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20022006
most citedThe Librating Companions in HD 37124, HD 12661, HD 82943, 47 Uma and GJ 876: Alignment or Antialignment?

76 citations · 331 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph2006★ 55 cited

The Secular Evolution and Dynamical Architecture of the Neptunian Triplet Planetary System HD 69830

Ji Jianghui, H. Kinoshita, Liu Lin +1

We perform numerical simulations to study the secular orbital evolution and dynamical structure in the HD 69830 system with the best-fit orbital solutions by Lovis and coworkers (2…

astro-ph2005★ 62 cited

Could the 47 UMa Planetary System be a Second Solar System: predicting the Earth-like planets

Jianghui Ji, Lin Liu, H. Kinoshita +1

(Abridged)We numerically investigated the dynamical architecture of 47 UMa with the planetary configuration of the best-fit orbital solutions by Fischer et al. We systematically st…

gr-qc2005★ 9 cited

Constraint on intermediate-range gravity from earth-satellite and lunar orbiter measurements, and lunar laser ranging

Guangyu Li, Haibin Zhao

In the experimental tests of gravity, there have been considerable interests in the possibility of intermediate-range gravity. In this paper, we use the earth-satellite measurement…

astro-ph2003★ 76 cited

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

Jianghui Ji, Lin Liu, H. Kinoshita +3

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 aps…

astro-ph2003★ 55 cited

The Apsidal Antialignment of the HD 82943 System

Ji Jianghui, H. Kinoshita, Liu Lin +2

We perform numerical simulations to explore the dynamical evolution of the HD 82943 planetary system. By simulating diverse planetary configurations, we find two mechanisms of stab…

astro-ph2003★ 74 cited

Could the 55 Cancri Planetary System Really Be in the 3:1 Mean Motion Resonance?

Ji Jianghui, H. Kinoshita, Liu Lin +1

We integrate the orbital solutions of the planets orbiting 55 Cnc. In the simulations, we find that not only three resonant arguments , $θ_{2}=λ_{1…