The limit of the gyrochronology - A new age determination technique: the tidal-chronology
Florian Gallet, Philippe Delorme

TL;DR
This paper introduces tidal-chronology, a new age estimation method for star-planet systems, addressing gyrochronology limitations caused by tidal interactions with close-in massive planets.
Contribution
The study develops a numerical model to define the applicability limits of gyrochronology and proposes tidal-chronology as a novel age determination technique for specific star-planet systems.
Findings
Gyrochronology is limited for stars with significant tidal interactions.
Tidal-chronology uses stellar rotation period and planetary semi-major axis for age estimation.
Applicable to stars 0.3-1.2 solar masses with massive close-in planets.
Abstract
While the number of detected planets is continuously increasing since 1995, their impact on their central star still remain poorly understood. Yet, the presence of a massive close-in planet can strongly modify the surface angular velocity evolution of the star. In these circumstances, age estimation techniques based on rotation, such as the gyrochronology, can't be applied to stars that experienced significant star-planet magnetic and tidal interactions during their evolution. With the use of a numerical model that combines an angular momentum evolution and an orbital evolution code, we investigated the evolution of initial distribution of star-planet systems, in which the orbital evolution of the planet is driven by the tidal dissipation formalism. Based on these initial distributions we highlighted the limits of applicability of the gyrochronology analysis and proposed a new age…
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Taxonomy
TopicsGeomagnetism and Paleomagnetism Studies · Geology and Paleoclimatology Research · Maritime and Coastal Archaeology
