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Physical properties of trans-Neptunian object (143707) 2003 UY117 derived from stellar occultation and photometric observations

dc.contributor.authorKretlow, M.
dc.contributor.authorOrtiz, J. L.
dc.contributor.authorDesmars, J.
dc.contributor.authorMorales, N.
dc.contributor.authorRommel, F. L.
dc.contributor.authorSantos-Sanz, P.
dc.contributor.authorVara-Lubiano, M.
dc.contributor.authorFernández-Valenzuela, E.
dc.contributor.authorAlvarez-Candal, A.
dc.contributor.authorDuffard, R.
dc.contributor.authorBraga-Ribas, F.
dc.contributor.authorSicardy, B.
dc.contributor.authorCastro-Tirado, A.
dc.contributor.authorFernández-García, E. J.
dc.contributor.authorSánchez, M.
dc.contributor.authorSota, A.
dc.contributor.authorAssafin, M.
dc.contributor.authorBenedetti-Rossi, G. [UNESP]
dc.contributor.authorBoufleur, R.
dc.contributor.authorCamargo, J. I.B.
dc.contributor.authorCikota, S.
dc.contributor.authorGomes-Junior, A.
dc.contributor.authorGómez-Limón, J. M.
dc.contributor.authorKilic, Y.
dc.contributor.authorLecacheux, J.
dc.contributor.authorLeiva, R.
dc.contributor.authorMarques-Oliveira, J.
dc.contributor.authorMorales, R.
dc.contributor.authorMorgado, B.
dc.contributor.authorRizos, J. L.
dc.contributor.authorRoques, F.
dc.contributor.authorSouami, D.
dc.contributor.authorVieira-Martins, R.
dc.contributor.authorAlarcon, M. R.
dc.contributor.authorBoninsegna, R.
dc.contributor.authorÇakir, O.
dc.contributor.authorCasarramona, F.
dc.contributor.authorCastellani, J. J.
dc.contributor.authorDe La Cueva, I.
dc.contributor.authorFişek, S.
dc.contributor.authorGuijarro, A.
dc.contributor.authorHaymes, T.
dc.contributor.authorJehin, E.
dc.contributor.authorKidd, S.
dc.contributor.authorLicandro, J.
dc.contributor.authorMaestre, J. L.
dc.contributor.authorMurgas, F.
dc.contributor.authorPallé, E.
dc.contributor.authorPopescu, M.
dc.contributor.authorPratt, A.
dc.contributor.authorSerra-Ricart, M.
dc.contributor.authorTalbot, J. C.
dc.contributor.institutionIAA-CSIC
dc.contributor.institutionInstitut Polytechnique des Sciences Avancées IPSA
dc.contributor.institutionUniv. Lille
dc.contributor.institutionFederal University of Technology-Paraná (UTFPR/PPGFA)
dc.contributor.institutionINCT Do E-Universo
dc.contributor.institutionSorbonne Université
dc.contributor.institutionUniversity of Central Florida
dc.contributor.institutionUniversidade Federal de Uberlândia (UFU)
dc.contributor.institutionUniversidade Do Rio de Janeiro - Observatório Do Valongo
dc.contributor.institutionFederal University of Technology - Paraná (PPGFA/UTFPR-Curitiba)
dc.contributor.institutionUniversity of California
dc.contributor.institutionUniversity of Namur
dc.contributor.institutionObservatório Nacional/MCTI
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.contributor.institutionSociedad Astronómica Granadina
dc.contributor.institutionAgrupación Astronómica de Eivissa
dc.contributor.institutionObservatorio Astronómico de Albox
dc.contributor.institutionAstronomical Institute of the Romanian Academy
dc.contributor.institutionSierra de Los Filabres
dc.contributor.institutionUniversity of Liège
dc.contributor.institutionInstituto de Astrofísica de Canarias (IAC)
dc.contributor.institutionUniversidad de Alicante
dc.contributor.institutionAgrupación Astronómica de Sabadell
dc.contributor.institutionInternational Occultation Timing Association/European Section
dc.contributor.institutionAkdeniz University Campus
dc.contributor.institutionIstanbul University
dc.contributor.institutionIstanbul University Observatory Research and Application Centre
dc.contributor.institutionMacquarie University
dc.date.accessioned2025-04-29T20:17:01Z
dc.date.issued2024-11-01
dc.description.abstractContext. Trans-Neptunian objects (TNOs) are considered to be among the most primitive objects in our Solar System. Knowledge of their primary physical properties is essential for understanding their origin and the evolution of the outer Solar System. In this context, stellar occultations are a powerful and sensitive technique for studying these distant and faint objects. Aims. We aim to obtain the size, shape, absolute magnitude, and geometric albedo for TNO (143707) 2003 UY117. Methods. We predicted a stellar occultation by this TNO for 2020 October 23 UT and ran a specific campaign to investigate this event. We derived the projected profile shape and size from the occultation observations by means of an elliptical fit to the occultation chords. We also performed photometric observations of (143707) 2003 UY117 to obtain the absolute magnitude and the rotational period from the observed rotational light curve. Finally, we combined these results to derive the three-dimensional shape, volume-equivalent diameter, and geometric albedo for this TNO. Results. From the stellar occultation, we obtained a projected ellipse with axes of (282 ± 18) × (184 ± 32) km. The area-equivalent diameter for this ellipse is Deq,A = 228 ± 21 km. From our photometric R band observations, we derived an absolute magnitude of HV = 5.97 ± 0.07 mag using V - R = 0.46 ± 0.07 mag, which was derived from a V band subset of these data. The rotational light curve has a peak-to-valley amplitude of Δm = 0.36 ± 0.13 mag. We find the most likely rotation period to be P = 12.376 ± 0.0033 hours. By combining the occultation with the rotational light curve results and assuming a triaxial ellipsoid, we derived axes of a × b × c = (332 ± 24) km × (216 ± 24) km × (180-24+28) km for this ellipsoid, and therefore a volume-equivalent diameter of Deq,V = 235 ± 25 km. Finally, the values for the absolute magnitude and for the area-equivalent diameter yield a geometric albedo of pV = 0.139 ± 0.027.en
dc.description.affiliationInstituto de Astrofísica de Andalucía IAA-CSIC, Glorieta de la Astronomía s/n
dc.description.affiliationInstitut Polytechnique des Sciences Avancées IPSA, Ivrysur-Seine
dc.description.affiliationIMCCE Observatoire de Paris PSL Research University CNRS Sorbonne Université Univ. Lille
dc.description.affiliationFederal University of Technology-Paraná (UTFPR/PPGFA), PR
dc.description.affiliationLaboratório Interinstitucional de E-Astronomia - LIneA INCT Do E-Universo, Av. Pastor Martin Luther King Jr, 126 - Del Castilho, Nova América Offices, Torre 3000/sala 817, RJ
dc.description.affiliationLESIA Observatoire de Paris Université PSL CNRS Sorbonne Université, 5 place Jules Janssen
dc.description.affiliationFlorida Space Institute University of Central Florida
dc.description.affiliationFederal University of Uberlândia (UFU) Physics Institute, Av. João Naves de Ávila 2121
dc.description.affiliationUniversidade Do Rio de Janeiro - Observatório Do Valongo, Ladeira do Pedro Antonio 43
dc.description.affiliationFederal University of Technology - Paraná (PPGFA/UTFPR-Curitiba), Av. Sete de Setembro, PR
dc.description.affiliationDepartments of Astronomy and of Earth and Planetary Science University of California, 501 Campbell Hall
dc.description.affiliationNaXys Department of Mathematics University of Namur, Rue de Bruxelles 61
dc.description.affiliationObservatório Nacional/MCTI, Rua Gal. José Cristino 77
dc.description.affiliationUNESP-São Paulo State University Grupo de Dinâmica Orbital e Planetologia, SP
dc.description.affiliationSociedad Astronómica Granadina, Apartado de Correos 195
dc.description.affiliationAgrupación Astronómica de Eivissa, C. Lucio Oculacio s/n
dc.description.affiliationObservatorio Astronómico de Albox, Apt. 63, Almeria
dc.description.affiliationAstronomical Institute of the Romanian Academy, 5 Cuţitul de Argint
dc.description.affiliationCentro Astronómico Hispano en Andalucía Observatorio de Calar Alto Sierra de Los Filabres, Almeria
dc.description.affiliationUniversity of Liège
dc.description.affiliationInstituto de Astrofísica de Canarias (IAC), C/Vía Láctea s/n, Tenerife
dc.description.affiliationInstituto de Física Aplicada A Las Ciencias y Las Tecnologías Universidad de Alicante, San Vicente del Rapeig
dc.description.affiliationAgrupación Astronómica de Sabadell, Prat de la Riba sn
dc.description.affiliationInternational Occultation Timing Association/European Section, Am Brombeerhag 13
dc.description.affiliationTÜBITAK National Observatory Akdeniz University Campus
dc.description.affiliationDepartment of Astronomy and Space Sciences Faculty of Science Istanbul University
dc.description.affiliationIstanbul University Observatory Research and Application Centre
dc.description.affiliationSchool of Mathematical and Physical Sciences Macquarie University
dc.description.affiliationAstrophysics and Space Technologies Research Centre Macquarie University
dc.description.affiliationUnespUNESP-São Paulo State University Grupo de Dinâmica Orbital e Planetologia, SP
dc.identifierhttp://dx.doi.org/10.1051/0004-6361/202451329
dc.identifier.citationAstronomy and Astrophysics, v. 691.
dc.identifier.doi10.1051/0004-6361/202451329
dc.identifier.issn1432-0746
dc.identifier.issn0004-6361
dc.identifier.scopus2-s2.0-85208725785
dc.identifier.urihttps://hdl.handle.net/11449/309895
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.sourceScopus
dc.subjectAstrometry
dc.subjectKuiper belt objects: individual: (143707) 2003 UY117
dc.subjectMethods: observational
dc.subjectOccultations
dc.subjectTechniques: photometric
dc.titlePhysical properties of trans-Neptunian object (143707) 2003 UY117 derived from stellar occultation and photometric observationsen
dc.typeArtigopt
dspace.entity.typePublication
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