The trans-Neptunian object (84922) 2003 VS2 through stellar occultations

Detalhes bibliográficos
Autor(a) principal: Benedetti-Rossi, Gustavo
Data de Publicação: 2019
Outros Autores: Santos-Sanz, P., Ortiz, J. L., Assafin, M., Sicardy, B., Morales, N., Vieira-Martins, R., Duffard, R., Braga-Ribas, F., Rommel, F. L., Camargo, J. I.B., Desmars, J., Colas, A. F., Vachier, F., Alvarez-Candal, A., Fernández-Valenzuela, E., Almenares, L., Artola, R., Baum, T. P., Behrend, R., Bérard, D., Bianco, F. B., Brosch, N., Ceretta, A., Colazo, C. A., Gomes, A. R. [UNESP], Ivanov, V. D., Jehin, E., Kaspi, S., Lecacheux, J., Maury, A., Melia, R., Moindrot, S., Morgado, B., Opitom, C., Peyrot, A., Pollock, J., Pratt, A., Roland, S., Spagnotto, J., Tancredi, G., Teng, J. P., Cacella, P., Emilio, M., Feys, F., Gil-Hutton, R., Jacques, C., Machado, D. I., Malacarne, M., Manulis, I., Milone, A. C., Rojas, G., Sfair, R. [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.3847/1538-3881/ab3b05
http://hdl.handle.net/11449/198579
Resumo: We present results from three world-wide campaigns that resulted in the detections of two single-chord and one multi-chord stellar occultations by the plutino object (84922) 2003 VS2. From the single-chord occultations in 2013 and 2014 we obtained accurate astrometric positions for the object, while from the multi-chord occultation on 2014 November 7, we obtained the parameters of the best-fitting ellipse to the limb of the body at the time of occultation. We also obtained short-term photometry data for the body in order to derive its rotational phase during the occultation. The rotational light curve present a peak-to-peak amplitude of 0.141 ± 0.009 mag. This allows us to reconstruct the 3D shape of the body, with principal semi-axes of a = 313.8 ± 7.1 km, b = 265.5- + 9.8 8.8 km, and c = 247.3- + 43.6 26.6 km, which is not consistent with a Jacobi triaxial equilibrium figure. The derived spherical volume equivalent diameter of 548.3- + 44.6 29.5 km is about 5% larger than the radiometric diameter of 2003 VS2 derived from Herschel data of 523 ± 35 km, but still compatible with it within error bars. From those results we can also derive the geometric albedo (0.123- + 0.014 0.015) and, under the assumption that the object is a Maclaurin spheroid, the density r = 1400- + 300 1000 for the plutino. The disappearances and reappearances of the star during the occultations do not show any compelling evidence for a global atmosphere considering a pressure upper limit of about 1 microbar for a pure nitrogen atmosphere, nor secondary features (e.g., rings or satellite) around the main body.
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spelling The trans-Neptunian object (84922) 2003 VS2 through stellar occultationsKuiper belt (893)Trans-Neptunian objects (1705)Unified Astronomy Thesaurus concepts)We present results from three world-wide campaigns that resulted in the detections of two single-chord and one multi-chord stellar occultations by the plutino object (84922) 2003 VS2. From the single-chord occultations in 2013 and 2014 we obtained accurate astrometric positions for the object, while from the multi-chord occultation on 2014 November 7, we obtained the parameters of the best-fitting ellipse to the limb of the body at the time of occultation. We also obtained short-term photometry data for the body in order to derive its rotational phase during the occultation. The rotational light curve present a peak-to-peak amplitude of 0.141 ± 0.009 mag. This allows us to reconstruct the 3D shape of the body, with principal semi-axes of a = 313.8 ± 7.1 km, b = 265.5- + 9.8 8.8 km, and c = 247.3- + 43.6 26.6 km, which is not consistent with a Jacobi triaxial equilibrium figure. The derived spherical volume equivalent diameter of 548.3- + 44.6 29.5 km is about 5% larger than the radiometric diameter of 2003 VS2 derived from Herschel data of 523 ± 35 km, but still compatible with it within error bars. From those results we can also derive the geometric albedo (0.123- + 0.014 0.015) and, under the assumption that the object is a Maclaurin spheroid, the density r = 1400- + 300 1000 for the plutino. The disappearances and reappearances of the star during the occultations do not show any compelling evidence for a global atmosphere considering a pressure upper limit of about 1 microbar for a pure nitrogen atmosphere, nor secondary features (e.g., rings or satellite) around the main body.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Horizon 2020 Framework ProgrammeFundação de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ)Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)Observatório Nacional (ON/MCTIC), Rua Gal. José Cristino, 77Laboratório Interinstitucional de e-Astronomia (LIneA) & INCT do e-UniversoLESIA Observatoire de Paris Section Meudon, 5 Place Jules JanssenInstituto de Astrofísica de Andalucía IAA-CSIC, Glorieta de la Astronomía s/nObservatório do Valongo/UFRJ, Ladeira Pedro Antonio 43PSL Research University CNRS Sorbonne Université UPMC Univ. Paris 06 Univ. Paris DiderotIMCCE/Observatoire de Paris CNRS UMR F-8028Federal University of Technology—Paraná (UTFPR/DAFIS), Av. Sete de Setembro, 3165Florida Space Institute University of Central Florida, 12354 Research Parkway, Partnership 1, Suite 211Departamento de Astronomía Facultad de CienciasEstación Astrofísica de Bosque AlegreObservatoire Astronomique des Makes, Les MakesObservatoire de GenèveUniversity of Delaware Department of Physics and AstronomyUniversity of Delaware Joseph R. Biden Jr. School for Public Policy and AdministrationUniversity of Delaware Data Science InstituteNew York University Center for Urban Science and ProgressSchool of Physics and Astronomy and Wise Observatory Tel Aviv UniversityObservatorio Astronómico Los MolinosUNESP—São Paulo State University Grupo de Dinâmica Orbital e PlanetologiaESO, Karl-Schwarzschild-Str. 2STAR Institute University of Liège, Alleé du 6 Août 17San Pedro de Atacama Celestial Explorations, Casilla 21European Southern Observatory—Alonso de Cordova 3107Physics and Astronomy Department Appalachian State UniversityIOTA/ES—International Occultation Timing Association European SectionCURE Universidad de la RepublicaObservatorio El CatalejoDogsHeaven Observatory X87Universidade Estadual de Ponta Grossa O.A.—DEGEO, Avenida Carlos Cavalcanti 4748Grupo de Ciencias Planetarias Departamento de Geofísica y Astronomía San Juan National University and CONICET, Av. José I. de la Roza 590(0)Southern Observatory for Near Earth Asteroids Research (SONEAR)Universidade Estadual do Oeste do Paraná (Unioeste), Avenida Tarquínio Joslin dos Santos 1300Polo Astronômico Casimiro Montenegro Filho FPTI-BR, Avenida Tancredo Neves 6731Universidade Federal do Espírito Santo (UFES)Weizmann Institute of ScienceAstrophysics Division National Institute for Space Research (INPE), Av. dos Astronautas 1758Observatório Astronômico Universidade Federal de São Carlos (UFSCar)UNESP—São Paulo State University Grupo de Dinâmica Orbital e PlanetologiaFAPESP: 2011/08171-3FAPESP: 2016/ 24561-0FAPESP: 2018/11239-8CNPq: 304544/2017-5CNPq: 304971/2016-2CNPq: 308150/2016-3CNPq: 309578/2017-5CNPq: 310683/2017-3CNPq: 401669/2016-5CNPq: 401903/2016-8CNPq: 427700/ 2018-3CNPq: 473002/2013-2Horizon 2020 Framework Programme: 669416Horizon 2020 Framework Programme: 687378FAPERJ: E-26/111.488/2013FAPERJ: E-26/203.026/ 2015FAPERJ: E-26/203.186/2016CAPES: E26/203.173/2016FAPERJ: PAPDRJ-45/2013Observatório Nacional (ON/MCTIC)INCT do e-UniversoSection MeudonIAA-CSICUniversidade Federal do Rio de Janeiro (UFRJ)Univ. Paris DiderotCNRS UMR F-8028Federal University of Technology—Paraná (UTFPR/DAFIS)University of Central FloridaFacultad de CienciasEstación Astrofísica de Bosque AlegreObservatoire Astronomique des MakesObservatoire de GenèveUniversity of DelawareJoseph R. Biden Jr. School for Public Policy and AdministrationData Science InstituteCenter for Urban Science and ProgressTel Aviv UniversityObservatorio Astronómico Los MolinosUniversidade Estadual Paulista (Unesp)ESOUniversity of LiègeSan Pedro de Atacama Celestial ExplorationsEuropean Southern Observatory—Alonso de Cordova 3107Appalachian State UniversityEuropean SectionUniversidad de la RepublicaObservatorio El CatalejoDogsHeaven Observatory X87Universidade Estadual de Ponta Grossa (UEPG)San Juan National University and CONICETSouthern Observatory for Near Earth Asteroids Research (SONEAR)Universidade Estadual do Oeste do Paraná (Unioeste)FPTI-BRUniversidade Federal do Espírito Santo (UFES)Weizmann Institute of ScienceNational Institute for Space Research (INPE)Universidade Federal de São Carlos (UFSCar)Benedetti-Rossi, GustavoSantos-Sanz, P.Ortiz, J. L.Assafin, M.Sicardy, B.Morales, N.Vieira-Martins, R.Duffard, R.Braga-Ribas, F.Rommel, F. L.Camargo, J. I.B.Desmars, J.Colas, A. F.Vachier, F.Alvarez-Candal, A.Fernández-Valenzuela, E.Almenares, L.Artola, R.Baum, T. P.Behrend, R.Bérard, D.Bianco, F. B.Brosch, N.Ceretta, A.Colazo, C. A.Gomes, A. R. [UNESP]Ivanov, V. D.Jehin, E.Kaspi, S.Lecacheux, J.Maury, A.Melia, R.Moindrot, S.Morgado, B.Opitom, C.Peyrot, A.Pollock, J.Pratt, A.Roland, S.Spagnotto, J.Tancredi, G.Teng, J. P.Cacella, P.Emilio, M.Feys, F.Gil-Hutton, R.Jacques, C.Machado, D. I.Malacarne, M.Manulis, I.Milone, A. C.Rojas, G.Sfair, R. [UNESP]2020-12-12T01:16:44Z2020-12-12T01:16:44Z2019-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.3847/1538-3881/ab3b05Astronomical Journal, v. 158, n. 4, 2019.0004-6256http://hdl.handle.net/11449/19857910.3847/1538-3881/ab3b052-s2.0-85080149396Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengAstronomical Journalinfo:eu-repo/semantics/openAccess2021-10-22T17:02:34Zoai:repositorio.unesp.br:11449/198579Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T23:56:59.273135Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv The trans-Neptunian object (84922) 2003 VS2 through stellar occultations
title The trans-Neptunian object (84922) 2003 VS2 through stellar occultations
spellingShingle The trans-Neptunian object (84922) 2003 VS2 through stellar occultations
Benedetti-Rossi, Gustavo
Kuiper belt (893)
Trans-Neptunian objects (1705)
Unified Astronomy Thesaurus concepts)
title_short The trans-Neptunian object (84922) 2003 VS2 through stellar occultations
title_full The trans-Neptunian object (84922) 2003 VS2 through stellar occultations
title_fullStr The trans-Neptunian object (84922) 2003 VS2 through stellar occultations
title_full_unstemmed The trans-Neptunian object (84922) 2003 VS2 through stellar occultations
title_sort The trans-Neptunian object (84922) 2003 VS2 through stellar occultations
author Benedetti-Rossi, Gustavo
author_facet Benedetti-Rossi, Gustavo
Santos-Sanz, P.
Ortiz, J. L.
Assafin, M.
Sicardy, B.
Morales, N.
Vieira-Martins, R.
Duffard, R.
Braga-Ribas, F.
Rommel, F. L.
Camargo, J. I.B.
Desmars, J.
Colas, A. F.
Vachier, F.
Alvarez-Candal, A.
Fernández-Valenzuela, E.
Almenares, L.
Artola, R.
Baum, T. P.
Behrend, R.
Bérard, D.
Bianco, F. B.
Brosch, N.
Ceretta, A.
Colazo, C. A.
Gomes, A. R. [UNESP]
Ivanov, V. D.
Jehin, E.
Kaspi, S.
Lecacheux, J.
Maury, A.
Melia, R.
Moindrot, S.
Morgado, B.
Opitom, C.
Peyrot, A.
Pollock, J.
Pratt, A.
Roland, S.
Spagnotto, J.
Tancredi, G.
Teng, J. P.
Cacella, P.
Emilio, M.
Feys, F.
Gil-Hutton, R.
Jacques, C.
Machado, D. I.
Malacarne, M.
Manulis, I.
Milone, A. C.
Rojas, G.
Sfair, R. [UNESP]
author_role author
author2 Santos-Sanz, P.
Ortiz, J. L.
Assafin, M.
Sicardy, B.
Morales, N.
Vieira-Martins, R.
Duffard, R.
Braga-Ribas, F.
Rommel, F. L.
Camargo, J. I.B.
Desmars, J.
Colas, A. F.
Vachier, F.
Alvarez-Candal, A.
Fernández-Valenzuela, E.
Almenares, L.
Artola, R.
Baum, T. P.
Behrend, R.
Bérard, D.
Bianco, F. B.
Brosch, N.
Ceretta, A.
Colazo, C. A.
Gomes, A. R. [UNESP]
Ivanov, V. D.
Jehin, E.
Kaspi, S.
Lecacheux, J.
Maury, A.
Melia, R.
Moindrot, S.
Morgado, B.
Opitom, C.
Peyrot, A.
Pollock, J.
Pratt, A.
Roland, S.
Spagnotto, J.
Tancredi, G.
Teng, J. P.
Cacella, P.
Emilio, M.
Feys, F.
Gil-Hutton, R.
Jacques, C.
Machado, D. I.
Malacarne, M.
Manulis, I.
Milone, A. C.
Rojas, G.
Sfair, R. [UNESP]
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dc.contributor.none.fl_str_mv Observatório Nacional (ON/MCTIC)
INCT do e-Universo
Section Meudon
IAA-CSIC
Universidade Federal do Rio de Janeiro (UFRJ)
Univ. Paris Diderot
CNRS UMR F-8028
Federal University of Technology—Paraná (UTFPR/DAFIS)
University of Central Florida
Facultad de Ciencias
Estación Astrofísica de Bosque Alegre
Observatoire Astronomique des Makes
Observatoire de Genève
University of Delaware
Joseph R. Biden Jr. School for Public Policy and Administration
Data Science Institute
Center for Urban Science and Progress
Tel Aviv University
Observatorio Astronómico Los Molinos
Universidade Estadual Paulista (Unesp)
ESO
University of Liège
San Pedro de Atacama Celestial Explorations
European Southern Observatory—Alonso de Cordova 3107
Appalachian State University
European Section
Universidad de la Republica
Observatorio El Catalejo
DogsHeaven Observatory X87
Universidade Estadual de Ponta Grossa (UEPG)
San Juan National University and CONICET
Southern Observatory for Near Earth Asteroids Research (SONEAR)
Universidade Estadual do Oeste do Paraná (Unioeste)
FPTI-BR
Universidade Federal do Espírito Santo (UFES)
Weizmann Institute of Science
National Institute for Space Research (INPE)
Universidade Federal de São Carlos (UFSCar)
dc.contributor.author.fl_str_mv Benedetti-Rossi, Gustavo
Santos-Sanz, P.
Ortiz, J. L.
Assafin, M.
Sicardy, B.
Morales, N.
Vieira-Martins, R.
Duffard, R.
Braga-Ribas, F.
Rommel, F. L.
Camargo, J. I.B.
Desmars, J.
Colas, A. F.
Vachier, F.
Alvarez-Candal, A.
Fernández-Valenzuela, E.
Almenares, L.
Artola, R.
Baum, T. P.
Behrend, R.
Bérard, D.
Bianco, F. B.
Brosch, N.
Ceretta, A.
Colazo, C. A.
Gomes, A. R. [UNESP]
Ivanov, V. D.
Jehin, E.
Kaspi, S.
Lecacheux, J.
Maury, A.
Melia, R.
Moindrot, S.
Morgado, B.
Opitom, C.
Peyrot, A.
Pollock, J.
Pratt, A.
Roland, S.
Spagnotto, J.
Tancredi, G.
Teng, J. P.
Cacella, P.
Emilio, M.
Feys, F.
Gil-Hutton, R.
Jacques, C.
Machado, D. I.
Malacarne, M.
Manulis, I.
Milone, A. C.
Rojas, G.
Sfair, R. [UNESP]
dc.subject.por.fl_str_mv Kuiper belt (893)
Trans-Neptunian objects (1705)
Unified Astronomy Thesaurus concepts)
topic Kuiper belt (893)
Trans-Neptunian objects (1705)
Unified Astronomy Thesaurus concepts)
description We present results from three world-wide campaigns that resulted in the detections of two single-chord and one multi-chord stellar occultations by the plutino object (84922) 2003 VS2. From the single-chord occultations in 2013 and 2014 we obtained accurate astrometric positions for the object, while from the multi-chord occultation on 2014 November 7, we obtained the parameters of the best-fitting ellipse to the limb of the body at the time of occultation. We also obtained short-term photometry data for the body in order to derive its rotational phase during the occultation. The rotational light curve present a peak-to-peak amplitude of 0.141 ± 0.009 mag. This allows us to reconstruct the 3D shape of the body, with principal semi-axes of a = 313.8 ± 7.1 km, b = 265.5- + 9.8 8.8 km, and c = 247.3- + 43.6 26.6 km, which is not consistent with a Jacobi triaxial equilibrium figure. The derived spherical volume equivalent diameter of 548.3- + 44.6 29.5 km is about 5% larger than the radiometric diameter of 2003 VS2 derived from Herschel data of 523 ± 35 km, but still compatible with it within error bars. From those results we can also derive the geometric albedo (0.123- + 0.014 0.015) and, under the assumption that the object is a Maclaurin spheroid, the density r = 1400- + 300 1000 for the plutino. The disappearances and reappearances of the star during the occultations do not show any compelling evidence for a global atmosphere considering a pressure upper limit of about 1 microbar for a pure nitrogen atmosphere, nor secondary features (e.g., rings or satellite) around the main body.
publishDate 2019
dc.date.none.fl_str_mv 2019-01-01
2020-12-12T01:16:44Z
2020-12-12T01:16:44Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.3847/1538-3881/ab3b05
Astronomical Journal, v. 158, n. 4, 2019.
0004-6256
http://hdl.handle.net/11449/198579
10.3847/1538-3881/ab3b05
2-s2.0-85080149396
url http://dx.doi.org/10.3847/1538-3881/ab3b05
http://hdl.handle.net/11449/198579
identifier_str_mv Astronomical Journal, v. 158, n. 4, 2019.
0004-6256
10.3847/1538-3881/ab3b05
2-s2.0-85080149396
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Astronomical Journal
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
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