Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in planets I. From the PMS to the RGB at solar metallicity

Abstract

Star-planet interactions must be taken into account in stellar models to understand the dynamical evolution of close-in planets. The dependence of the tidal interactions on the structural and rotational evolution of the star is of peculiar importance and should be correctly treated. We quantify how tidal dissipation in the convective envelope of rotating low-mass stars evolves from the pre-main sequence up to the red-giant branch depending on the initial stellar mass. We investigate the consequences of this evolution on planetary orbital evolution. We couple the tidal dissipation formalism described in Mathis (2015) to the stellar evolution code STAREVOL and apply it to rotating stars with masses between 0.3 and 1.4 M${}_{\odot }$. In addition, we generalize the work of Bolmont & Mathis (2016) by following the orbital evolution of close-in planets using the new tidal dissipation predictions for advanced phases of stellar evolution. On the PMS the evolution of tidal dissipation is controlled by the evolution of the internal structure of the contracting star. On the MS it is strongly driven by the variation of surface rotation that is impacted by magnetized stellar winds braking. The main effect of taking into account the rotational evolution of the stars is to lower the tidal dissipation strength by about four orders of magnitude on the main-sequence, compared to a normalized dissipation rate that only takes into account structural changes. The evolution of the dissipation strongly depends on the evolution of the internal structure and rotation of the star. From the pre-main sequence up to the tip of the red-giant branch, it varies by several orders of magnitude, with strong consequences for the orbital evolution of close-in massive planets. These effects are the strongest during the pre-main sequence, implying that the planets are mainly sensitive to the star's early history.

arXiv comment13 pages, 7 figures, accepted for publication in A&A

References in corpus (64)

• The chemical composition of the Sun
• MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models
• The K2 Mission: Characterization and Early results
• Detection of Planetary Transits Across a Sun-like Star
• The PLATO 2.0 Mission
• Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones
• Hot Stars with Hot Jupiters Have High Obliquities
• Architecture of Kepler's Multi-transiting Systems: II. New investigations with twice as many candidates
• Obliquities of Hot Jupiter host stars: Evidence for tidal interactions and primordial misalignments
• Tidal dissipation in stars and giant planets
• Tidal Evolution of Close-in Extra-Solar Planets
• Tidal dissipation in rotating giant planets
• Improved angular momentum evolution model for solar-like stars
• The Equilibrium-Tide Model for Tidal Friction
• Tidal dissipation in rotating solar-type stars
• Dearth of short-period Neptunian exoplanets - a desert in period-mass and period-radius planes
• Is tidal heating sufficient to explain bloated exoplanets? Consistent calculations accounting for finite initial eccentricity
• Testing a Predictive Theoretical Model for the Mass Loss Rates of Cool Stars
• The Orbital Evolution of Gas Giant Planets around Giant Stars
• The Mass-Dependence of Angular Momentum Evolution in Sun-Like Stars
• Thermohaline instability and rotation-induced mixing. III - Grid of stellar models and asymptotic asteroseismic quantities from the pre-main sequence up to the AGB for low- and intermediate-mass stars at various metallicities
• The accretion of planets and brown dwarfs by giant stars -- II. solar mass stars on the red giant branch
• On the tidal evolution of Hot Jupiters on inclined orbits
• Stellar Rotation Periods of the Kepler Objects of Interest: A Dearth of Close-in Planets around Fast Rotators
• The effect of magnetic topology on thermally-driven winds: towards a general formulation of the braking law
• Stellar Winds on the Main-Sequence II: the Evolution of Rotation and Winds
• Improved angular momentum evolution model for solar-like stars II. Exploring the mass dependence
• Distant future of the Sun and Earth revisited
• On the tidal interaction of a solar-type star with an orbiting companion: Excitation of g mode oscillation and orbital evolution
• Radius Dependent Angular Momentum Evolution in Low-Mass Stars. I
• Rotational mixing in low-mass stars II. Self-consistent models of Pop II RGB stars
• Tidal Dissipation in Planet-Hosting Stars: Damping of Spin-Orbit Misalignment and Survival of Hot Jupiters
• On shear-induced turbulence in rotating stars
• Calibration of Equilibrium Tide Theory for Extrasolar Planet Systems
• Rotational mixing in low-mass stars : I Effect of the mu-gradients in main sequence and subgiant Pop I stars
• Transport and mixing in the radiation zones of rotating stars: I-Hydrodynamical processes
• Tides in rotating barotropic fluid bodies: the contribution of inertial waves and the role of internal structure
• Rotating models of young solar-type stars : Exploring braking laws and angular momentum transport processes
• Diagnoses to unravel secular hydrodynamical processes in rotating main sequence stars
• Origin of Tidal Dissipation in Jupiter: II. the Value of Q
• Calibration of Equilibrium Tide Theory for Extrasolar Planet Systems II
• Observational constraints on tidal effects using orbital eccentricities
• On the diversity of magnetic interactions in close-in star-planet systems
• Nonlinear evolution of tidally forced inertial waves in rotating fluid bodies
• Effect of the rotation and tidal dissipation history of stars on the evolution of close-in planets
• The equilibrium tide in stars and giant planets: I - the coplanar case
• The variation of tidal dissipation in the convective envelope of low-mass stars along their evolution
• On the interaction between tides and convection
• Tidal evolution of planets around brown dwarfs
• Effect of the stellar spin history on the tidal evolution of close-in planets
• Star-planet interactions: II. Is planet engulfment the origin of fast rotating red giants?
• Why is there a Dearth of Close-In Planets around Fast-Rotating stars?
• Rotational evolution of slow-rotators sequence stars
• Star-planet interactions: I. Stellar rotation and planetary orbits
• Assessing magnetic torques and energy fluxes in close-in star-planet systems
• A unified normal mode approach to dynamic tides and its application to rotating Sun-like stars
• Impacts of stellar evolution and dynamics on the habitable zone: The role of rotation and magnetic activity
• Impact of the frequency dependence of tidal Q on the evolution of planetary systems
• The impact of rotation on turbulent tidal friction in stellar and planetary convective regions
• Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in massive planets. II. Effect of stellar metallicity
• Tidal inertial waves in the differentially rotating convective envelopes of low-mass stars - I. Free oscillation modes
• Secular orbital evolution of planetary systems and the dearth of close-in planets around fast rotators
• Interplay of tidal evolution and stellar wind braking in the rotation of stars hosting massive close-in planets
• Evolution of Exoplanets and their Parent Stars

Cited by in corpus (67)

• Nightside condensation of iron in an ultra-hot giant exoplanet
• Tidal dissipation in evolving low-mass and solar-type stars with predictions for planetary orbital decay
• RV-detected planets around M dwarfs: Challenges for core accretion models
• Orbital Decay of Short-Period Exoplanets via Tidal Resonance Locking
• Star-planet interactions. V. Dynamical and equilibrium tides in convective zones
• Rotation Period Evolution in Low-Mass Binary Stars: The Impact of Tidal Torques and Magnetic Braking
• Tidal dissipation in rotating fluid bodies: the presence of a magnetic field
• WASP-128b: a transiting brown dwarf in the dynamical-tide regime
• The fate of close-in planets: tidal or magnetic migration?
• TESS Asteroseismology of the known red-giant host stars HD 212771 and HD 203949
• Evolution of star-planet systems under magnetic braking and tidal interaction
• TOI-503: The first known brown dwarf-Am star binary from the TESS mission
• Spectroscopic and seismic analysis of red giants in eclipsing binaries discovered by Kepler
• TOI-3714 b and TOI-3629 b: Two gas giants transiting M dwarfs confirmed with HPF and NEID
• Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in massive planets. II. Effect of stellar metallicity
• Speeding past planets? Asteroids radiatively propelled by giant branch Yarkovsky effects
• Tidal dissipation due to inertial waves can explain the circularization periods of solar-type binaries
• Seismic probing of the first dredge-up event through the eccentric red-giant & red-giant spectroscopic binary KIC9163796
• Orbital Decay in Binaries Containing Post-Main Sequence Stars
• Magnetic and tidal migration of close-in planets. Influence of secular evolution on their population
• Post-main-sequence debris from rotation-induced YORP break-up of small bodies II: multiple fissions, internal strengths and binary production
• The lifetimes of planetary debris discs around white dwarfs
• Tidal circularization of gaseous planets orbiting white dwarfs
• Embedding planetesimals into white dwarf discs from large distances
• Orbital relaxation and excitation of planets tidally interacting with white dwarfs
• The dynamical history of the evaporating or disrupted ice giant planet around white dwarf WD J0914+1914
• TOI-3984 A b and TOI-5293 A b: two temperate gas giants transiting mid-M dwarfs in wide binary systems
• Horizontal shear instabilities in rotating stellar radiation zones: II. Effects of the full Coriolis acceleration
• An eccentric Brown Dwarf eclipsing an M dwarf
• Testing tidal theory for evolved stars by using red-giant binaries observed by Kepler
• Influence of stellar structure, evolution and rotation on the tidal damping of exoplanetary spin-orbit angles
• A close-in giant planet escapes engulfment by its star
• Planetary tidal interactions and the rotational evolution of low-mass stars. The Pleiades' anomaly
• Chaotic rotation and evolution of asteroids and small planets in high-eccentricity orbits around white dwarfs
• TESS Asteroseismic Analysis of the Known Exoplanet Host Star HD 222076
• Tidal migration of hot Jupiters: introducing the impact of gravity wave dissipation
• Survivability of radio-loud planetary cores orbiting white dwarfs
• The critical binary star separation for a planetary system origin of white dwarf pollution
• The STAR-MELT Python package for emission line analysis of YSOs
• Hydrodynamics and survivability during post-main-sequence planetary engulfment
• Linking the formation and fate of exo-Kuiper belts within solar system analogues
• Constraining planet formation around 6$M_{\odot }$-8$M_{\odot }$ stars
• The effects of nonlinearities on tidal flows in the convective envelopes of rotating stars and planets in exoplanetary systems
• Layered semi-convection and tides in giant planet interiors - II. Tidal dissipation
• Does magnetic field impact tidal dynamics inside the convective zone of low-mass stars along their evolution?
• Revisiting Kepler-444. II. Rotational, orbital and high-energy fluxes evolution of the system
• Constraining Tidal Quality Factor using Spin Period in Eclipsing Binaries
• The complex interplay between tidal inertial waves and zonal flows in differentially rotating stellar and planetary convective regions I. Free waves
• Star-planet tidal interaction and the limits of gyrochronology
• On the orbital decay of the gas giant Kepler-1658b
• The ultra-hot-Jupiter KELT-16 b: Dynamical Evolution and Atmospheric Properties
• The impact of tidal friction evolution on the orbital decay of ultra-short period planets
• Tidal Dissipation in Evolved Low and Intermediate Mass Stars
• The grain size survival threshold in one-planet post-main-sequence exoplanetary systems
• The unusual M-dwarf Warm Jupiter TOI-1899~b: Refinement of orbital and planetary parameters
• Pollux: A weak dynamo-driven dipolar magnetic field and implications for its probable planet
• Tidal evolution of exoplanetary systems hosting Potentially Habitable Exoplanets. The cases of LHS-1140 b-c and K2-18 b-c
• TATOO: a tidal-chronology standalone tool to estimate the age of massive close-in planetary systems
• Interplay between tidal flows and magnetic fields in nonlinear simulations of stellar and planetary convective envelopes
• The Rate of Planet-star Coalescences Due to Tides and Stellar Evolution
• Short-term stability of particles in the WD J0914+1914 white dwarf planetary system
• Tidally-induced migration of TESS gas giants orbiting M dwarfs
• Constraining Planetary Migration and Tidal Dissipation with Coeval Hot Jupiters
• Coralie radial velocity search for companions around evolved stars (CASCADES) II. Seismic masses for three red giants orbited by long-period massive planets
• Survival of satellites during the migration of a Hot Jupiter
• The Tale of a Hungry Subgiant and Its Brown Dwarf: Interior Radiative Damping Dominates the Tidal Evolution of TOI-5882
• An internal heating mechanism operating in ultra-short-period planets orbiting magnetically active stars