Planetesimal Capture by an Evolving Jupiter

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• Aerodynamic heatingHeating• Radiation from ambient atmosphere1E D= "!v2E = !4atmT atm3Cooling• Radiative cooling• Evaporative coolingE = !E4radT surfvap=qPvap( Tsurf)µ2!N kTAsurf

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• Aerodynamic heatingHeating• Radiation from ambient atmosphere1E D= "!v2E = !4atmT atm3Cooling• Radiative cooling• Evaporative coolingE = !E4radT surfvap=qPvap( Tsurf)µ2!N kTAsurf

3.7 AU Σ = r -3/26.6 AU

Page 3 and 4: Motivation• Gravitational perturb
Page 5 and 6: Jupiter-massclump0.5 AUIncreasing t
Page 7 and 8: • Jupiter-mass envelope/clump•
Page 9 and 10: • 3600 Planetesimal• Size = 1,
Page 11 and 12: 3.7 AU Σ = r -3/26.6 AU
Page 13: Dynamical Breakup1Pdyn = ! v22(Ram
Page 17 and 18: 100km
Page 19 and 20: 100km10km1km
Page 21 and 22: Radius Loss (km)Time (yr)
Page 23: Conclusions and Future Work- Smalle

Planetesimal Capture by an Evolving Jupiter

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