Daphnis' Chaotic Orbit

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EPSC Abstracts Vol. 13, EPSC-DPS2019-1085-1, 2019 EPSC-DPS Joint Meeting 2019 c Author(s) 2019. CC Attribution 4.0 license. Daphnis’ Chaotic Orbit Thamiris Santana (1), Radwan Tajeddine (2), Maryame El Moutamid (2), Philip D. Nicholson (2) and Othon Winter (1) (1) UNESP Sao Paulo State University, Sao Paulo, Brazil ([email protected]), (2) Cornell University, New York, USA 1 Daphnis’ discovery Cassini has changed our knowledge about Saturn sys- tem with its discoveries. One of those is Daphnis, an almost 8 km in size moon, orbiting inside the Keeler gap. Its existence was inferred from to the observation of waves in the edge of the gap, and from a images taken by Cassini in 2005 the moon was resolved. Figure 1: Daphnis residual longitude relative to a cir- 2 Orbital motion cular orbit. The dots are the astrometric data and the lines indicate the expected longitude. After the discovery, image sequences taken at different epochs of Cassini mission were used to derive Daph- 4 Numerical integration nis’ orbit. Through a preliminary longitudinal analy- sis based on Cassini astrometry, it was noted that the To analyze the orbital evolution of Daphnis, we per- longitude of Daphnis did not match the expected posi- formed numerical simulations taking into account the tion when considering a propagation of its initial orbit. gravity field of Saturn (with its gravitational harmonics Here we aim to improve the astrometric data to follow up to J6), the perturbation of the nearby satellites At- the satellite orbit in order to better understand Daph- las, Prometheus, Pandora and also Mimas. Our results nis’ movement. show that Daphnis is in a chaotic orbit due to more than one nearby resonances with the satellites Atlas and Prometheus. We also compute the Lyapunov indicator to verify 3 Astrometry the chaotic motion of the moon, and the estimated characteristic time is only few years. We first performed the astrometry of Daphnis based This is a new result about the puzzling motion of on Cassini’s Narrow Angle Camera images, covering Daphnis, contributing to understand why the satellite the period from 2006 to almost the end of the mis- changed orbit twice since its discovery by Cassini. sion. It was revealed that the satellite actually experienced two changes in semimajor axis during the times- pan that Daphnis was observed. Figure 1 shows the Acknowledgements residual longitude relative to a circular orbit with the This study was financed in part by the Coordenação de initial semimajor axis. The variation in the expected Aperfeiçoamento de Pessoal de Nível Superior - Brasil longitude can be related to changes in semimajor axis: (CAPES) - Finance Code 001 and FAPESP (Proc. an increase of ∆a = 107 m in 2010 and a drop of 2016/24561-0). The authors also thanks to Hartmann ∆a = 57 m in early 2016. These changes are large − Grant and Cassini Mission for the financial support. enough to not be attributed to errors in the orbit de- termination, therefore the satellite experienced some perturbation that altered its orbit at least twice during the Cassini time..

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