{"@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/1362825895436507392.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1126/science.1219381"}},{"identifier":{"@type":"URI","@value":"https://www.science.org/doi/pdf/10.1126/science.1219381"}}],"dc:title":[{"@value":"Dawn at Vesta: Testing the Protoplanetary Paradigm"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>A New Dawn</jats:title>\n          <jats:p>\n            Since 17 July 2011, NASA's spacecraft Dawn has been orbiting the asteroid Vesta—the second most massive and the third largest asteroid in the solar system (see the cover).\n            <jats:bold>\n              Russell\n              <jats:italic>et al.</jats:italic>\n            </jats:bold>\n            (p.\n            <jats:related-article xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"doi\" page=\"684\" related-article-type=\"in-this-issue\" vol=\"336\" xlink:href=\"10.1126/science.1219381\">684</jats:related-article>\n            ) use Dawn's observations to confirm that Vesta is a small differentiated planetary body with an inner core, and represents a surviving proto-planet from the earliest epoch of solar system formation; Vesta is also confirmed as the source of the howardite-eucrite-diogenite (HED) meteorites.\n            <jats:bold>\n              Jaumann\n              <jats:italic>et al.</jats:italic>\n            </jats:bold>\n            (p.\n            <jats:related-article xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"doi\" page=\"687\" related-article-type=\"in-this-issue\" vol=\"336\" xlink:href=\"10.1126/science.1219122\">687</jats:related-article>\n            ) report on the asteroid's overall geometry and topography, based on global surface mapping. Vesta's surface is dominated by numerous impact craters and large troughs around the equatorial region.\n            <jats:bold>\n              Marchi\n              <jats:italic>et al.</jats:italic>\n            </jats:bold>\n            (p.\n            <jats:related-article xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"doi\" page=\"690\" related-article-type=\"in-this-issue\" vol=\"336\" xlink:href=\"10.1126/science.1218757\">690</jats:related-article>\n            ) report on Vesta's complex cratering history and constrain the age of some of its major regions based on crater counts.\n            <jats:bold>\n              Schenk\n              <jats:italic>et al.</jats:italic>\n            </jats:bold>\n            (p.\n            <jats:related-article xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"doi\" page=\"694\" related-article-type=\"in-this-issue\" vol=\"336\" xlink:href=\"10.1126/science.1223272\">694</jats:related-article>\n            ) describe two giant impact basins located at the asteroid's south pole. Both basins are young and excavated enough amounts of material to form the Vestoids—a group of asteroids with a composition similar to that of Vesta—and HED meteorites.\n            <jats:bold>\n              De Sanctis\n              <jats:italic>et al.</jats:italic>\n            </jats:bold>\n            (p.\n            <jats:related-article xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"doi\" page=\"697\" related-article-type=\"in-this-issue\" vol=\"336\" xlink:href=\"10.1126/science.1219270\">697</jats:related-article>\n            ) present the mineralogical characterization of Vesta, based on data obtained by Dawn's visual and infrared spectrometer, revealing that this asteroid underwent a complex magmatic evolution that led to a differentiated crust and mantle. The global color variations detailed by\n            <jats:bold>\n              Reddy\n              <jats:italic>et al.</jats:italic>\n            </jats:bold>\n            (p.\n            <jats:related-article xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"doi\" page=\"700\" related-article-type=\"in-this-issue\" vol=\"336\" xlink:href=\"10.1126/science.1219088\">700</jats:related-article>\n            ) are unlike those of any other asteroid observed so far and are also indicative of a preserved, differentiated proto-planet.\n          </jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380005518352718470","@type":"Researcher","foaf:name":[{"@value":"C. T. Russell"}],"jpcoar:affiliationName":[{"@value":"Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095–1567, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507404","@type":"Researcher","foaf:name":[{"@value":"C. A. Raymond"}],"jpcoar:affiliationName":[{"@value":"Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507393","@type":"Researcher","foaf:name":[{"@value":"A. Coradini"}],"jpcoar:affiliationName":[{"@value":"Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica, Rome, Italy."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507521","@type":"Researcher","foaf:name":[{"@value":"H. Y. McSween"}],"jpcoar:affiliationName":[{"@value":"Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996–1410, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507394","@type":"Researcher","foaf:name":[{"@value":"M. T. Zuber"}],"jpcoar:affiliationName":[{"@value":"Massachussetts Institute of Technology, Cambridge, MA 02139–4307, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507528","@type":"Researcher","foaf:name":[{"@value":"A. Nathues"}],"jpcoar:affiliationName":[{"@value":"Max-Planck-Institut fur Sonnensystemforschung, Katlenburg-Lindau, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507402","@type":"Researcher","foaf:name":[{"@value":"M. C. De Sanctis"}],"jpcoar:affiliationName":[{"@value":"Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica, Rome, Italy."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507533","@type":"Researcher","foaf:name":[{"@value":"R. Jaumann"}],"jpcoar:affiliationName":[{"@value":"Institute of Planetary Research, DLR, Berlin, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507398","@type":"Researcher","foaf:name":[{"@value":"A. S. Konopliv"}],"jpcoar:affiliationName":[{"@value":"Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507395","@type":"Researcher","foaf:name":[{"@value":"F. Preusker"}],"jpcoar:affiliationName":[{"@value":"Institute of Planetary Research, DLR, Berlin, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507396","@type":"Researcher","foaf:name":[{"@value":"S. W. Asmar"}],"jpcoar:affiliationName":[{"@value":"Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507527","@type":"Researcher","foaf:name":[{"@value":"R. S. Park"}],"jpcoar:affiliationName":[{"@value":"Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507529","@type":"Researcher","foaf:name":[{"@value":"R. Gaskell"}],"jpcoar:affiliationName":[{"@value":"Planetary Science Institute, Tucson, AZ 85719, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507524","@type":"Researcher","foaf:name":[{"@value":"H. U. Keller"}],"jpcoar:affiliationName":[{"@value":"Max-Planck-Institut fur Sonnensystemforschung, Katlenburg-Lindau, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507530","@type":"Researcher","foaf:name":[{"@value":"S. Mottola"}],"jpcoar:affiliationName":[{"@value":"Institute of Planetary Research, DLR, Berlin, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507534","@type":"Researcher","foaf:name":[{"@value":"T. Roatsch"}],"jpcoar:affiliationName":[{"@value":"Institute of Planetary Research, DLR, Berlin, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507397","@type":"Researcher","foaf:name":[{"@value":"J. E. C. Scully"}],"jpcoar:affiliationName":[{"@value":"Department of Earth and Space Sciences, University of California, Los Angeles, CA 90095–1567, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507522","@type":"Researcher","foaf:name":[{"@value":"D. E. Smith"}],"jpcoar:affiliationName":[{"@value":"Massachussetts Institute of Technology, Cambridge, MA 02139–4307, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507532","@type":"Researcher","foaf:name":[{"@value":"P. Tricarico"}],"jpcoar:affiliationName":[{"@value":"Planetary Science Institute, Tucson, AZ 85719, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507525","@type":"Researcher","foaf:name":[{"@value":"M. J. Toplis"}],"jpcoar:affiliationName":[{"@value":"Institut de Recherche en Astrophysique et Planetologie, Université de Toulouse, France."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507526","@type":"Researcher","foaf:name":[{"@value":"U. R. Christensen"}],"jpcoar:affiliationName":[{"@value":"Max-Planck-Institut fur Sonnensystemforschung, Katlenburg-Lindau, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895436507401","@type":"Researcher","foaf:name":[{"@value":"W. C. 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