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Authordc.contributor.authorMorgado, B. E.
Authordc.contributor.authorSicardy, B.
Authordc.contributor.authorBraga Ribas, F.
Authordc.contributor.authorDesmars, J.
Authordc.contributor.authorGomes Junior, A. R.
Authordc.contributor.authorBerard, D.
Authordc.contributor.authorLeiva Espinoza, Rodrigo Andrés
Authordc.contributor.authorOrtiz, J. L.
Authordc.contributor.authorVieira Martins, R.
Authordc.contributor.authorBenedetti Rossi, G.
Authordc.contributor.authorSantos Sanz, P.
Authordc.contributor.authorCamargo, J. I. B.
Authordc.contributor.authorDuffard, R.
Authordc.contributor.authorRommel, F. L.
Authordc.contributor.authorAssafin, M.
Authordc.contributor.authorBoufleur, R. C.
Authordc.contributor.authorColas, F.
Authordc.contributor.authorKretlow, M.
Authordc.contributor.authorBeisker, W.
Authordc.contributor.authorSfair, R.
Authordc.contributor.authorSnodgrass, C.
Authordc.contributor.authorMorales, N.
Authordc.contributor.authorFernández Valenzuela, E.
Authordc.contributor.authorAmaral, L. S.
Authordc.contributor.authorAmarante, A.
Authordc.contributor.authorArtola, R. A.
Authordc.contributor.authorBackes, M.
Authordc.contributor.authorBath, K. L.
Authordc.contributor.authorBouley, S.
Authordc.contributor.authorBuie, M. W.
Authordc.contributor.authorCacella, P.
Authordc.contributor.authorColazo, C. A.
Authordc.contributor.authorColque, J. P.
Authordc.contributor.authorDauvergne, J. L.
Authordc.contributor.authorDominik, M.
Authordc.contributor.authorEmilio, M.
Authordc.contributor.authorErickson, C.
Authordc.contributor.authorEvans, R.
Authordc.contributor.authorFabrega Polleri, J.
Authordc.contributor.authorGarcia Lambas, D.
Authordc.contributor.authorGiacchini, B. L.
Authordc.contributor.authorHanna, W.
Authordc.contributor.authorHerald, D.
Authordc.contributor.authorHesler, G.
Authordc.contributor.authorHinse, T. C.
Authordc.contributor.authorJacques, C.
Authordc.contributor.authorJehin, E.
Authordc.contributor.authorJorgensen, U. G.
Authordc.contributor.authorMachado, D. I.
Authordc.contributor.authorMaquet, L.
Authordc.contributor.authorMaury, A.
Authordc.contributor.authorMelia, R.
Authordc.contributor.authorMeza, E.
Authordc.contributor.authorMondon, B.
Authordc.contributor.authorMoura, T.
Authordc.contributor.authorNewman, J.
Authordc.contributor.authorPayet, T.
Authordc.contributor.authorPereira, C. L.
Authordc.contributor.authorPollock, J.
Authordc.contributor.authorPoltronieri, R. C.
Authordc.contributor.authorQuispe Huaynasi, F.
Authordc.contributor.authorReichart, D.
Authordc.contributor.authorde Santana, T.
Authordc.contributor.authorSchneiter, E. M.
Authordc.contributor.authorSieyra, M. V.
Authordc.contributor.authorSkottfelt, J.
Authordc.contributor.authorSoulier, J. F.
Authordc.contributor.authorStarck, M.
Authordc.contributor.authorThierry, P.
Authordc.contributor.authorTorres, P. J.
Authordc.contributor.authorTrabuco, L. L.
Authordc.contributor.authorUnda Sanzana, E.
Authordc.contributor.authorYamashita, T. A. R.
Authordc.contributor.authorWinter, O. C.
Authordc.contributor.authorZapata, A.
Authordc.contributor.authorZuluaga, C. A.
Admission datedc.date.accessioned2021-11-29T21:07:17Z
Available datedc.date.available2021-11-29T21:07:17Z
Publication datedc.date.issued2021
Cita de ítemdc.identifier.citationAstronomy & Astrophysics Volume 652 Article Number A141 Published Aug 25 2021es_ES
Identifierdc.identifier.other10.1051/0004-6361/202141543
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/182926
Abstractdc.description.abstractContext. The Centaur (10199) Chariklo has the first ring system discovered around a small object. It was first observed using stellar occultation in 2013. Stellar occultations allow sizes and shapes to be determined with kilometre accuracy, and provide the characteristics of the occulting object and its vicinity. Aims. Using stellar occultations observed between 2017 and 2020, our aim is to constrain the physical parameters of Chariklo and its rings. We also determine the structure of the rings, and obtain precise astrometrical positions of Chariklo. Methods. We predicted and organised several observational campaigns of stellar occultations by Chariklo. Occultation light curves were measured from the datasets, from which ingress and egress times, and the ring widths and opacity values were obtained. These measurements, combined with results from previous works, allow us to obtain significant constraints on Chariklo's shape and ring structure. Results. We characterise Chariklo's ring system (C1R and C2R), and obtain radii and pole orientations that are consistent with, but more accurate than, results from previous occultations. We confirm the detection of W-shaped structures within C1R and an evident variation in radial width. The observed width ranges between 4.8 and 9.1 km with a mean value of 6.5 km. One dual observation (visible and red) does not reveal any differences in the C1R opacity profiles, indicating a ring particle size larger than a few microns. The C1R ring eccentricity is found to be smaller than 0.022 (3 sigma), and its width variations may indicate an eccentricity higher than similar to 0.005. We fit a tri-axial shape to Chariklo's detections over 11 occultations, and determine that Chariklo is consistent with an ellipsoid with semi-axes of 143.8(-1.5)(+1.4), 135.2(-2.8)(+1.4), and 99.1(-2.7)(+5.4) km. Ultimately, we provided seven astrometric positions at a milliarcsecond accuracy level, based on Gaia EDR3, and use it to improve Chariklo's ephemeris.es_ES
Patrocinadordc.description.sponsorshipEuropean Research Council under the European Community's H2020 669416 Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPQ) Fundacao de Apoio a Pesquisa do Distrito Federal (FAPDF) 465376/2014-2 European Union H2020-MSCA-ITN-2019 860470 Novo Nordisk Foundation Interdisciplinary Synergy Programme NNF19OC0057374 Fonds de la Recherche Scientifique - FNRS PDR T.0120.21 Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPQ) BEM 150612/2020-6 FB-R 314772/2020-0 RV-M 304544/2017-f5 401903/2016-8 JIBC 308150/2016-3 305917/20196 MA 427700/2018-3es_ES
Lenguagedc.language.isoenes_ES
Publisherdc.publisherEDP Scienceses_ES
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 United States*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/us/*
Sourcedc.sourceAstronomy & Astrophysicses_ES
Keywordsdc.subjectOccultationses_ES
Keywordsdc.subjectMethods: observationales_ES
Keywordsdc.subjectMethods: data analysises_ES
Keywordsdc.subjectMinor planets, asteroids: individual: Charikloes_ES
Keywordsdc.subjectPlanets and satellites: ringses_ES
Títulodc.titleRefined physical parameters for Chariklo's body and rings from stellar occultations observed between 2013 and 2020es_ES
Document typedc.typeArtículo de revistaes_ES
dc.description.versiondc.description.versionVersión aceptada para publicar - Postprintes_ES
dcterms.accessRightsdcterms.accessRightsAcceso abiertoes_ES
Catalogueruchile.catalogadorcrbes_ES
Indexationuchile.indexArtículo de publícación WoSes_ES


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Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 United States