1. Physical Characteristics of Jupiter's Trojan (1437) Diomedes from a Tri-chord Stellar Occultation in 2020 and Dimensionless 3D Model
- Author
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Dutra, H., Assafin, M., Sicardy, B., Ortiz, J. L., Gomes-Júnior, A. R., Morgado, B. E., Benedetti-Rossi, G., Braga-Ribas, F., Margoti, G., Gradovski, E., Camargo, J. I. B., Boufleur, R., Vieira-Martins, R., Desmars, J., Oesper, D., Bender, K., Kitting, C., and Nolthenius, R.
- Subjects
Astrophysics - Earth and Planetary Astrophysics - Abstract
Jupiter Trojans preserve primitive formation characteristics due to their collisionless stable orbits. Determination of their shapes and size-frequency distribution constrains the collisional evolution of their parent population which also originated the Kuiper Belt. We started a program to find precise sizes/shapes for Trojans, combining stellar occultations and DAMIT 3D shape models. We report results for Diomedes, by fitting its dimensionless 3D model to 3 chords of a stellar occultation observed in 2020, using iterative $\chi^{2}$ procedures. The pole coordinates, rotation period, volume-equivalent radius and geometric albedo were: $\lambda$ = 153.73$^{o}$ $\pm$ 2.5$^{o}$, $\beta$ = 12.69$^{o}$ $\pm$ 2.6$^{o}$, $P$ = 24.4984 $\pm$ 0.0002 h, $R_{eq}$ = 59.4 $\pm$ 0.3 km and $p_{V}$ = 0.030 $\pm$ 0.004. A precise position was obtained too., Comment: 14 pages, 6 figures, 7 tables
- Published
- 2024