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dc.contributor.authorRibeiro, Tânia M.es-ES
dc.contributor.authorD’Ambrosio, Andreaes-ES
dc.contributor.authorDomínguez Calabuig, Guillermo J.es-ES
dc.contributor.authorAthanasopoulos, Dimitrioses-ES
dc.contributor.authorBates, Helenaes-ES
dc.contributor.authorRiegler, Clemenses-ES
dc.contributor.authorGassot, Orianees-ES
dc.contributor.authorGerig, Selina-Barbaraes-ES
dc.contributor.authorGómez González, Juan Luises-ES
dc.contributor.authorHuber, Nikolauses-ES
dc.contributor.authorSeton, Ragnares-ES
dc.contributor.authorMagalhães, Tiago E.C.es-ES
dc.date.accessioned2024-02-23T13:19:36Z
dc.date.available2024-02-23T13:19:36Z
dc.date.issued2023-11-01es_ES
dc.identifier.issn0094-5765es_ES
dc.identifier.urihttps://doi.org/10.1016/j.actaastro.2023.07.035es_ES
dc.descriptionArtículos en revistases_ES
dc.description.abstractD-type asteroids are among the most primitive small bodies of the solar system. Believed to be formed in the outer solar system, a minor fraction of these faint objects can be found in the near-Earth region. Some were suspected to be extinct comets disguised as asteroids. If D-type near-Earth asteroids could represent extinct comets, they would offer us a unique opportunity to investigate the relationship between two classes of minor bodies in our solar system. To provide new insights into D-type asteroids’ composition and dynamical evolution and the possible relation with comets, we introduce the mission concept CARINA (Comet Asteroid Relation INvestigation and Analysis). CARINA will visit and collect a sample from the asteroid 2002 AT4 and address key scientific questions related to our understanding of the early solar system evolution, and the origins of water and life on the early Earth. This paper outlines the scientific motivation and the means for the sample return. The spacecraft is equipped with a sampling ring to perform in-situ analysis and to collect, in a “touch and go” manner, samples from the surface and subsurface of the asteroid. A capsule is expected to return the samples to Earth in pristine conditions for detailed and extended analysis. These would represent a rare contribution to our meteorite collection since it would be the first time that material from a D class asteroid would be collected.es-ES
dc.description.abstractD-type asteroids are among the most primitive small bodies of the solar system. Believed to be formed in the outer solar system, a minor fraction of these faint objects can be found in the near-Earth region. Some were suspected to be extinct comets disguised as asteroids. If D-type near-Earth asteroids could represent extinct comets, they would offer us a unique opportunity to investigate the relationship between two classes of minor bodies in our solar system. To provide new insights into D-type asteroids’ composition and dynamical evolution and the possible relation with comets, we introduce the mission concept CARINA (Comet Asteroid Relation INvestigation and Analysis). CARINA will visit and collect a sample from the asteroid 2002 AT4 and address key scientific questions related to our understanding of the early solar system evolution, and the origins of water and life on the early Earth. This paper outlines the scientific motivation and the means for the sample return. The spacecraft is equipped with a sampling ring to perform in-situ analysis and to collect, in a “touch and go” manner, samples from the surface and subsurface of the asteroid. A capsule is expected to return the samples to Earth in pristine conditions for detailed and extended analysis. These would represent a rare contribution to our meteorite collection since it would be the first time that material from a D class asteroid would be collected.en-GB
dc.format.mimetypeapplication/octet-streames_ES
dc.language.isoen-GBes_ES
dc.sourceRevista: Acta Astronautica, Periodo: 1, Volumen: online, Número: , Página inicial: 213, Página final: 225es_ES
dc.subject.otherInstituto de Investigación Tecnológica (IIT)es_ES
dc.titleCARINA: a near-Earth D-type asteroid sample return missiones_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.description.versioninfo:eu-repo/semantics/publishedVersiones_ES
dc.rights.holderes_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.keywordsD-type asteroids; Comets; Near-earth objects; Sample return; Asteroid–comet continuum; Solar system evolution; Astrobiologyes-ES
dc.keywordsD-type asteroids; Comets; Near-earth objects; Sample return; Asteroid–comet continuum; Solar system evolution; Astrobiologyen-GB


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