The multichord stellar occultation on 2019 October 22 by the trans-Neptunian object (84922) 2003 VS$_2$
M. Vara-Lubiano, G. Benedetti-Rossi, P. Santos-Sanz, J. L. Ortiz, B., Sicardy, M. Popescu, N. Morales, F. L. Rommel, B. Morgado, C. L. Pereira, A., \'Alvarez-Candal, E. Fern\'andez-Valenzuela, D. Souami, D. Ilic, O. Vince, R., Bachev, E. Semkov, D. A. Nedelcu, A. \c{S}onka

TL;DR
This study used a multichord stellar occultation and photometry to determine the 3D shape, size, and surface properties of trans-Neptunian object (84922) 2003 VS2, providing detailed physical characterization and insights into its internal structure.
Contribution
First detailed 3D shape and size determination of VS2 using multichord occultation data combined with photometry, revealing its non-homogeneous structure and surface features.
Findings
Mean diameter of 545 km with 13 km uncertainty
Best-fit triaxial shape with axes a=339 km, b=235 km, c=226 km
No rings or orbiting material detected around VS2
Abstract
We predicted, observed, and analyzed the multichord stellar occultation of the Second Gaia Data Release (Gaia DR2) source 3449076721168026624 (m = 14.1 mag) by the plutino object 2003 VS (hereafter, VS) on 2019 October 22. We also carried out photometric observations to derive the rotational light curve amplitude and rotational phase of VS during the stellar occultation. Combining the results and assuming a triaxial shape, we derived the 3D shape of VS. 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 m = 0.264 0.017 mag, a mean area-equivalent diameter of D = 545 13 km, and a geometric albedo of 0.134 0.010. The best triaxial shape obtained…
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