{"@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/1360574092889076352.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1126/science.1219088"}},{"identifier":{"@type":"URI","@value":"https://www.science.org/doi/pdf/10.1126/science.1219088"}}],"dc:title":[{"@value":"Color and Albedo Heterogeneity of Vesta from Dawn"}],"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/1380574092889076357","@type":"Researcher","foaf:name":[{"@value":"Vishnu Reddy"}],"jpcoar:affiliationName":[{"@value":"Max Planck Institute for Solar System Research, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany."},{"@value":"Department of Space Studies, University of North Dakota, Grand Forks, ND 58202, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076361","@type":"Researcher","foaf:name":[{"@value":"Andreas Nathues"}],"jpcoar:affiliationName":[{"@value":"Max Planck Institute for Solar System Research, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076226","@type":"Researcher","foaf:name":[{"@value":"Lucille Le Corre"}],"jpcoar:affiliationName":[{"@value":"Max Planck Institute for Solar System Research, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076356","@type":"Researcher","foaf:name":[{"@value":"Holger Sierks"}],"jpcoar:affiliationName":[{"@value":"Max Planck Institute for Solar System Research, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076373","@type":"Researcher","foaf:name":[{"@value":"Jian-Yang Li"}],"jpcoar:affiliationName":[{"@value":"Department of Astronomy, University of Maryland, College Park, MD 20742, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076355","@type":"Researcher","foaf:name":[{"@value":"Robert Gaskell"}],"jpcoar:affiliationName":[{"@value":"Planetary Science Institute, 1700 East Fort Lowell, Suite 106, Tucson, AZ 85719, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076369","@type":"Researcher","foaf:name":[{"@value":"Timothy McCoy"}],"jpcoar:affiliationName":[{"@value":"Department of Mineral Sciences, Smithsonian National Museum of Natural History, 10th and Constitution NW, Washington, DC 20560–0119, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076228","@type":"Researcher","foaf:name":[{"@value":"Andrew W. Beck"}],"jpcoar:affiliationName":[{"@value":"Department of Mineral Sciences, Smithsonian National Museum of Natural History, 10th and Constitution NW, Washington, DC 20560–0119, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076353","@type":"Researcher","foaf:name":[{"@value":"Stefan E. Schröder"}],"jpcoar:affiliationName":[{"@value":"Max Planck Institute for Solar System Research, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076354","@type":"Researcher","foaf:name":[{"@value":"Carle M. Pieters"}],"jpcoar:affiliationName":[{"@value":"Department of Geological Sciences, Brown University, Providence, RI 02912, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076352","@type":"Researcher","foaf:name":[{"@value":"Kris J. Becker"}],"jpcoar:affiliationName":[{"@value":"Astrogeology Science Center, U.S. Geological Survey, Flagstaff, AZ 86001, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076366","@type":"Researcher","foaf:name":[{"@value":"Bonnie J. Buratti"}],"jpcoar:affiliationName":[{"@value":"Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076224","@type":"Researcher","foaf:name":[{"@value":"Brett Denevi"}],"jpcoar:affiliationName":[{"@value":"Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076363","@type":"Researcher","foaf:name":[{"@value":"David T. Blewett"}],"jpcoar:affiliationName":[{"@value":"Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076359","@type":"Researcher","foaf:name":[{"@value":"Ulrich Christensen"}],"jpcoar:affiliationName":[{"@value":"Max Planck Institute for Solar System Research, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076362","@type":"Researcher","foaf:name":[{"@value":"Michael J. Gaffey"}],"jpcoar:affiliationName":[{"@value":"Department of Space Studies, University of North Dakota, Grand Forks, ND 58202, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076370","@type":"Researcher","foaf:name":[{"@value":"Pablo Gutierrez-Marques"}],"jpcoar:affiliationName":[{"@value":"Max Planck Institute for Solar System Research, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076227","@type":"Researcher","foaf:name":[{"@value":"Michael Hicks"}],"jpcoar:affiliationName":[{"@value":"Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076371","@type":"Researcher","foaf:name":[{"@value":"Horst Uwe Keller"}],"jpcoar:affiliationName":[{"@value":"Institut für Geophysik und extraterrestrische Physik, TU Braunschweig Mendelssohnstrasse 3, DE 38106 Braunschweig, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076360","@type":"Researcher","foaf:name":[{"@value":"Thorsten Maue"}],"jpcoar:affiliationName":[{"@value":"Max Planck Institute for Solar System Research, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076365","@type":"Researcher","foaf:name":[{"@value":"Stefano Mottola"}],"jpcoar:affiliationName":[{"@value":"Deutsches Zentrum für Luft und Raumfahrt (DLR)–German Aerospace Center, Institute of Planetary Research, Rutherfordstrasse 2, D-12489 Berlin, Germany."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076225","@type":"Researcher","foaf:name":[{"@value":"Lucy A. McFadden"}],"jpcoar:affiliationName":[{"@value":"NASA/Goddard Space Flight Center, Mail Code 160, Greenbelt, MD 20771, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076372","@type":"Researcher","foaf:name":[{"@value":"Harry Y. McSween"}],"jpcoar:affiliationName":[{"@value":"Department of Earth and Planetary Sciences, University of Tennessee, 1412 Circle Drive, Knoxville, TN 37996–1410, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076368","@type":"Researcher","foaf:name":[{"@value":"David Mittlefehldt"}],"jpcoar:affiliationName":[{"@value":"Astromaterials Research Office, NASA Johnson Space Center, Mail Code KR, Houston, TX 77058, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076367","@type":"Researcher","foaf:name":[{"@value":"David P. O’Brien"}],"jpcoar:affiliationName":[{"@value":"Planetary Science Institute, 1700 East Fort Lowell, Suite 106, Tucson, AZ 85719, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076364","@type":"Researcher","foaf:name":[{"@value":"Carol Raymond"}],"jpcoar:affiliationName":[{"@value":"Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092889076358","@type":"Researcher","foaf:name":[{"@value":"Christopher Russell"}],"jpcoar:affiliationName":[{"@value":"Institute of Geophysics and Planetary Physics, University of California Los Angeles, Los Angeles, CA 90024–1567, USA."}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00368075"},{"@type":"EISSN","@value":"10959203"}],"prism:publicationName":[{"@value":"Science"}],"dc:publisher":[{"@value":"American Association for the Advancement of Science (AAAS)"}],"prism:publicationDate":"2012-05-11","prism:volume":"336","prism:number":"6082","prism:startingPage":"700","prism:endingPage":"704"},"reviewed":"false","url":[{"@id":"https://www.science.org/doi/pdf/10.1126/science.1219088"}],"createdAt":"2012-05-10","modifiedAt":"2024-01-10","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360009142419725184","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Characterization of D‐Type Spectra Based on Hyperspectral Remote Sensing of the Lunar Surface"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848656365527424","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Albedo Observation by Hayabusa2 LIDAR: Instrument Performance and Error Evaluation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848660727841152","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Mixing relations of the howardite‐eucrite‐diogenite suite: A new statistical approach of independent component analysis for the Dawn mission"}]},{"@id":"https://cir.nii.ac.jp/crid/2050588892108521984","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Derivation of 1.064 μm normal albedos on the C-type asteroid Ryugu from laser pulse intensity measurement of the Hayabusa2 LIDAR"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1126/science.1219088"},{"@type":"CROSSREF","@value":"10.1029/2020je006669_references_DOI_RRON0wpK20TjxxP1MKv6OAEWKqm"},{"@type":"CROSSREF","@value":"10.1186/s40623-022-01717-z_references_DOI_RRON0wpK20TjxxP1MKv6OAEWKqm"},{"@type":"CROSSREF","@value":"10.1007/s11214-016-0240-9_references_DOI_RRON0wpK20TjxxP1MKv6OAEWKqm"},{"@type":"CROSSREF","@value":"10.1111/maps.12205_references_DOI_RRON0wpK20TjxxP1MKv6OAEWKqm"}]}