More Likely Than You Think: Inclination-Driving Secular Resonances are Common in Known Exoplanet Systems
Thea Faridani, Smadar Naoz, Gongjie Li, Malena Rice, Nicholas Inzunza

TL;DR
This paper investigates how inclination-driving secular resonances, influenced by stellar oblateness decay, are common in known three-planet exoplanet systems and affect their detectability and stability.
Contribution
It demonstrates that secular resonances driven by stellar oblateness decay are prevalent in known exoplanet systems, impacting their mutual inclinations and detection prospects.
Findings
Approximately 20% of studied systems undergo early secular resonances.
Resonances significantly affect planetary mutual inclinations and detection likelihood.
Stellar oblateness decay expands resonance regions in parameter space.
Abstract
Multi-planet systems face significant challenges to detection. For example, further orbiting planets have reduced signal-to-noise ratio in radial velocity detection methods, and small mutual inclinations between planets can prevent them from all transiting. One mechanism to excite mutual inclination between planets is secular resonance, where the nodal precession frequencies of the planets align such as to greatly increase the efficiency of angular momentum transport between planets. These resonances can significantly misalign planets from one another, hindering detection, and typically can only occur when there are three or more planets in the system. Naively, systems can only be in resonance for particular combinations of planet semimajor axes and masses; however, effects that alter the nodal precession frequencies of the planets, such as the decay of stellar oblateness, can…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research
