A framework for the architecture of exoplanetary systems. I. Four classes of planetary system architecture
arXiv:2301.02374 · doi:10.1051/0004-6361/202243751
Abstract
We present a novel, model-independent framework for studying the architecture of an exoplanetary system at the system level. This framework allows us to characterise, quantify, and classify the architecture of an individual planetary system. Our aim in this endeavour is to generate a systematic method to study the arrangement and distribution of various planetary quantities within a single planetary system. We propose that the space of planetary system architectures be partitioned into four classes: similar, mixed, anti-ordered, and ordered. We applied our framework to observed and synthetic multi-planetary systems, thereby studying their architectures of mass, radius, density, core mass, and the core water mass fraction. We explored the relationships between a system's (mass) architecture and other properties. Our work suggests that: (a) similar architectures are the most common outcome of planet formation; (b) internal structure and composition of planets shows a strong link with their system architecture; (c) most systems inherit their mass architecture from their core mass architecture; (d) most planets that started inside the ice line and formed in-situ are found in systems with a similar architecture; and (e) most anti-ordered systems are expected to be rich in wet planets, while most observed mass ordered systems are expected to have many dry planets. We find, in good agreement with theory, that observations are generally biased towards the discovery of systems whose density architectures are similar, mixed, or anti-ordered. This study probes novel questions and new parameter spaces for understanding theory and observations. Future studies may utilise our framework to not only constrain the knowledge of individual planets, but also the multi-faceted architecture of an entire planetary system. We also speculate on the role of system architectures in hosting habitable worlds.
28 pages, 19 figures, accepted in A&A
References in corpus (51)
- The Gaia mission
- The Transiting Exoplanet Survey Satellite
- Direct Imaging of Multiple Planets Orbiting the Star HR 8799
- Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1
- New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit
- Optical Images of an Exosolar Planet 25 Light Years from Earth
- Mass-Radius Relationships for Solid Exoplanets
- Habitable Zones Around Main-Sequence Stars: Dependence on Planetary Mass
- Accurate, Empirical Radii and Masses of Planets and their Host Stars with Gaia Parallaxes
- Planetary population synthesis coupled with atmospheric escape: a statistical view of evaporation
- The Mass of KOI-94d and a Relation for Planet Radius, Mass, and Incident Flux
- Kepler-62: A five-planet system with planets of 1.4 and 1.6 Earth radii in the Habitable Zone
- A resonant chain of four transiting, sub-Neptune planets
- Six transiting planets and a chain of Laplace resonances in TOI-178
- On the formation of planetary systems via oligarchic growth in thermally evolving viscous discs
- The Occurrence of Rocky Habitable Zone Planets Around Solar-Like Stars from Kepler Data
- Kepler Multi-Planet Systems Exhibit Unexpected Intra-system Uniformity in Mass and Radius
- First direct detection of an exoplanet by optical interferometry; Astrometry and K-band spectroscopy of HR8799 e
- A Dynamical Analysis of the Kepler-80 System of Five Transiting Planets
- The HARPS search for southern extra-solar planets. IX. mu Ara, a system with four planets
- On the Age of the TRAPPIST-1 System
- A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system
- The Elemental Abundances (with Uncertainties) of the Most Earth-like Planet
- From planetesimals to planets: volatile molecules
- A 1.9 Earth radius rocky planet and the discovery of a non-transiting planet in the Kepler-20 system
- From stellar nebula to planetesimals
- Kepler-411: a four-planet system with an active host star
- Precise Masses in the WASP-47 System
- On the extrasolar multi-planet system around HD160691
- Exoplanet characterisation in the longest known resonant chain: the K2-138 system seen by HARPS
- Long-Period Giant Companions to Three Compact, Multiplanet Systems
- Host star metallicity of directly imaged wide-orbit planets: implications for planet formation
- The mass of planet GJ676A b from ground-based astrometry: A planetary system with two mature gas giants suitable for direct imaging
- The influence of infall on the properties of protoplanetary discs
- A framework for the architecture of exoplanetary systems. II. Nature versus nurture: Emergent formation pathways of architecture classes
- Pairwise Tidal Equilibrium States and the Architecture of Extrasolar Planetary Systems
- Earths in Other Solar Systems N-body simulations: the Role of Orbital Damping in Reproducing the Kepler Planetary Systems
- Do planets remember how they formed?
- A new metric to quantify the similarity between planetary systems - application to dimensionality reduction using T-SNE
- MCMCI: A code to fully characterise an exoplanetary system
- A Simplified Photodynamical Model for Planetary Mass Determination in Low-Eccentricity Multi-Transiting Systems
- On the Inclination and Habitability of the HD 10180 System
- HD22496b: the first ESPRESSO standalone planet discovery
- When the Peas Jump around the Pod: How Stellar Clustering Affects the Observed Correlations between Planet Properties in Multi-Planet Systems
- A Six-Planet System Around the Star HD 34445
- Quantifying the Similarity of Planetary System Architectures
- The California Legacy Survey II. Occurrence of Giant Planets Beyond the Ice line
- Radial velocity precision of ESPRESSO through the analysis of the solar twin HIP 11915
- The DRAKE mission: finding the frequency of life in the Cosmos
- The California Legacy Survey I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades
- Split Peas in a Pod: Intra-System Uniformity of Super-Earths and Sub-Neptunes
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- The magnetic field and multiple planets of the young dwarf AU~Mic
- Super-Earths and Earth-like Exoplanets
- Planetary Population Synthesis and the Emergence of Four Classes of Planetary System Architectures
- Unveiling the internal structure and formation history of the three planets transiting HIP 29442 (TOI-469) with CHEOPS
- A framework for the architecture of exoplanetary systems. II. Nature versus nurture: Emergent formation pathways of architecture classes
- Architecture Classification for Extrasolar Planetary Systems
- Radii, masses, and transit-timing variations of the three-planet system orbiting the naked-eye star TOI-396
- Earth-like planets hosting systems: Architecture and properties
- Diversities and similarities exhibited by multi-planetary systems and their architectures: I. Orbital spacings
- Earth-like planet predictor: A machine learning approach
- The TESS-Keck Survey. XIX. A Warm Transiting Sub-Saturn Mass Planet and a non-Transiting Saturn Mass Planet Orbiting a Solar Analog
- The SPIRou Legacy Survey: Detection of a nearby world orbiting in the habitable zone of Gl725B achieved by correcting strong telluric contamination in near-infrared radial velocities with WAPITI
- The multi-planet system TOI-5624: Four transiting sub-Neptunes with an outer companion revealed by transit-timing variations
- Gas-depleted planet formation occurred in the four-planet system around the red dwarf LHS 1903