The multichord stellar occultation on 2019 October 22 by the trans-Neptunian object (84922) 2003 VS\(_2\)
We predicted, observed, and analyzed the multichord stellar occultation of the Second Gaia Data Release (Gaia DR2) source 3449076721168026624 (m\(_v\) = 14.1 mag) by the plutino object 2003 VS\(_2\) (hereafter, VS\(_2\)) on 2019 October 22. We also carried out photometric observations to derive the...
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creator | Vara-Lubiano, M Benedetti-Rossi, G Santos-Sanz, P Ortiz, J L Sicardy, B Popescu, M Morales, N Rommel, F L Morgado, B Pereira, C L Álvarez-Candal, A Fernández-Valenzuela, E Souami, D Ilic, D Vince, O Bachev, R Semkov, E Nedelcu, D A A \c{S}onka Hudin, L Boaca, M Inceu, V Curelaru, L Gherase, R Turcu, V Moldovan, D Mircea, L Predatu, M Teodorescu, M Stoian, L Juravle, A Braga-Ribas, F Desmars, J Duffard, R Lecacheux, J Camargo, J I B Assafin, M Vieira-Martins, R Pribulla, T Husárik, M Sivanič, P Pal, A Szakats, R Kiss, C Alonso-Santiago, J Frasca, A Szabó, G M Derekas, A Szigeti, L Drozdz, M Ogloza, W J Skvar\u{c} Ciabattari, F Delincak, P P Di Marcantonio Iafrate, G Coretti, I Baldini, V Baruffetti, P Klös, O Dumitrescu, V Mikuž, H Mohar, A |
description | We predicted, observed, and analyzed the multichord stellar occultation of the Second Gaia Data Release (Gaia DR2) source 3449076721168026624 (m\(_v\) = 14.1 mag) by the plutino object 2003 VS\(_2\) (hereafter, VS\(_2\)) on 2019 October 22. We also carried out photometric observations to derive the rotational light curve amplitude and rotational phase of VS\(_2\) during the stellar occultation. Combining the results and assuming a triaxial shape, we derived the 3D shape of VS\(_2\). Out of the 39 observatories involved in the observational campaign, 12 sites reported a positive detection; this makes it one of the best observed stellar occultations by a TNO so far. We obtained a rotational light curve amplitude of \({\Delta}\)m = 0.264 \(\pm\) 0.017 mag, a mean area-equivalent diameter of D\(_{A_{eq}}\) = 545 \(\pm\) 13 km, and a geometric albedo of 0.134 \(\pm\) 0.010. The best triaxial shape obtained for VS\(_2\) has semiaxes a = 339 \(\pm\) 5 km, b = 235 \(\pm\) 6 km, and c = 226 \(\pm\) 8 km. The derived aspect angle is \({\theta}\) = 59\({\deg} \pm\) 2\({\deg}\) or its supplementary \({\theta}\) = 121\({\deg} \pm\) 2\({\deg}\), depending on the north-pole position. The spherical-volume equivalent diameter is D\(_{V_{eq}}\) = 524 \(\pm\) 7 km. If we consider large albedo patches on its surface, the semi-major axis of the ellipsoid could be ~10 km smaller. These results are compatible with the previous ones determined from the single-chord 2013 and four-chord 2014 stellar occultations and with the effective diameter and albedo derived from Herschel and Spitzer data. They provide evidence that VS\(_2\)'s 3D shape is not compatible with a homogeneous triaxial body in hydrostatic equilibrium, but it might be a differentiated body and/or might be sustaining some stress. No secondary features related to rings or material orbiting around VS\(_2\) were detected. |
doi_str_mv | 10.48550/arxiv.2205.12878 |
format | Article |
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We also carried out photometric observations to derive the rotational light curve amplitude and rotational phase of VS\(_2\) during the stellar occultation. Combining the results and assuming a triaxial shape, we derived the 3D shape of VS\(_2\). Out of the 39 observatories involved in the observational campaign, 12 sites reported a positive detection; this makes it one of the best observed stellar occultations by a TNO so far. We obtained a rotational light curve amplitude of \({\Delta}\)m = 0.264 \(\pm\) 0.017 mag, a mean area-equivalent diameter of D\(_{A_{eq}}\) = 545 \(\pm\) 13 km, and a geometric albedo of 0.134 \(\pm\) 0.010. The best triaxial shape obtained for VS\(_2\) has semiaxes a = 339 \(\pm\) 5 km, b = 235 \(\pm\) 6 km, and c = 226 \(\pm\) 8 km. The derived aspect angle is \({\theta}\) = 59\({\deg} \pm\) 2\({\deg}\) or its supplementary \({\theta}\) = 121\({\deg} \pm\) 2\({\deg}\), depending on the north-pole position. The spherical-volume equivalent diameter is D\(_{V_{eq}}\) = 524 \(\pm\) 7 km. If we consider large albedo patches on its surface, the semi-major axis of the ellipsoid could be ~10 km smaller. These results are compatible with the previous ones determined from the single-chord 2013 and four-chord 2014 stellar occultations and with the effective diameter and albedo derived from Herschel and Spitzer data. They provide evidence that VS\(_2\)'s 3D shape is not compatible with a homogeneous triaxial body in hydrostatic equilibrium, but it might be a differentiated body and/or might be sustaining some stress. No secondary features related to rings or material orbiting around VS\(_2\) were detected.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2205.12878</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Albedo ; Amplitudes ; Chords (geometry) ; Equivalence ; Light curve ; Observatories ; Stellar occultation ; Trans-Neptunian objects</subject><ispartof>arXiv.org, 2022-05</ispartof><rights>2022. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). 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We also carried out photometric observations to derive the rotational light curve amplitude and rotational phase of VS\(_2\) during the stellar occultation. Combining the results and assuming a triaxial shape, we derived the 3D shape of VS\(_2\). Out of the 39 observatories involved in the observational campaign, 12 sites reported a positive detection; this makes it one of the best observed stellar occultations by a TNO so far. We obtained a rotational light curve amplitude of \({\Delta}\)m = 0.264 \(\pm\) 0.017 mag, a mean area-equivalent diameter of D\(_{A_{eq}}\) = 545 \(\pm\) 13 km, and a geometric albedo of 0.134 \(\pm\) 0.010. The best triaxial shape obtained for VS\(_2\) has semiaxes a = 339 \(\pm\) 5 km, b = 235 \(\pm\) 6 km, and c = 226 \(\pm\) 8 km. The derived aspect angle is \({\theta}\) = 59\({\deg} \pm\) 2\({\deg}\) or its supplementary \({\theta}\) = 121\({\deg} \pm\) 2\({\deg}\), depending on the north-pole position. The spherical-volume equivalent diameter is D\(_{V_{eq}}\) = 524 \(\pm\) 7 km. If we consider large albedo patches on its surface, the semi-major axis of the ellipsoid could be ~10 km smaller. These results are compatible with the previous ones determined from the single-chord 2013 and four-chord 2014 stellar occultations and with the effective diameter and albedo derived from Herschel and Spitzer data. They provide evidence that VS\(_2\)'s 3D shape is not compatible with a homogeneous triaxial body in hydrostatic equilibrium, but it might be a differentiated body and/or might be sustaining some stress. No secondary features related to rings or material orbiting around VS\(_2\) were detected.</description><subject>Albedo</subject><subject>Amplitudes</subject><subject>Chords (geometry)</subject><subject>Equivalence</subject><subject>Light curve</subject><subject>Observatories</subject><subject>Stellar occultation</subject><subject>Trans-Neptunian 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J</creatorcontrib><creatorcontrib>Frasca, A</creatorcontrib><creatorcontrib>Szabó, G M</creatorcontrib><creatorcontrib>Derekas, A</creatorcontrib><creatorcontrib>Szigeti, L</creatorcontrib><creatorcontrib>Drozdz, M</creatorcontrib><creatorcontrib>Ogloza, W</creatorcontrib><creatorcontrib>J Skvar\u{c}</creatorcontrib><creatorcontrib>Ciabattari, F</creatorcontrib><creatorcontrib>Delincak, P</creatorcontrib><creatorcontrib>P Di Marcantonio</creatorcontrib><creatorcontrib>Iafrate, G</creatorcontrib><creatorcontrib>Coretti, I</creatorcontrib><creatorcontrib>Baldini, V</creatorcontrib><creatorcontrib>Baruffetti, P</creatorcontrib><creatorcontrib>Klös, O</creatorcontrib><creatorcontrib>Dumitrescu, V</creatorcontrib><creatorcontrib>Mikuž, H</creatorcontrib><creatorcontrib>Mohar, A</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>ProQuest - Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Vara-Lubiano, M</au><au>Benedetti-Rossi, G</au><au>Santos-Sanz, P</au><au>Ortiz, J L</au><au>Sicardy, B</au><au>Popescu, M</au><au>Morales, N</au><au>Rommel, F L</au><au>Morgado, B</au><au>Pereira, C L</au><au>Álvarez-Candal, A</au><au>Fernández-Valenzuela, E</au><au>Souami, D</au><au>Ilic, D</au><au>Vince, O</au><au>Bachev, R</au><au>Semkov, E</au><au>Nedelcu, D A</au><au>A \c{S}onka</au><au>Hudin, L</au><au>Boaca, M</au><au>Inceu, V</au><au>Curelaru, L</au><au>Gherase, R</au><au>Turcu, V</au><au>Moldovan, D</au><au>Mircea, L</au><au>Predatu, M</au><au>Teodorescu, M</au><au>Stoian, L</au><au>Juravle, A</au><au>Braga-Ribas, F</au><au>Desmars, J</au><au>Duffard, R</au><au>Lecacheux, J</au><au>Camargo, J I B</au><au>Assafin, M</au><au>Vieira-Martins, R</au><au>Pribulla, T</au><au>Husárik, M</au><au>Sivanič, P</au><au>Pal, A</au><au>Szakats, R</au><au>Kiss, C</au><au>Alonso-Santiago, J</au><au>Frasca, A</au><au>Szabó, G M</au><au>Derekas, A</au><au>Szigeti, L</au><au>Drozdz, M</au><au>Ogloza, W</au><au>J Skvar\u{c}</au><au>Ciabattari, F</au><au>Delincak, P</au><au>P Di Marcantonio</au><au>Iafrate, G</au><au>Coretti, I</au><au>Baldini, V</au><au>Baruffetti, P</au><au>Klös, O</au><au>Dumitrescu, V</au><au>Mikuž, H</au><au>Mohar, A</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>The multichord stellar occultation on 2019 October 22 by the trans-Neptunian object (84922) 2003 VS\(_2\)</atitle><jtitle>arXiv.org</jtitle><date>2022-05-25</date><risdate>2022</risdate><eissn>2331-8422</eissn><abstract>We predicted, observed, and analyzed the multichord stellar occultation of the Second Gaia Data Release (Gaia DR2) source 3449076721168026624 (m\(_v\) = 14.1 mag) by the plutino object 2003 VS\(_2\) (hereafter, VS\(_2\)) on 2019 October 22. We also carried out photometric observations to derive the rotational light curve amplitude and rotational phase of VS\(_2\) during the stellar occultation. Combining the results and assuming a triaxial shape, we derived the 3D shape of VS\(_2\). Out of the 39 observatories involved in the observational campaign, 12 sites reported a positive detection; this makes it one of the best observed stellar occultations by a TNO so far. We obtained a rotational light curve amplitude of \({\Delta}\)m = 0.264 \(\pm\) 0.017 mag, a mean area-equivalent diameter of D\(_{A_{eq}}\) = 545 \(\pm\) 13 km, and a geometric albedo of 0.134 \(\pm\) 0.010. The best triaxial shape obtained for VS\(_2\) has semiaxes a = 339 \(\pm\) 5 km, b = 235 \(\pm\) 6 km, and c = 226 \(\pm\) 8 km. The derived aspect angle is \({\theta}\) = 59\({\deg} \pm\) 2\({\deg}\) or its supplementary \({\theta}\) = 121\({\deg} \pm\) 2\({\deg}\), depending on the north-pole position. The spherical-volume equivalent diameter is D\(_{V_{eq}}\) = 524 \(\pm\) 7 km. If we consider large albedo patches on its surface, the semi-major axis of the ellipsoid could be ~10 km smaller. These results are compatible with the previous ones determined from the single-chord 2013 and four-chord 2014 stellar occultations and with the effective diameter and albedo derived from Herschel and Spitzer data. They provide evidence that VS\(_2\)'s 3D shape is not compatible with a homogeneous triaxial body in hydrostatic equilibrium, but it might be a differentiated body and/or might be sustaining some stress. No secondary features related to rings or material orbiting around VS\(_2\) were detected.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2205.12878</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2022-05 |
issn | 2331-8422 |
language | eng |
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source | Open Access: Freely Accessible Journals by multiple vendors |
subjects | Albedo Amplitudes Chords (geometry) Equivalence Light curve Observatories Stellar occultation Trans-Neptunian objects |
title | The multichord stellar occultation on 2019 October 22 by the trans-Neptunian object (84922) 2003 VS\(_2\) |
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