Physical properties of trans-Neptunian object (143707) 2003 UY117 derived from stellar occultation and photometric observations
M. Kretlow, J. L. Ortiz, J. Desmars, N. Morales, F. L. Rommel, P., Santos-Sanz, M. Vara-Lubiano, E. Fern\'andez-Valenzuela, A. Alvarez-Candal,, R. Duffard, F. Braga-Ribas, B. Sicardy, A. Castro-Tirado, E. J., Fern\'andez-Garc\'ia, M. S\'anchez, A. Sota, M. Assafin

TL;DR
This study combines stellar occultation and photometric data to determine the physical properties of TNO (143707) 2003 UY117, including size, shape, rotation, and albedo, enhancing understanding of primitive Solar System objects.
Contribution
It provides the first detailed physical characterization of this TNO by integrating occultation and photometry, revealing its 3D shape, size, rotation period, and surface reflectivity.
Findings
Projected ellipse axes: 282x184 km
Rotation period: 12.376 hours
Geometric albedo: 0.139
Abstract
Trans-Neptunian objects (TNOs) are considered to be among the most primitive objects in our Solar System. Knowledge of their primary physical properties is essential for understanding their origin and the evolution of the outer Solar System. We predicted a stellar occultation by this TNO for 2020 October 23 UT and ran a specific campaign to investigate this event. We derived the projected profile shape and size from the occultation observations by means of an elliptical fit to the occultation chords. We also performed photometric observations of (143707) 2003 UY117 to obtain the absolute magnitude and the rotational period from the observed rotational light curve. Finally, we combined these results to derive the three-dimensional shape, volume-equivalent diameter, and geometric albedo for this TNO. From the stellar occultation, we obtained a projected ellipse with axes of $(282 \pm…
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Taxonomy
TopicsAstro and Planetary Science
