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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 4.

Fit of the 3D shape model of Paris to the stellar occultation data. Cyan lines represent positive chords, with red segments indicating their uncertainty regions. The dashed black line corresponds to a near-limb negative chord. Dashed red contours around the limb denote the model error at ±1σ (in kilometers). Red and blue lines extending outside the shape illustrate the orientation of the spin axis.

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