Hidden Worlds: Dynamical Architecture Predictions of Undetected Planets in Multi-planet Systems and Applications to TESS Systems
arXiv:2007.06745 · doi:10.3847/1538-3881/aba61d
Abstract
Multi-planet systems produce a wealth of information for exoplanet science, but our understanding of planetary architectures is incomplete. Probing these systems further will provide insight into orbital architectures and formation pathways. Here we present a model to predict previously undetected planets in these systems via population statistics. The model considers both transiting and non-transiting planets, and can test the addition of more than one planet. Our tests show the model's orbital period predictions are robust to perturbations in system architectures on the order of a few percent, much larger than current uncertainties. Applying it to the multi-planet systems from TESS provides a prioritized list of targets, based on predicted transit depth and probability, for archival searches and for guiding ground-based follow-up observations hunting for hidden planets.
24 pages, 14 figures, 3 tables, accepted to Astronomical Journal
References in corpus (10)
- The NumPy array: a structure for efficient numerical computation
- The Transiting Exoplanet Survey Satellite
- A terrestrial planet candidate in a temperate orbit around Proxima Centauri
- Kepler constraints on planets near hot Jupiters
- Exploring Exoplanet Populations with NASA's Kepler Mission
- The period ratio distribution of Kepler's candidate multiplanet systems
- A 1.9 Earth radius rocky planet and the discovery of a non-transiting planet in the Kepler-20 system
- Two massive rocky planets transiting a K-dwarf 6.5 parsecs away
- Realistic On-the-fly Outcomes of Planetary Collisions II: Bringing Machine Learning to N-body Simulations
- Transiting Planets near the Snow Line from Kepler. I. Catalog
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- An Integrated Analysis with Predictions on the Architecture of the tau Ceti Planetary System, Including a Habitable Zone Planet
- Multiplicity Boost Of Transit Signal Classifiers: Validation of 69 New Exoplanets Using The Multiplicity Boost of ExoMiner
- K2-138 g: Spitzer Spots a Sixth Planet for the Citizen Science System
- Architecture Classification for Extrasolar Planetary Systems
- Planet Hunters TESS III: two transiting planets around the bright G dwarf HD 152843
- An Integrative Analysis of the HD 219134 Planetary System and the Inner Solar System: Extending DYNAMITE with Enhanced Orbital Dynamical Stability Criteria
- On planetary systems as ordered sequences
- Separated twins or just siblings? A multi-planet system around an M dwarf including a cool sub-Neptune
- Earth-like planet predictor: A machine learning approach
- The TESS-Keck Survey. XI. Mass Measurements for Four Transiting sub-Neptunes orbiting K dwarf TOI-1246
- Friends and Foes: Conditional Occurrence Rates of Exoplanet Companions and their Impact on Radial Velocity Follow-up Surveys