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An Irregular Shape of the Jupiter Trojan (3317) Paris Revealed by Stellar Occultations and Rotational Light Curves

  • Authors: Luan M. Catani, Bruno E. Morgado, Eros Gradovski, Pablo Santos-Sanz, Bruno Sicardy, Felipe Braga-Ribas, Gustavo Benedetti-Rossi, Roberto Vieira-Martins, José-Luis Ortiz, Flavia L. Rommel, Altair R. Gomes-Júnior, Yucel Kilic, Josselin Desmars, Marcelo Assafin, Rodrigo Boufleur, Chrystian L. Pereira, Giuliano Margoti, Juan Luis Rizos, Toshio Hirose, Miyoshi Ida, Júlio I. B. Camargo, Jonatã Arcas-Silva, Viviane F. Peixoto, Hélio Dutra, Damya Souami, Rafael Sfair, Thamiris de Santana, Tiago F. L. L. Pinheiro, Luana Liberato, Patrícia B. Siqueira, George L. Hashimoto, Norihiro Manago, Hideki Yoshihara, David Oesper, Joan Aragonès, David L. Aznar, Jerry Bardecker, Kirk Bender, Michel Boutet, Silvia C. Belloc, Ricard Casas, Oscar Canales-Moreno, Jean-Louis Dumont, Gregor Krannich, Pierre Le Cam, Arnaud Leroy, Steve Messner, Waldemar Ogłoza, Lionel Rousselot, Carles Schnabel, Julio Spagnotto, Adrianus Verveen

Luan M. Catani et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 8.

Fit positions of the shape model to the astrometric solutions of the multichord occultation events. Dashed lines represent the model uncertainties. The positions are provided relative to the NIMA v10 ephemeris (J. Desmars et al. 2015).

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