The dynamics of self-gravity wakes in the Mimas 5:3 bending wave: Modifying the linear theory
The satellite Mimas launches a bending wave – a warping of the rings that propagates radially through self-gravity – at the 5:3 inner vertical resonance with Saturn’s rings. We present a modification of the linear bending wave theory (Shu et al., 1983) which includes the effects of satellite self-gr...
Gespeichert in:
Veröffentlicht in: | Icarus (New York, N.Y. 1962) N.Y. 1962), 2024-05, Vol.413, p.115987, Article 115987 |
---|---|
Hauptverfasser: | , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
Zusammenfassung: | The satellite Mimas launches a bending wave – a warping of the rings that propagates radially through self-gravity – at the 5:3 inner vertical resonance with Saturn’s rings. We present a modification of the linear bending wave theory (Shu et al., 1983) which includes the effects of satellite self-gravity wakes on the particles in the wave. We show that, when treated as rigid, these wakes generate an extra layer of particles whose number density is proportional to the magnitude of the slope of the warped ring. Using a ray-tracing code we compare our predictions with those of Shu et al. (1983) and with 60 stellar occultations observed by the Cassini Ultraviolet Imaging Spectrograph (UVIS) and find that the extra layer of particles of our perturbed bending wave model has a considerable explanatory power for the UVIS dataset. Our best model explains the most discrepant and surprising features of the Mimas 5:3 bending wave; the enhancement of the signal for the cases of occultations with high ring opening angle and the bigger-than-expected viscosity, ν= 576 cm2/s, which is more than double the viscosity computed from density waves (Tiscareno et al., 2007). This shows that self-gravity wakes can be effective at transporting angular momentum in a vertically perturbed disk. Relative to neighboring density waves (Tiscareno et al., 2007), we find a lower-than-expected value for the surface mass density, σ= 36.7 g/cm2, which suggests that the enhanced viscous interactions may be transporting material into the surrounding regions.
•Modified wave theory matches the Cassini data significantly better than previous attempts.•Extra layer of particles explains most discrepant aspects between previous theory and data.•Bending waves enhances local viscosity up to a factor of 5, this can have secular dynamical effects.•The local viscosity enhancement occurs due to the self-gravity wake-bending wave interaction.•The obtained surface mass density is smaller than others in the region, suggesting mass transport. |
---|---|
ISSN: | 0019-1035 1090-2643 |
DOI: | 10.1016/j.icarus.2024.115987 |