir.nii.ac.jp/all?q=520","dc:title":"520"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Earth%20and%20Planetary%20Astrophysics","dc:title":"Astrophysics - Earth and Planetary Astrophysics"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040000781956268416","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17H02990"},{"@type":"JGN","@value":"JP17H02990"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-17H02990/"}],"notation":[{"@language":"ja","@value":"衝突剥離過程の解明：天体衝突による惑星間物質輸送への応用"},{"@language":"en","@value":"Study on impact spallation: Material transfer between planetary bodies by impacts"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000781959777024","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17H06457"},{"@type":"JGN","@value":"JP17H06457"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PLANNED-17H06457/"}],"notation":[{"@language":"ja","@value":"太陽系天体における水・物質循環のモデリング"},{"@language":"en","@value":"Modeling of water and material circulations in the solar system objects"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282256932958592","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17H02975"},{"@type":"JGN","@value":"JP17H02975"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-17H02975/"}],"notation":[{"@language":"ja","@value":"溶融宇宙塵から復元する大気酸素同位体比と生物生産の変動"},{"@language":"en","@value":"Reconstruction of atmospheric oxygen isotope composition using ancient cosmic spherules"}]},{"@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"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282256937329792","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17J01269"},{"@type":"JGN","@value":"JP17J01269"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-17J01269/"}],"notation":[{"@language":"ja","@value":"多様なリング－衛星系の起源・進化の統一的理解に向けた理論研究"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360002220784820864","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"On the Impact Origin of Phobos and Deimos. I. Thermodynamic and Physical Aspects"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004232135523968","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The cool and distant formation of Mars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004239675372544","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"On the Impact Origin of Phobos and Deimos. IV. Volatile Depletion"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144519675520","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Condensation of CaOMgOAl2O3SiO2 liquids from cosmic gases"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144531208448","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Quantitative Chemico-Mineralogical Classification and Nomenclature of Igneous Rocks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145046682624","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The effect of the regular solution model in the condensation of protoplanetary dust"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145591342208","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Chemical Composition of the Sun"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011146074346496","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Color heterogeneity of the surface of Phobos: Relationships to geologic features and comparison to meteorite analogs"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021389828694912","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Optimizing Image Compression Ratio for Generating Highly Accurate Local Digital Terrain Models: Experimental Study for Martian Moons eXploration Mission"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283691784003712","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Accretion of Phobos and Deimos in an extended debris disc stirred by transient moons"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620217975040","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Reproduction of chondrules from levitated, hypercooled melts"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306906082988288","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Spectro-photometry of Phobos simulants"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565165902965760","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Formation of Phobos and Deimos via a giant impact"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567189627944704","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"On the Impact Origin of Phobos and Deimos. II. True Polar Wander and Disk Evolution"}]},{"@id":"https://cir.nii.ac.jp/crid/1360568468126136832","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Measuring the Elemental Composition of Phobos: The Mars‐moon Exploration with GAmma rays and NEutrons (MEGANE) Investigation for the Martian Moons eXploration (MMX) Mission"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574093972969856","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Compositions of chondrites"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574094326769152","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"RECONCILING THE ORBITAL AND PHYSICAL PROPERTIES OF THE MARTIAN MOONS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095140535424","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CHEMISTRY OF IMPACT-GENERATED SILICATE MELT-VAPOR DEBRIS DISKS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095443655936","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Mineralogical Applications of Crystal Field Theory"}]},{"@id":"https://cir.nii.ac.jp/crid/1360579820493876608","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Giga-year dynamical evolution of particles around Mars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584340517297536","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Mixing model of Phobos’ bulk elemental composition for the determination of its origin: Multivariate analysis of MMX/MEGANE data"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848654737971072","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A colossal impact enriched Mars' mantle with noble metals"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569084939648","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Spectroscopy of synthetic Mg‐Fe pyroxenes I: Spin‐allowed and spin‐forbidden crystal field bands in the visible and near‐infrared"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569370659840","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Are Phobos and Deimos the result of a giant impact?"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569497044480","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Solar System Abundances and Condensation Temperatures of the Elements"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569521250560","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Near‐infrared spectral reflectance of mineral mixtures: Systematic combinations of pyroxenes, olivine, and iron oxides"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569627334656","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Reflectance spectra of mafic silicate-opaque assemblages with applications to meteorite spectra"}]},{"@id":"https://cir.nii.ac.jp/crid/1360865816803777280","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Origin of Phobos and Deimos Awaiting Direct Exploration"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137043506799104","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Aqueous alteration of carbonaceous chondrites: Evidence for preaccretionary alteration—A review"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137045039596416","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"2D condensation model for the inner Solar Nebula: an enstatite-rich environment"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418520440166784","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A post-accretionary lull in large impacts on early Mars"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418521115073536","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A POSSIBLE CARBON-RICH INTERIOR IN SUPER-EARTH 55 Cancri e"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699993490819328","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Self-Perpetuating Catalyst for the Production of Complex Organic Molecules in Protostellar Nebulae"}]},{"@id":"https://cir.nii.ac.jp/crid/1361975843214532736","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Transport of impact ejecta from Mars to its moons as a means to reveal Martian history"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981469753112832","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Reflectance spectra of “featureless” materials and the surface mineralogies of M‐ and E‐class asteroids"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981470222738432","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Near-Infrared Spectrophotometry of Phobos and Deimos"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262944432296704","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Mars Pathfinder spectral measurements of Phobos and Deimos: Comparison with previous data"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262945821813248","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE COMPOSITIONAL DIVERSITY OF EXTRASOLAR TERRESTRIAL PLANETS. I. IN SITU SIMULATIONS"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544418744297728","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Origin of water in the inner Solar System: Planetesimals scattered inward during Jupiter and Saturn’s rapid gas accretion"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420024886400","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Reflectance spectra of glass-bearing mafic silicate mixtures and spectral deconvolution procedures"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420293712128","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Condensation from supernova gas made of free atoms"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420695075072","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Cometary Refractory Grains: Interstellar and Nebular Sources"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825893534304512","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The effect of ratio on the condensation of planetary material"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825893998962944","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Compositional interpretation of PFS/MEx and TES/MGS thermal infrared spectra of Phobos"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825894831755264","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"An experimental study on Fischer-Tropsch catalysis: Implications for impact phenomena and nebular chemistry"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825895846310912","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Sulfur chemistry with time-varying oxygen abundance during Solar System formation"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368965015680","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Condensation chemistry of carbon stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369259578240","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Polymers and Other Macromolecules in Comets"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369776013952","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemical Equilibrium in Complex Mixtures"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369914919296","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Mineral formation in stellar winds"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107370590247296","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A condensation model for the formation of chondrules in enstatite chondrites"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388844405884416","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The origin of the Martian moons revisited"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670320043845888","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Thermal infrared (2.5–13.5 μm) spectroscopic remote sensing of igneous rock types on particulate planetary surfaces"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951793526743552","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"An ongoing satellite–ring cycle of Mars and the origins of Phobos and Deimos"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951795087970432","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The condensation and fractionation of refractory lithophile elements"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233269600607232","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A multi‐step model for the origin of E3 (enstatite) chondrites"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233270276594304","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Reaction kinetics over iron catalysts used for the fischer‐tropsch synthesis"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233271006893184","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Metal silicate mixtures: Spectral properties and applications to asteroid taxonomy"}]},{"@id":"https://cir.nii.ac.jp/crid/1390001206545698304","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Critical cooling rates for glass formation in levitated Mg2SiO4-MgSiO3 chondrule melts"}]},{"@id":"https://cir.nii.ac.jp/crid/2051151842057867776","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Analytical protocols for Phobos regolith samples returned by the Martian Moons eXploration (MMX) mission"}]},{"@id":"https://cir.nii.ac.jp/crid/2051996266990214656","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"MIRS : an imaging spectrometer for the MMX mission"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.3847/1538-4357/aaa23e"},{"@type":"KAKEN","@value":"PRODUCT-21767494"},{"@type":"KAKEN","@value":"PRODUCT-21814914"},{"@type":"KAKEN","@value":"PRODUCT-22518187"},{"@type":"KAKEN","@value":"PRODUCT-22328509"},{"@type":"KAKEN","@value":"PRODUCT-22518241"},{"@type":"OPENAIRE","@value":"doi_dedup___::8297db0cc6b18839935308295e68127d"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/aac024_references_DOI_QU5HtULVRgRR98qb0qEswE0zpua"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01423-2_references_DOI_QU5HtULVRgRR98qb0qEswE0zpua"},{"@type":"CROSSREF","@value":"10.3390/rs15235500_references_DOI_QU5HtULVRgRR98qb0qEswE0zpua"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2024.116216_references_DOI_QU5HtULVRgRR98qb0qEswE0zpua"},{"@type":"CROSSREF","@value":"10.1029/2019ea000811_references_DOI_QU5HtULVRgRR98qb0qEswE0zpua"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01438-9_references_DOI_QU5HtULVRgRR98qb0qEswE0zpua"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2022.115335_references_DOI_QU5HtULVRgRR98qb0qEswE0zpua"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2023.115891_references_DOI_QU5HtULVRgRR98qb0qEswE0zpua"},{"@type":"CROSSREF","@value":"10.1146/annurev-earth-040522-110615_references_DOI_QU5HtULVRgRR98qb0qEswE0zpua"},{"@type":"CROSSREF","@value":"10.1038/s41598-019-56139-x_references_DOI_QU5HtULVRgRR98qb0qEswE0zpua"}]}