Degeneracy in the characterization of non-transiting planets from transit timing variations
Gwena\"el Bou\'e, Mahmoudreza Oshagh, Marco Montalto, Nuno C. Santos

TL;DR
This paper investigates the challenges in characterizing non-transiting planets using transit timing variations, highlighting degeneracies near mean-motion resonances that hinder precise parameter determination.
Contribution
It provides an analysis of TTV signals near MMRs, revealing degeneracies that complicate planetary parameter inference and detection.
Findings
TTV signals are quasiperiodic near MMRs with dominant long periods.
Degeneracy occurs when TTV residuals are too weak to detect.
Detecting Earth-mass planets is possible but not definitive near MMRs.
Abstract
The transit timing variation (TTV) method allows the detection of non-transiting planets through their gravitational perturbations. Since TTVs are strongly enhanced in systems close to mean-motion resonances (MMR), even a low mass planet can produce an observable signal. This technique has thus been proposed to detect terrestrial planets. In this letter, we analyse TTV signals for systems in or close to MMR in order to illustrate the difficulties arising in the determination of planetary parameters. TTVs are computed numerically with an n-body integrator for a variety of systems close to MMR. The main features of these TTVs are also derived analytically. Systems deeply inside MMR do not produce particularly strong TTVs, while those close to MMR generate quasiperiodic TTVs characterised by a dominant long period term and a low amplitude remainder. If the remainder is too weak to be…
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