Study of the Plutino Object (208996) 2003 AZ(84) from Stellar Occultations: Size, Shape, and Topographic Features | |
Dias-Oliveira, A.1; Sicardy, B.2; Ortiz, J. L.3; Braga-Ribas, F.1,4; Leiva, R.2,5; Vieira-Martins, R.1,6,7; Benedetti-Rossi, G.1; Camargo, J. I. B.1,7; Assafin, M.8; Gomes-Junior, A. R.8; Baug, T.9; Chandrasekhar, T.9; Desmars, J.2; Duffard, R.3; Santos-Sanz, P.3; Zhao EG(赵二刚)10; Ganesh, S.9; Ikari, Y.11; Irawati, P.12; Jain, J.9; Zhu LY(朱俐颖)10; Richichi, A.12; Qian SB(钱声帮)10; Behrend, R.13; Benkhaldoun, Z.14; Brosch, N.15; Daassou, A.14; Frappa, E.16; Gal-Yam, A.17; Garcia-Lozano, R.18; Gillon, M.19; Jehin, E.19; Kaspi, S.15; Klotz, A.20; Lecacheux, J.2; Mahasena, P.21; Manfroid, J.19; Manulis, I.17; Maury, A.22; Mohan, V.23; Morales, N.3; Ofek, E.17; Rinner, C.24; Sharma, A.25; Sposetti, S.13; Tanga, P.26; Thirouin, A.27; Vachier, F.6; Widemann, T.2; Asai, A.11; Hayato, Watanabe11; Hiroyuki, Watanabe11; Owada, M.11; Yamamura, H.11; Hayamizu, T.11; Bradshaw, J.28,29; Kerr, S.30; Tomioka, H.36; Andersson, S.31; Dangl, G.32; Haymes, T.33; Naves, R.34; Wortmann, G.35 | |
发表期刊 | ASTRONOMICAL JOURNAL |
2017-07-01 | |
卷号 | 154期号:1 |
DOI | 10.3847/1538-3881/aa74e9 |
产权排序 | 第10完成单位 |
收录类别 | SCI |
关键词 | Kuiper Belt Objects: Individual (208996, 2003az84) Occultations Planets And Satellites: Fundamental Parameters Planets And Satellites: Surfaces |
摘要 | We present results derived from four stellar occultations by the plutino object (208996) 2003. AZ(84), detected on 2011 January 8 (single-chord event), 2012 February 3 (multi-chord), 2013 December 2 (single-chord), and 2014 November 15 (multi-chord). Our observations rule out an oblate spheroid solution for 2003. AZ(84)'s shape. Instead, assuming hydrostatic equilibrium, we find that a Jacobi triaxial solution with semiaxes (470 +/- 20) x (383 +/- 10) x (245 +/- 8) km can better account for all our occultation observations. Combining these dimensions with the rotation period of the body (6.75 hr) and the amplitude of its rotation light curve, we derive a density rho = 0.87 +/- 0.01g cm(-3), a geometric albedo p(V) = 0.097 +/- 0.009. A grazing chord observed during the 2014 occultation reveals a topographic feature along 2003. AZ(84) ' s limb, which can be interpreted as an abrupt chasm of width similar to 23. km and depth >8 km, or a smooth depression of width similar to 80. km and depth similar to 13 km (or an intermediate feature between those two extremes). |
资助项目 | French grants "Beyond Neptune"[ANR-08-BLAN-0177] ; "Beyond Neptune II"[ANR-11-IS56-0002] ; European Research Council under the European Community's[H2020 (2014-2020/ERC] ; European Research Council under the European Community's[669416] ; CONICYT-PCHA/Doctorado[Nacional/2014-21141198] ; CAPES[BEX 9110/12-7] ; CAPES[203.173/2016] ; FAPERJ/PAPDRJ[E-45/2013] ; FAPERJ/PAPDRJ[E26/200.464/2015227833] ; European Union's Horizon Research and Innovation Programme[687378] ; CNPq[306885/2013] ; CNPq[473002/2013-2] ; CNPq[308721/ 2011-0] ; Capes/Cofecub[2506/2015] ; Faperj[PAPDRJ-45/2013] ; Faperj[E-26/203.026/2015] ; Faperj[E-26/111.488/2013] ; CNPq/PQ2 fellowship[308489/ 2013-6] ; Searchlight Observatory Network Funding from Spanish[AYA-2014-56637-C2-1-P] ; Proyecto de Excelencia de la Junta de Andaluca[JA 2012FQM1776] ; Lowell Observatory |
项目资助者 | French grants "Beyond Neptune"[ANR-08-BLAN-0177] ; "Beyond Neptune II"[ANR-11-IS56-0002] ; European Research Council under the European Community's[H2020 (2014-2020/ERC, 669416] ; CONICYT-PCHA/Doctorado[Nacional/2014-21141198] ; CAPES[BEX 9110/12-7, 203.173/2016] ; FAPERJ/PAPDRJ[E-45/2013, E26/200.464/2015227833] ; European Union's Horizon Research and Innovation Programme[687378] ; CNPq[306885/2013, 473002/2013-2, 308721/ 2011-0] ; Capes/Cofecub[2506/2015] ; Faperj[PAPDRJ-45/2013, E-26/203.026/2015, E-26/111.488/2013] ; CNPq/PQ2 fellowship[308489/ 2013-6] ; Searchlight Observatory Network Funding from Spanish[AYA-2014-56637-C2-1-P] ; Proyecto de Excelencia de la Junta de Andaluca[JA 2012FQM1776] ; Lowell Observatory |
语种 | 英语 |
学科领域 | 天文学 ; 恒星与银河系 |
文章类型 | Article |
出版者 | IOP PUBLISHING LTD |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
ISSN | 0004-6256 |
URL | 查看原文 |
WOS记录号 | WOS:000404755100001 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | Trans-neptunian Objects ; Short-term Variability ; Solar-system ; 2060 Chiron ; Albedo ; Radius ; Planet ; Centaurs |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/10153 |
专题 | 双星与变星研究组 |
通讯作者 | Dias-Oliveira, A. |
作者单位 | 1.Observatório Nacional/MCTI, Rua General José Cristino 77, Rio de Janeiro—RJ, 20.921-400, Brazil 2.LESIA/Observatoire de Paris, CNRS UMR 8109, Université Pierre et Marie Curie, Université Paris-Diderot, 5 place Jules Janssen, F-92195 Meudon Cédex, France 3.Instituto de Astrofísica de Andalucía-CSIC, Apt 3004, E-18080, Granada, Spain 4.Federal University of Technology—Paraná (UTFPR/DAFIS), R. Sete de Setembro 3165, Curitiba—PR, 80230-901, Brazil 5.Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 7820436 Macul, Santiago, Chile 6.IMCCE/Observatorie de Paris, 77 Avenue Denfert Rochereau, Paris, F-75014, France 7.Laboratório Interinstitucional de e-Astronomia—LIneA, Rua General José Cristino 77, Rio de Janeiro—RJ, 20.921-400, Brazil 8.Observatório do Valongo/UFRJ, Ladeira Pedro Antonio 43, Rio de Janeiro—RJ, 20080-090, Brazil 9.Physical Research Laboratory, Ahmedabad, Gujarat 380009, India 10.Yunnan Observatories, Chinese Academy of Sciences, Yunnan, China 11.Japan Occultation Information Network (JOIN), Japan 12.National Astronomical Research Institute of Thailand, Siriphanich Building, Chiang Mai 50200, Thailand 13.Observatoire de Genève, 1290 Versoix, Switzerland 14.Oukaimeden Observatory, LPHEA, Cadi Ayyad University, Morocco 15.Wise Observatory and School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv 69978, Israel 16.EURASTER, 8 route de Soulomes, F-46240 Labastide-Murat, France 17.Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 7610001, Israel 18.Observatorio de Busot, Spain 19.Institut d'Astrophysique, de Géophysique et Océanographie, Université de Liège, Allée du 6 aohat ut 17, B-4000 Liége, Belgium 20.Université de Toulouse, UPS-OMP, IRAP, 14 Avenue Edouard Belin, F-31400 Toulouse, France 21.Observatorium Bosscha, Institut Teknologi Bandung, Indonesia 22.San Pedro de Atacama Celestial Explorations (S.P.A.C.E.), San Pedro de Atacama, Chile 23.IUCAA Girawali Observatory, India 24.Moroccan Oukaimeden Sky Survey, Morocco 25.Nikaya Observatory, Tamil Nadu 635114, India 26.Laboratoire Lagrange, UMR7293, Uni. Côte d'Azur, CNRS, Observatoire de la Côte d'Azur Boulevard de l'Observatoire, CS 34229, F-06304 Nice, France 27.Lowell Observatory, 1400 W Mars Hill Rd, Flagstaff, Arizona, USA 28.International Occultation Timing Association (IOTA), P.O. Box 7152, Kent, WA 98042, USA 29.Samford Valley Observatory, QLD, Australia 30.Royal Astronomical Society of New Zealand—Occultation Section, New Zealand 31.Amateursternwarte Mueggelheim, Wiesbacher Weg 8, D-12559 Berlin, Germany 32.A-3830, Nonndorf 12, Austria 33.BAA Asteroids and Remote Planets Section, Hill Rise, Knowl Hill Common, RG10 9YD, UK 34.c/Jaume Balmes n 24 Cabrils E-08348, Spain 35.Archenhold-Observatory, Neue Krugallee 180, D-12437 Berlin, Germany 36.Independent Astronomer. |
推荐引用方式 GB/T 7714 | Dias-Oliveira, A.,Sicardy, B.,Ortiz, J. L.,et al. Study of the Plutino Object (208996) 2003 AZ(84) from Stellar Occultations: Size, Shape, and Topographic Features[J]. ASTRONOMICAL JOURNAL,2017,154(1). |
APA | Dias-Oliveira, A..,Sicardy, B..,Ortiz, J. L..,Braga-Ribas, F..,Leiva, R..,...&Wortmann, G..(2017).Study of the Plutino Object (208996) 2003 AZ(84) from Stellar Occultations: Size, Shape, and Topographic Features.ASTRONOMICAL JOURNAL,154(1). |
MLA | Dias-Oliveira, A.,et al."Study of the Plutino Object (208996) 2003 AZ(84) from Stellar Occultations: Size, Shape, and Topographic Features".ASTRONOMICAL JOURNAL 154.1(2017). |
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