Dynamical Interactions in the Planetary System GJ4276
Fergus Horrobin, Hanno Rein

TL;DR
This study reanalyzes RV data of GJ4276, suggesting the presence of a second planet in a mean motion resonance, with system stability confirmed through dynamical modeling, highlighting the importance of resonances in planet formation.
Contribution
The paper provides a dynamical analysis of GJ4276, identifying potential resonant configurations and stability regions, which advances understanding of multi-planet interactions in this system.
Findings
Possible two-planet resonant configurations identified
System likely in a first order mean motion resonance
Stable orbital solutions confirmed via MEGNO analysis
Abstract
GJ4276 is an M4.0 dwarf star with an inferred Neptune mass planet from radial velocity (RV) observations. We reanalyse the RV data for this system and focus on the possibility of a second, super earth mass, planet. We compute the timescale for fast resonant librations in the eccentricity to be . Given that the observations were taken over , we expect to see the effect of these librations in the observations. We perform a fully dynamical fit to test this hypothesis. Similar to previous results, we determine that the data could be fit by two planets in a 2:1 mean motion resonance. However, we also find solutions near the 5:4 mean motion resonance which are not present when planet-planet interactions are ignored. Using the MEGNO indicator, we analyze the stability of the system and find that our solutions lie in a stable region of parameter…
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