The Librating Companions in HD 37124, HD 12661, HD 82943, 47 Uma and GJ 876: Alignment or Antialignment?

Abstract

We investigated the apsidal motion for the multi-planet systems. In the simulations, we found that the two planets of HD 37124, HD 12661, 47 Uma and HD 82943 separately undergo apsidal alignment or antialignment. But the companions of GJ 876 and $\upsilon$ And are only in apsidal lock about $0^{\circ }$. Moreover, we obtained the criteria with Laplace-Lagrange secular theory to discern whether a pair of planets for a certain system are in libration or circulation.

13 Pages, 3 figures, 2 tables, Published by ApJ Letters, 591, July 1, 2003 (Figures now included to match the publication)

References in corpus (11)

• Planet Migration and Binary Companions: the case of HD 80606b
• A Planet at 5 AU Around 55 Cancri
• The Dynamical Simulations of the Planets Orbiting GJ 876
• A dynamical mechanism for establishing apsidal resonance
• Apsidal Alignment in Upsilon Andromedae
• Could the 55 Cancri Planetary System Really Be in the 3:1 Mean Motion Resonance?
• Eccentricity Excitation and Apsidal Resonance Capture in the Planetary System Upsilon Andromedae
• A Dynamical Analysis of the 47 UMa Planetary System
• Eccentricity Evolution of Extrasolar Multiple Planetary Systems due to the Depletion of Nascent Protostellar Disks
• The Janus head of the HD 12661 planetary system
• Global dynamics and stability limits for planetary systems around HD 12661, HD 38529, HD 37124 and HD 160691

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