Paper

A large topographic feature on the surface of the trans-Neptunian object (307261) 2002 MS\\(_4\\) measured from stellar occultations

Lecacheux, J, Castro-Tirado, A J, Albanese, D, Danescu, C A, Bacci, R, Kozhukhov, O M, Rousselot, L, Bacci, P, Stoian, L, Hopp, U, Fuentes, C, Dumitru, B D, Conjat, M, Montigiani, N, Sickafoose, A A, Tsamis, V, Tagliaferri, U, D Baba Aissa, Kalkan, S, Lavayssière, M, Anghel, R M, Sonbas, E, Rengstorf, A W, Licandro, J, Gonçalves, R, Renner, S, Alarcon, M R, Pereira, C L, Vara-Lubiano, M, Rodríguez-Marco, M, Gowe, B, Trigo-Rodríguez, J M, Gillon, M, Lekkas, G, de la Cueva, I, Juravle, A, Sota, A, Marciniak, A, Moravec, Z, Bento, M, Succi, G, Klös, O, J -F Gout, Ogloza, W, Ruocco, N, Pál, A, Behem, R, Pribulla, T, Mariey, H, Vieira-Martins, R, Schmitz, C J, Kubánek, J, Krugly, Y, Wake, D A, Meister, S, Dumitrescu, V, Desmars, J, Sybilski, P Waldemar, Klotz, A, Komžík, R, Delinčák, P, Duffard, R, Hudin, L, Husárik, M, Fisher, R S, Tomko, D, Catanzaro, G, Mammana, L A, Nardiello, D, Tekeş, M, Belskaya, I, Schnabel, C, Calvo-Fernández, J F, Sánchez-Lavega, A, Collins, M, Frasca, A, Hueso, R, Morgado, B E, Müller, T G, Canales-Moreno, O, Sicardy, B, Schnabel, M, Boutet, M, Bagiran, M N, M Bachini, Cikota, S, Ferreira, M, de Santana, T, Eryilmaz, S, Tigani, K, Vîntdeva

2023

Overview

This work aims at constraining the size, shape, and geometric albedo of the dwarf planet candidate 2002 MS4 through the analysis of nine stellar occultation events. Using multichord detection, we also studied the object's topography by analyzing the obtained limb and the residuals between observed chords and the best-fitted ellipse. We predicted and organized the observational campaigns of nine stellar occultations by 2002 MS4 between 2019 and 2022, resulting in two single-chord events, four double-chord detections, and three events with three to up to sixty-one positive chords. Using 13 selected chords from the 8 August 2020 event, we determined the global elliptical limb of 2002 MS4. The best-fitted ellipse, combined with the object's rotational information from the literature, constrains the object's size, shape, and albedo. Additionally, we developed a new method to characterize topography features on the object's limb. The global limb has a semi-major axis of 412 \\(\\pm\\) 10 km, a semi-minor axis of 385 \\(\\pm\\) 17 km, and the position angle of the minor axis is 121 \\(^\\circ\\) \\(\\pm\\) 16\\(^\\circ\\). From this instantaneous limb, we obtained 2002 MS4's geometric albedo and the projected area-equivalent diameter. Significant deviations from the fitted ellipse in the northernmost limb are detected from multiple sites highlighting three distinct topographic features: one 11 km depth depression followed by a 25\\(^{+4}_{-5}\\) km height elevation next to a crater-like depression with an extension of 322 \\(\\pm\\) 39 km and 45.1 \\(\\pm\\) 1.5 km deep. Our results present an object that is \\(\\approx\\)138 km smaller in diameter than derived from thermal data, possibly indicating the presence of a so-far unknown satellite. However, within the error bars, the geometric albedo in the V-band agrees with the results published in the literature, even with the radiometric-derived albedo.

• Publisher: Cornell University Library, arXiv.org
• Subject: Albedo / Chords (geometry) / Diameters / Dwarf planets / Extrasolar planets / Stellar occultation / Topography / Trans-Neptunian objects