Planetesimal Capture by an Evolving Jupiter

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-Two-body system- Uniform distributionof planetesimals1km-V = 1 km/s- No interaction withProto-JupiterMass (gr)10km-No planetesimal isejected.100kmTime (years)Helled, Podolak, Kovetz (2006)

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• Jupiter-mass envelope/clump• Initial radius = 0.5 AU• Duration of contraction = 2.71 x 10 5 years0.5 AUIncreasing temp.& density

Page 3 and 4: Motivation• Gravitational perturb
Page 5: Jupiter-massclump0.5 AUIncreasing t
Page 9 and 10: • 3600 Planetesimal• Size = 1,
Page 11 and 12: 3.7 AU Σ = r -3/26.6 AU
Page 13 and 14: Dynamical Breakup1Pdyn = ! v22(Ram
Page 15 and 16: 3.7 AU Σ = r -3/26.6 AU
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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