Why is there a Dearth of Close-In Planets around Fast-Rotating stars?
arXiv:1403.5860 · doi:10.1088/0004-637X/786/2/139
Abstract
We propose that the reported dearth of Objects of Interest (KOIs) with orbital periods days around stars with rotation periods days can be attributed to tidal ingestion of close-in planets by their host stars. We show that the planet distribution in this region of the plane is qualitatively reproduced with a model that incorporates tidal interaction and magnetic braking as well as the dependence on the stellar core--envelope coupling timescale. We demonstrate the consistency of this scenario with the inferred break in the distribution of close-in KOIs and point out a potentially testable prediction of this interpretation.
arXiv comment8 pages, 3 figures, accepted for publication in The Astrophysical Journal
References in corpus (30)
- Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler
- The false positive rate of Kepler and the occurrence of planets
- Kepler planets: a tale of evaporation
- Architecture and Dynamics of Kepler's Candidate Multiple Transiting Planet Systems
- Hot Stars with Hot Jupiters Have High Obliquities
- KEPLER's First Rocky Planet: Kepler-10b
- The Role of Core Mass in Controlling Evaporation: the Kepler Radius Distribution and the Kepler-36 Density Dichotomy
- Asteroseismic fundamental properties of solar-type stars observed by the NASA Kepler Mission
- Improved angular momentum evolution model for solar-like stars
- Tidal dissipation in rotating solar-type stars
- The Frequency of Hot Jupiters Orbiting Nearby Solar-Type Stars
- Orbital Evolution and Migration of Giant Planets: Modeling Extrasolar Planets
- On the tidal evolution of Hot Jupiters on inclined orbits
- The Kepler Cluster Study: Stellar Rotation in NGC6811
- Tidal Evolution of Close-in Planets
- Stellar Rotation Periods of the Kepler Objects of Interest: A Dearth of Close-in Planets around Fast Rotators
- The Exoplanet Census: A General Method, Applied to Kepler
- Observational Evidence for Tidal Destruction of Exoplanets
- Spin-Orbit Evolution Of Short-Period Planets
- Asteroseismology of the solar analogs 16 Cyg A & B from Kepler observations
- Rotation Periods, Variability Properties and Ages for Kepler Exoplanet Candidate Host Stars
- Weighing The Non-Transiting Hot Jupiter Tau BOO b
- A precise asteroseismic age and radius for the evolved Sun-like star KIC 11026764
- Empirical evidence for tidal evolution in transiting planetary systems
- Angular Momentum Transport In Solar-Type Stars: Testing the Timescale For Core-Envelope Coupling
- The Color-Period Diagram and Stellar Rotational Evolution - New Rotation Period Measurements in the Open Cluster M34
- Optical and X-ray Transients from Planet-Star Mergers
- Hot Jupiters and the evolution of stellar angular momentum
- Effect of the stellar spin history on the tidal evolution of close-in planets
- The Impact of Hot Jupiters on the Spin-down of their Host Stars
Cited by in corpus (43)
- The Occurrence and Architecture of Exoplanetary Systems
- The Apparently Decaying Orbit of WASP-12
- Orbital decay of hot Jupiters due to nonlinear tidal dissipation within solar-type hosts
- Hot Jupiters are Destroyed by Tides While Their Host Stars are on the Main Sequence
- Effect of the rotation and tidal dissipation history of stars on the evolution of close-in planets
- On the origin of the sub-Jovian desert in the orbital-period--planetary-mass plane
- The continuing search for evidence of tidal orbital decay of hot Jupiters
- 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
- From Hot Jupiters to Super-Earths via Roche Lobe Overflow
- Tidal Dissipation in WASP-12
- Evolution of angular-momentum-losing exoplanetary systems : Revisiting Darwin stability
- Are Tidal Effects Responsible for Exoplanetary Spin-Orbit Alignment?
- POET: A Model for (P)lanetary (O)rbital (E)volution due to (T)ides on Evolving Stars
- WASP-167b/KELT-13b: Joint discovery of a hot Jupiter transiting a rapidly-rotating F1V star
- The Dynamics of the Multi-planet System Orbiting Kepler-56
- WASP-4 is Accelerating Toward the Earth
- Discovery of XO-6b: a hot Jupiter transiting a fast rotating F5 star on an oblique orbit
- Evolution of star-planet systems under magnetic braking and tidal interaction
- A hot Jupiter for breakfast? --- Early stellar ingestion of planets may be common
- Stellar rotational periods in the planet hosting open cluster Praesepe
- Interplay of tidal evolution and stellar wind braking in the rotation of stars hosting massive close-in planets
- The CARMENES search for exoplanets around M dwarfs: Stable radial-velocity variations at the rotation period of AD~Leonis -- A test case study of current limitations to treating stellar activity
- Magnetic and tidal migration of close-in planets. Influence of secular evolution on their population
- Secular orbital evolution of planetary systems and the dearth of close-in planets around fast rotators
- AD Leonis: Radial velocity signal of stellar rotation or spin-orbit resonance?
- On the Stability of Extrasolar Planetary Systems and other Closely Orbiting Pairs
- Signature of Planetary Mergers on Stellar Spins
- Instability of mass transfer in a planet-star system
- On a Possible Solution to the Tidal Realignment Problem for Hot Jupiters
- Protostellar spin-down: a planetary lift?
- On the origin of dynamically isolated hot Earths
- Roche-lobe overflow in eccentric planet-star systems
- Optical-infrared flares and radio afterglows by Jovian planets inspiraling into their host stars
- Stellar spectral-type (mass) dependence of the dearth of close-in planets around fast-rotating stars. Architecture of Kepler confirmed single-exoplanet systems compared to star-planet evolution models
- A model for spin-orbit commensurability and synchronous starspot activity in stars with close-by planets
- A dearth of close-in planets around rapidly rotating stars or a dearth of data?
- The Rate of Planet-star Coalescences Due to Tides and Stellar Evolution
- Planet Across Space and Time (PAST). VII. The origin and tidal evolution of hot Jupiters constrained by a broken age-frequency relation
- On the behaviour of spin-orbit connection of exoplanets
- Tidal Evolution of Close-in Exoplanets and Host Stars
- Accretion of Planetary Material onto Host Stars
- Rotation of planet-harbouring stars
- Could star-planet magnetic interactions lead to planet migration and influence stellar rotation ?