Orbital Perturbations of the Galilean Satellites During Planetary Encounters

Abstract

The Nice model of the dynamical instability and migration of the giant planets can explain many properties of the present Solar System, and can be used to constrain its early architecture. In the jumping-Jupiter version of the Nice model, required from the terrestrial planet constraint and dynamical structure of the asteroid belt, Jupiter has encounters with an ice giant. Here we study the survival of the Galilean satellites in the jumping-Jupiter model. This is an important concern because the ice-giant encounters, if deep enough, could dynamically perturb the orbits of the Galilean satellites, and lead to implausible results. We performed numerical integrations where we tracked the effect of planetary encounters on the Galilean moons. We considered three instability cases from Nesvorny & Morbidelli (2012) that differed in the number and distribution of encounters. We found that in one case, where the number of close encounters was relatively small, the Galilean satellite orbits were not significantly affected. In the other two, the orbital eccentricities of all moons were excited by encounters, Callisto's semimajor axis changed, and, in a large fraction of trials, the Laplace resonance of the inner three moons was disrupted. The subsequent evolution by tides damps eccentricities and can recapture the moons in the Laplace resonance. A more important constraint is represented by the orbital inclinations of the moons, which can be excited during the encounters and not appreciably damped by tides. We find that one instability case taken from Nesvorny & Morbidelli (2012) clearly fails this constraint. This shows how the regular satellites of Jupiter can be used to set limits on the properties of encounters in the jumping-Jupiter model, and help us to better understand how the early Solar System evolved.

The Astronomical Journal, in press

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Cited by in corpus (30)

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• The excitation of a primordial cold asteroid belt as an outcome of the planetary instability
• On the contribution of PRIDE-JUICE to Jovian system ephemerides
• Born eccentric: constraints on Jupiter and Saturn's pre-instability orbits
• Saturn's formation and early evolution at the origin of Jupiter's massive moons
• The formation of the Galilean moons and Titan in the Grand Tack scenario
• Jumping Jupiter can explain Mercury's orbit
• Long-term evolution of the Galilean satellites: the capture of Callisto into resonance
• Exomoon Climate Models with the Carbonate-Silicate Cycle and Viscoelastic Tidal Heating
• Could Jupiter or Saturn Have Ejected a Fifth Giant Planet?
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• On the Detection of Extrasolar Moons and Rings
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• Can a jumping-Jupiter trigger the Moon's formation impact?
• Thermal and orbital evolution of low-mass exoplanets
• Cladistical analysis of the Jovian and Saturnian satellite systems
• Rethinking the role of the giant planet instability in terrestrial planet formation models
• Mercury's formation within the Early Instability Scenario
• The origin of Neptune's unusual satellites from a planetary encounter
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• Contribution of PRIDE VLBI products to the joint JUICE-Europa Clipper moons' ephemerides solution
• Capture of satellites during planetary encounters A case study of the Neptunian moons Triton and Nereid
• iSyMBA: A Symplectic Massive Bodies Integrator with Planets Interpolation
• The formation of transiting circumplanetary debris discs from the disruption of satellite systems during planet-planet scattering
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