The trans-Neptunian object (84922) 2003 VS2 through stellar occultations
Autor(a) principal: | |
---|---|
Data de Publicação: | 2019 |
Outros Autores: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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. |
id |
UNSP_c262e78d88b14e1b3ee7552f4d1b7fd2 |
---|---|
oai_identifier_str |
oai:repositorio.unesp.br:11449/198579 |
network_acronym_str |
UNSP |
network_name_str |
Repositório Institucional da UNESP |
repository_id_str |
2946 |
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] |
author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
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 |
|
_version_ |
1808129565911941120 |