Predicting the long-term stability of compact multiplanet systems
arXiv:2007.06521 · doi:10.1073/pnas.2001258117
Abstract
We combine analytical understanding of resonant dynamics in two-planet systems with machine learning techniques to train a model capable of robustly classifying stability in compact multi-planet systems over long timescales of orbits. Our Stability of Planetary Orbital Configurations Klassifier (SPOCK) predicts stability using physically motivated summary statistics measured in integrations of the first orbits, thus achieving speed-ups of up to over full simulations. This computationally opens up the stability constrained characterization of multi-planet systems. Our model, trained on three-planet systems sampled at discrete resonances, generalizes both to a sample spanning a continuous period-ratio range, as well as to a large five-planet sample with qualitatively different configurations to our training dataset. Our approach significantly outperforms previous methods based on systems' angular momentum deficit, chaos indicators, and parametrized fits to numerical integrations. We use SPOCK to constrain the free eccentricities between the inner and outer pairs of planets in the Kepler-431 system of three approximately Earth-sized planets to both be below 0.05. Our stability analysis provides significantly stronger eccentricity constraints than currently achievable through either radial velocity or transit duration measurements for small planets, and within a factor of a few of systems that exhibit transit timing variations (TTVs). Given that current exoplanet detection strategies now rarely allow for strong TTV constraints (Hadden et al., 2019), SPOCK enables a powerful complementary method for precisely characterizing compact multi-planet systems. We publicly release SPOCK for community use.
Published week of July 13th in Proceedings of the National Academy of Sciences: https://www.pnas.org/cgi/doi/10.1073/pnas.2001258117. Check out simple usage of package (and regenerate paper figures) at: https://github.com/dtamayo/spock
References in corpus (55)
- XGBoost: A Scalable Tree Boosting System
- Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1
- REBOUND: An open-source multi-purpose N-body code for collisional dynamics
- Dynamical Outcomes of Planet-Planet Scattering
- Catalog of Nearby Exoplanets
- Architecture of Kepler's Multi-transiting Systems: II. New investigations with twice as many candidates
- Probabilistic Forecasting of the Masses and Radii of Other Worlds
- Dynamical Origin of Extrasolar Planet Eccentricity Distribution
- WHFast: A fast and unbiased implementation of a symplectic Wisdom-Holman integrator for long term gravitational simulations
- Breaking the Chains: Hot Super-Earth systems from migration and disruption of compact resonant chains
- Terrestrial Planet Occurrence Rates for the Kepler GK Dwarf Sample
- The nature of the TRAPPIST-1 exoplanets
- Extracting Planet Mass and Eccentricity From TTV data
- The California-Kepler Survey V. Peas in a Pod: Planets in a Kepler Multi-planet System are Similar in Size and Regularly Spaced
- Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities
- The Lick-Carnegie Exoplanet Survey: A Uranus-mass Fourth Planet for GJ 876 in an Extrasolar Laplace Configuration
- Exoplanet Orbital Eccentricities Derived From LAMOST-Kepler Analysis
- A resonant chain of four transiting, sub-Neptune planets
- Kepler Planet Masses and Eccentricities from TTV Analysis
- First order resonance overlap and the stability of close two planet systems
- Transit Timing Observations from Kepler: VII. Confirmation of 27 planets in 13 multiplanet systems via Transit Timing Variations and orbital stability
- Post-Oligarchic Evolution of Protoplanetary Embryos and the Stability of Planetary Systems
- Secure TTV Mass Measurements: Ten Kepler Exoplanets between 3 and 8 Earth Masses with Diverse Densities and Incident Fluxes
- AMD-stability and the classification of planetary systems
- Dynamical Constraints on the HR 8799 Planets with GPI
- Three Body Resonance Overlap in Closely Spaced Multiple Planet Systems
- The (In)Stability of Planetary Systems
- KOI-152's Low Density Planets
- Convergent Migration Renders TRAPPIST-1 Long-lived
- The stability of tightly-packed, evenly-spaced systems of Earth-mass planets orbiting a Sun-like star
- Theory of Secular Chaos and Mercury's Orbit
- The Orbital Stability of Planets Trapped in the First-Order Mean-Motion Resonances
- A 1.9 Earth radius rocky planet and the discovery of a non-transiting planet in the Kepler-20 system
- A Criterion for the Onset of Chaos in Systems of Two Eccentric Planets
- The statistical mechanics of planet orbits
- Chaotic Disintegration of the Inner Solar System
- A Machine Learns to Predict the Stability of Tightly Packed Planetary Systems
- Dynamical Evolution of Multi-Resonant Systems: the Case of GJ876
- Numerical and Analytical Modelling of Transit Time Variations
- Dynamical Stability of Imaged Planetary Systems in Formation: Application to HL Tau
- Hill stability in the AMD framework
- Dynamical behaviour of multiplanet systems close to their stability limit
- A dynamical analysis of the Kepler-11 planetary system
- AMD-stability in presence of first order Mean Motion Resonances
- A machine learns to predict the stability of circumbinary planets
- An Integrable Model for the Dynamics of Planetary Mean Motion Resonances
- Survival of non-coplanar, closely-packed planetary systems after a close encounter
- A new paradigm for reproducing and analyzing N-body simulations of planetary systems
- Dynamical instability and its implications for planetary system architecture
- Plausible Compositions of the Seven TRAPPIST-1 Planets Using Long-term Dynamical Simulations
- Dynamical instabilities in systems of multiple short-period planets are likely driven by secular chaos: a case study of Kepler-102
- Resonant Chains and Three-body Resonances in the Closely-Packed Inner Uranian Satellite System
- Fundamental limits from chaos on instability time predictions in compact planetary systems
- Nekhoroshev Estimates for the Survival Time of Tightly Packed Planetary Systems
- Spacing of Kepler Planets: Sculpting by Dynamical Instability
Cited by in corpus (61)
- Warm terrestrial planet with half the mass of Venus transiting a nearby star
- Formation of Ultra-Short-Period Planets by Obliquity-Driven Tidal Runaway
- Architectures of Compact Super-Earth Systems Shaped by Instabilities
- The TESS-Keck Survey II: An Ultra-Short Period Rocky Planet and its Siblings Transiting the Galactic Thick-Disk Star TOI-561
- Statistical methods for exoplanet detection with radial velocities
- A super-Earth and a mini-Neptune near the 2:1 MMR straddling the radius valley around the nearby mid-M dwarf TOI-2096
- A Criterion for the Stability of Planets in Chains of Resonances
- 37 New Validated Planets in Overlapping K2 Campaigns
- A low-eccentricity migration pathway for a 13-h-period Earth analogue in a four-planet system
- A sub-Earth-mass planet orbiting Barnard's star
- On the long-term stability of the Solar System in the presence of weak perturbations from stellar flybys
- The TOI-763 system: sub-Neptunes orbiting a Sun-like star
- How Close are Compact Multi-Planet Systems to the Stability Limit?
- Dynamics and Origins of the Near-Resonant Kepler Planets
- Two super-Earths at the edge of the habitable zone of the nearby M dwarf TOI-2095
- Physical Parameters of the Multi-Planet Systems HD 106315 and GJ 9827
- Transit Timing Variations in the three-planet system: TOI-270
- Sporadic Spin-Orbit Variations in Compact Multi-planet Systems and their Influence on Exoplanet Climate
- A Tidal Origin for a 3-body Resonance in Kepler-221
- TOI-4010: A System of Three Large Short-Period Planets With a Massive Long-Period Companion
- The Criterion for Chaos in Three-Planet Systems
- Stability Constrained Characterization of Multiplanet Systems
- Stable lifetime of compact, evenly-spaced planetary systems with non-equal masses
- The instability mechanism of compact multiplanet systems
- A general stability-driven approach for the refinement of multi-planet systems
- Hot Jupiter formation in dense clusters: secular chaos in multi-planetary systems
- Chaos in multiplanetary extrasolar systems
- Exoplanet atmosphere evolution: emulation with neural networks
- Hyades Member K2-136c: The Smallest Planet in an Open Cluster with a Precisely Measured Mass
- The Exomoon Corridor for Multiple Moon Systems
- Updated Planetary Mass Constraints of the Young V1298 Tau System Using MAROON-X
- Stability Constrained Characterization of the 23 Myr-old V1298 Tau System: Do Young Planets Form in Mean Motion Resonance Chains?
- A young progenitor for the most common planetary systems in the Galaxy
- On the Degree of Dynamical Packing in the Kepler Multi-planet Systems
- Birth cluster simulations of planetary systems with multiple super-Earths: initial conditions for white dwarf pollution drivers
- TOI-1749: an M dwarf with a Trio of Planets including a Near-Resonant Pair
- The distribution of mutual inclinations arising from the stellar quadrupole moment
- An Integrative Analysis of the HD 219134 Planetary System and the Inner Solar System: Extending DYNAMITE with Enhanced Orbital Dynamical Stability Criteria
- Machine learning prediction for mean motion resonance behaviour -- The planar case
- Residual Neural Networks for the Prediction of Planetary Collision Outcomes
- Two warm Earth-sized exoplanets and an Earth-sized candidate in the M5V-M6V binary system TOI-2267
- Hiding Planets Near and Far: The Parameter Space of Hidden Companions for Known Planetary Systems
- Orbital stability of compact three-planet systems, II: Post-instability impact behaviour
- Can metal-rich worlds form by giant impacts?
- Machine learning approach for mapping the stable orbits around planets
- On Computational Poisson Geometry II: Numerical Methods
- Relative Habitability of Exoplanet Systems with Two Giant Planets
- TESS and HARPS-N unveil two planets transiting TOI-1453. A super-Earth and one of the lowest mass sub-Neptunes
- A Bayesian neural network predicts the dissolution of compact planetary systems
- Constraints on Evolutionary Timescales for M Dwarf Planets from Dynamical Stability Arguments
- Planet Mass Function around M stars at 1-10 au: A Plethora of sub-Earth mass objects
- A High-Precision, Differentiable Code for Solar System Ephemerides
- RedDots: Planetary masses in the GJ1061 system from planet-planet interaction
- Secular Dynamics of Compact Three-Planet Systems
- Particle dynamics in TOI-178 planetary system
- A Criterion for the Onset of Chaos in Compact, Eccentric Multiplanet Systems
- Instability from high-order resonant chains in wide-separation massive planet systems
- The Dynamical Environment of Kepler-223 Planetary System
- The TESS-Keck Survey. XI. Mass Measurements for Four Transiting sub-Neptunes orbiting K dwarf TOI-1246
- Advanced Techniques in Stability Analysis of Trans-Neptunian Objects
- Exploring Long-period Architectures: Four New Planet Candidates from Kepler with Periods >342 days