The Occurrence and Architecture of Exoplanetary Systems

Abstract

The basic geometry of the Solar System -- the shapes, spacings, and orientations of the planetary orbits -- has long been a subject of fascination as well as inspiration for planet formation theories. For exoplanetary systems, those same properties have only recently come into focus. Here we review our current knowledge of the occurrence of planets around other stars, their orbital distances and eccentricities, the orbital spacings and mutual inclinations in multiplanet systems, the orientation of the host star's rotation axis, and the properties of planets in binary-star systems.

41 pages. A few entries in Table 2 have been corrected

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• Photometry of Very Bright Stars with Kepler and K2 Smear Data
• An eccentric Brown Dwarf eclipsing an M dwarf
• Influence of stellar structure, evolution and rotation on the tidal damping of exoplanetary spin-orbit angles
• Stellar Obliquities & Planetary Alignments (SOPA) I. Spin-Orbit measurements of Three Transiting Hot Jupiters: WASP-72b, WASP-100b, & WASP-109b
• The EBLM project. VII. Spin-orbit alignment for the circumbinary planet host EBLM J0608-59 A/TOI-1338 A
• Peter Pan Discs: finding Neverland's parameters
• Transiting Exoplanet Monitoring Project (TEMP). IV. Refined System Parameters, Transit Timing Variations and Orbital Stability of the Transiting Planetary System HAT-P-25
• Kepler-1656b: a Dense Sub-Saturn With an Extreme Eccentricity
• In search of radio emission from exoplanets: GMRT observations of the binary system HD~41004
• The MUCHFUSS photometric campaign
• TESS Habitable Zone Star Catalog
• The ASAS-SN Catalog of Variable Stars VIII: "Dipper" Stars in the Lupus Star-Forming Region
• Super-Earths in the TW Hya disc
• CEMP stars: possible hosts to carbon planets in the early universe
• Quantifying the Influence of Jupiter on the Earth's Orbital Cycles
• DZ Cha: a bona fide photoevaporating disc
• Orbital Stability and Precession Effects in the Kepler-89 System
• A search for companions via direct imaging in the DSHARP planet-forming disks
• Close-in Super-Earths: The first and the last stages of planet formation in an MRI-accreting disc
• Orbital alignment of circumbinary planets that form in misaligned circumbinary discs: the case of Kepler-413b
• The direct imaging search for Earth 2.0: Quantifying biases and planetary false positives
• Extrasolar Kuiper Belts
• Extreme eccentricities of triple systems: Analytic results
• TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration
• ESPRESSO Mass determination of TOI-263b: An extreme inhabitant of the brown dwarf desert
• Kepler-1656b's Extreme Eccentricity: Signature of a Gentle Giant
• Kepler-90: Giant transit-timing variations reveal a super-puff
• The Spin-Orbit Misalignment of TOI-1842b: The First Measurement of the Rossiter-McLaughlin Effect for a Warm Sub-Saturn around a Massive Star
• Resonance in the K2-19 system is at odds with its high reported eccentricities
• Nodal Precession and Tidal Evolution of Two Hot-Jupiters: WASP-33 b and KELT-9 b
• Automated approach to measure stellar inclinations: validation through large-scale measurements on the red giant branch
• Exploring the Cosmic Evolution of Habitability with Galaxy Merger Trees
• A Theoretical Framework for the Mass Distribution of Gas Giant Planets forming through the Core Accretion Paradigm
• Expanding the Timeline for Earth's Photosynthetic Red Edge Biosignature
• Planet gap opening across stellar masses
• Planet occurrence rate density models including stellar effective temperature
• The resilience of Kepler systems to stellar obliquity
• The Epoch of Giant Planet Migration Planet Search Program. I. Near-Infrared Radial Velocity Jitter of Young Sun-like Stars
• TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS
• The Impact of Stellar Clustering on the Observed Multiplicity and Orbital Periods of Planetary Systems
• Atmospheric Dynamics of a Near Tidally Locked Earth-Size Planet
• A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113
• Magnetic topology in coupled binaries, spin-orbital resonances, and flares
• A recipe for orbital eccentricity damping in the type-I regime for low viscosity 2D-discs
• The Exosphere as a Boundary: Origin and Evolution of Airless Bodies in the Inner Solar System and Beyond Including Planets with Silicate Atmospheres
• The origins of nearly coplanar, non-resonant systems of close-in super-Earths
• CORALIE radial-velocity search for companions around evolved stars (CASCADES). I. Sample definition and first results: Three new planets orbiting giant stars
• Thermal Infrared Imaging and Atmospheric Modeling of VHS J125601.92-125723.9 b: Evidence for Moderately Thick Clouds and Equilibrium Carbon Chemistry in a Hierarchical Triple System
• Photometric survey of 67 near-Earth objects
• Atmospheric dynamics of temperate sub-Neptunes. Part I: dry dynamics
• Ejection of close-in super-Earths around low-mass stars in the giant impact stage
• A massive hot Jupiter orbiting a metal-rich early-M star discovered in the TESS full frame images
• Improving circumbinary planet detections by fitting their binary's apsidal precession
• The GAPS Programme at TNG XL: A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422
• Gap opening by planets in discs with magnetised winds
• The TESS-Keck Survey. VI. Two Eccentric sub-Neptunes Orbiting HIP-97166
• Stellar obliquities and magnetic activities of Planet-Hosting Stars and Eclipsing Binaries based on Transit Chord Correlation
• A reverse KAM method to estimate unknown mutual inclinations in exoplanetary systems
• One-third of Sun-like stars are born with misaligned planet-forming disks
• On the Orbital Spacing Pattern of Kepler Multiple Planet Systems
• Rapid rotators revisited: absolute dimensions of KOI-13
• The TEMPO Survey I: Predicting Yields of the Transiting Exosatellites, Moons, and Planets from a 30-day Survey of Orion with the Nancy Grace Roman Space Telescope
• Trapping (sub-)Neptunes similar to TOI-216b at the inner disk rim: Implications for the disk viscosity and the Neptunian desert
• A faint companion around CrA-9: protoplanet or obscured binary?
• Habitability properties of circumbinary planets
• On dust evolution in planet-forming discs in binary systems. II -- Comparison with Taurus and $\rho$ Ophiuchus (sub-)millimetre observations: discs in binaries have small dust sizes
• Interstellar communication network. I. Overview and assumptions
• Formation of a planetary Laplace resonance through migration in an eccentric disk - The case of GJ876
• Sub-Jovian desert of exoplanets at its boundaries. Parameter dependence along the main sequence
• EXPRES IV: Two Additional Planets Orbiting $\rho$ Coronae Borealis Reveal Uncommon System Architecture
• Cosmic evolution of black hole-spin and galaxy orientations: clues from the NewHorizon and Galactica simulations
• The evolution of circumstellar discs in the Galactic Centre: an application to the G-clouds
• Multi-planet disc interactions in binary systems
• Debris Disks in Multi-Planet Systems: Are Our Inferences Compromised by Unseen Planets?
• Photosynthesis on Exoplanets and Exomoons from Reflected Light
• Multiplicity of stars with planets in the solar neighbourhood
• In Situ and Ex Situ Formation Models of Kepler 11 Planets
• The scattering outcomes of Kepler circumbinary planets: planet mass ratio
• Qatar Exoplanet Survey: Qatar-6b -- a grazing transiting hot Jupiter
• Transiting Exoplanet Monitoring Project (TEMP). III. On the Relocation of the Kepler-9~b Transit
• Orphaned Exomoons: Tidal Detachment and Evaporation Following an Exoplanet-Star Collision
• Global Modeling of Nebulae With Particle Growth, Drift, and Evaporation Fronts. II. The Influence of Porosity on Solids Evolution
• A Pluto-Charon Sonata: The Dynamical Architecture of the Circumbinary Satellite System
• Demographics of Protoplanetary Disks: A Simulated Population of Edge-on Systems
• The PFS view of TOI-677 b: A spin-orbit aligned warm Jupiter in a dynamically hot system
• Efficient Dust Radial Drift Around Young Intermediate-mass Stars
• EOS-ESTM: A flexible climate model for habitable exoplanets
• The Demographics of Wide-Separation Planets
• Orbital Eccentricity -- Multiplicity Correlation for Planetary Systems and Comparison to the Solar System
• A collage of small planets from the Lick Carnegie Exoplanet Survey : Exploring the super-Earth and sub-Neptune mass regime
• K2-138 g: Spitzer Spots a Sixth Planet for the Citizen Science System
• Long term evolution of planetary systems with a terrestrial planet and a giant planet
• Optical-infrared flares and radio afterglows by Jovian planets inspiraling into their host stars
• Scientific Goals of the Kunlun Infrared Sky Survey (KISS)
• A possible misaligned orbit for the young planet AU Mic c
• Combined Effects of Disk Winds and Turbulence-Driven Accretion on Planet Populations
• A Machine Learning model to infer planet masses from gaps observed in protoplanetary disks
• Transits Probabilities Around Hypervelocity and Runaway Stars
• Debris Disks: Probing Planet Formation
• ALMA constraints on assembly of Core Accretion planets
• Toward Complete Characterization: Prospects for Directly Imaging Transiting Exoplanets
• DPNNet-2.0 Part I: Finding hidden planets from simulated images of protoplanetary disk gaps
• Search for Alignment of Disk Orientations in Nearby Star-Forming Regions: Lupus, Taurus, Upper Scorpius, $\rho$ Ophiuchi, and Orion
• CO isotopolog line fluxes of viscously evolving disks: cold CO conversion insufficient to explain observed low fluxes
• RV-exoplanet eccentricities: Good, Beta, and Best
• Role of Planetary Radius on Atmospheric Escape of Rocky Exoplanets
• Dynamical rearrangement of super-Earths during disk dispersal II. Assessment of the magnetospheric rebound model for planet formation scenarios
• Probing the Survival of Planetary Systems in Globular Clusters with Tidal Disruption Events
• Periodic optical variability and debris accretion in white dwarfs: a test for a causal connection
• Magnetic Fields and Accreting Giant Planets around PDS 70
• Non-adiabatic tidal oscillations induced by a planetary companion
• Self-gravity of debris discs can strongly change the outcomes of interactions with inclined planets
• A Dynamical Systems Approach to the Theory of Circumbinary Orbits in the Circular Restricted Problem
• Architecture of planetary systems predicted from protoplanetary disks observed with ALMA I: mass of the possible planets embedded in the dust gap
• Non-thermal emission from the interaction of magnetized exoplanets with the wind of their host star
• Connecting HL Tau to the Observed Exoplanet Sample
• A review of planetary systems around HD 99492, HD 147379 and HD 190007 with HARPS-N
• The distribution of mutual inclinations arising from the stellar quadrupole moment
• K2-HERMES II. Planet-candidate properties from K2 Campaigns 1-13
• XO-7 b: A transiting hot Jupiter with a massive companion on a wide orbit
• The GAPS Programme at TNG -- XXIV. An eccentric Neptune-mass planet near the inner edge of the BD-11 4672 habitable zone
• Model of a gap formed by a planet with fast inward migration
• Stellar activity and planetary atmosphere evolution in tight binary star systems
• Coralie radial-velocity search for companions around evolved stars (CASCADES) III. A new Jupiter host-star: in-depth analysis of HD 29399 using TESS data
• An SMA Continuum Survey of Circumstellar Disks in the Serpens Star-Forming Region
• The Dark Planets of the WASP-47 Planetary System
• Searching for planetary signals in Doppler time series: a performance evaluation of tools for periodograms analysis
• On planetary systems as ordered sequences
• On the Dayside Atmosphere of WASP-12b
• Meta-analysis of photometric and asteroseismic measurements of stellar rotation periods: the Lomb-Scargle periodogram, autocorrelation function, wavelet and rotational splitting analysis for 92 Kepler asteroseismic targets
• How the presence of a giant planet affects the outcome of terrestrial planet formation simulations
• The Telltale Heartbeat: Detection and Characterization of Eccentric Orbiting Planets via Tides on their Host Star
• BEBOP VII. SOPHIE discovery of BEBOP-3b, a circumbinary giant planet on an eccentric orbit
• Three Warm Jupiters orbiting TOI-6628, TOI-3837, TOI-5027 and one sub-Saturn orbiting TOI-2328
• The Heavy-element Content Trend of Planets: A Tracer of their Formation Sites
• High resolution ALMA and HST imaging of $\kappa$CrB: a broad debris disc around a post-main sequence star with low-mass companions
• Internal calibration of LAMOST and Gaia DR3 GSP-Spec stellar abundances
• Inclination Dynamics of Resonant Planets under the Influence of an Inclined External Companion
• Formation of multiple-planet systems in resonant chains around M dwarfs
• The GAPS programme at TNG. XLVI. Deep search for low-mass planets in late-dwarf systems hosting cold Jupiters
• The Impact of Stellar Clustering on the Observed Multiplicity of Super-Earth systems: Outside-in Cascade of Orbital Misalignments Initiated by Stellar Flybys
• The Impact of Tidal Migration of Hot Jupiters on the Rotation of Sun-like Main-sequence Stars
• Kepler-62f: Kepler's First Small Planet in the Habitable Zone, but Is It Real?
• Nature vs. nurture: a Bayesian framework for assessing apparent correlations between planetary orbital properties and stellar ages
• Close-in giant-planet formation via in-situ gas accretion and their natal disk properties
• Scheduling strategies for the ESPRESSO follow-up of TESS targets
• Characterization of debris disks observed with SPHERE
• A highly mutually-inclined, compact warm-Jupiter system KOI-984 ?
• Architecture of three-planet systems predicted from the observed protoplanetary disk of HL Tau
• Evidence for Primordial Alignment II: Insights from Stellar Obliquity Measurements for Hot Jupiters in Compact Multiplanet Systems
• On the role of magnetic fields in star formation
• The origin of the occurrence rate profile of gas giants inside 100 days
• Revisiting the Full Sets of Orbital Parameters for the XO-3 System: No evidence for Temporal Variation of the Spin-Orbit Angle
• An Asymmetric Eclipse Seen Towards the Pre-Main Sequence Binary System V928 Tau
• The Rate of Planet-star Coalescences Due to Tides and Stellar Evolution
• Ariel stellar characterisation III. Fast rotators and new FGK stars in the Ariel Mission Candidate Sample
• The Aligned Orbit of a Hot Jupiter around the M Dwarf TOI-4201
• HATS-59b,c: A Transiting Hot Jupiter and a Cold Massive Giant Planet Around a Sun-Like Star
• HATS-15 b and HATS-16 b: Two massive planets transiting old G dwarf stars
• Sub-stellar engulfment by a main sequence star: where is the lithium?
• Analysis of the public HARPS/ESO spectroscopic archive -- Jupiter-like planets around HD 103891 and HD 105779
• Higher Order Harmonics in the Light Curves of Eccentric Planetary Systems
• Revealing the Fate of Exoplanet Systems: Asteroseismic Identification of Host Star in the Red Clump or Red Giant Branch
• On the methanol emission detection in the TW Hya disc: the role of grain surface chemistry and non-LTE excitation
• Possible progression of mass flow processes around young intermediate-mass stars based on high-resolution near-infrared spectroscopy. I. Taurus
• The Habitability of GJ 357 d : Possible Climates and Observability
• Prospects for detecting the astrometric signature of Barnard's Star b
• Destination exoplanet: Habitability conditions influenced bystellar winds properties
• Emerging population of gap-opening planets around type-A stars -- Long-term evolution of the forming planets around HD 163296
• Change in the Orbital Period of a Binary System Due to Dynamical Tides for Main-Sequence Stars
• Revised Properties and Dynamical History for the HD 17156 System
• Variability of Known Exoplanet Host Stars Observed by TESS
• A Large Double-ring Disk around the Taurus M Dwarf J04124068+2438157
• Planet Occurrence: Doppler and Transit Surveys
• Multiverse Predictions for Habitability: Planetary Characteristics
• TOI-858 B b: A hot Jupiter on a polar orbit in a loose binary
• Radii, masses, and transit-timing variations of the three-planet system orbiting the naked-eye star TOI-396
• Geoastronomy: Rocky planets as the Lavosier-Lomonosov Bridge from the non-living to the living world
• Exoplanets Prediction in Multiplanetary Systems
• Enrichment of the HR 8799 planets by minor bodies and dust
• Orbital structure of planetary systems formed by giant impacts: stellar mass dependence
• Obliquities of Exoplanet Host Stars from Precise Distances and Stellar Angular Diameters
• Forming rocky exoplanets around K-dwarf stars
• The Case for a Large-Scale Occultation Network
• Planet formation: key mechanisms and global models
• Orbital evolution of potentially habitable planets of tidally interacting binary stars
• Tracking Advanced Planetary Systems (TAPAS) with HARPS-N VII. Elder suns with low-mass companions
• Detection and Characterization of Extrasolar Planets through Mean-Motion Resonances. II. The Effect of the Planet's Orbital Eccentricity on Debris Disk Structures
• Solid Accretion onto Neptune-Mass Planets I: In-Situ Accretion and Constraints from the metallicity of Uranus and Neptune
• The Properties of Planetesimal Collisions under Jupiter's Perturbation and the Application to Chondrule Formation via Impact Jetting
• Relative Habitability of Exoplanet Systems with Two Giant Planets
• Directly Detecting the Envelopes of Low-mass Planets Embedded In Protoplanetary Discs and The Case For TW Hydrae
• Estimating photoevaporative mass loss of exoplanets with PLATYPOS
• Searching for giant planets in the outer Solar System with far-infrared all-sky surveys
• Constrained Evolution of a Radially Magnetized Protoplanetary Disk: Implications for Planetary Migration
• GTC/CanariCam deep mid-infrared imaging survey of northern stars within 5 pc
• Stellar evolution and modelling stars
• True spin-orbit obliquities distribution: data-driven confirmation of no clustering of misaligned planets
• An upper limit for the growth of inner planets?
• On the behaviour of spin-orbit connection of exoplanets
• Planets similar in size are often dissimilar in interior
• Following up TESS Single Transits With Archival Photometry and Radial Velocities
• An HST/STIS View of Protoplanetary Disks in Upper Scorpius: Observations of Three Young M-Stars
• TESS Discovery of Twin Planets near 2:1 Resonance around Early M-Dwarf TOI 4342
• Design of the vacuum high contrast imaging testbed for CDEEP, the Coronagraphic Debris and Exoplanet Exploring Pioneer
• Planetary Edge Trends (PET). I. The Inner Edge-Stellar Mass Correlation
• TOI-2458 b: A mini-Neptune consistent with in situ hot Jupiter formation
• On the Dynamical Erasure of Initial Conditions in Multi-Planetary Systems
• Diversities and similarities exhibited by multi-planetary systems and their architectures: I. Orbital spacings
• Elemental Abundances of Kepler Objects of Interest in APOGEE DR17
• Detecting planet pairs in mean motion resonances via astrometry method
• The Influence of Magnetic Field Geometry on the Formation of Close-in Exoplanets
• Close-in compact super-Earth systems emerging from resonant chains: slow destabilization by unseen remnants of formation
• Architecture of planetary systems predicted from protoplanetary disks observed with ALMA II: evolution outcomes and dynamical stability
• Can planet formation resolve the dust budget crisis in high redshift galaxies?
• Mid-infrared absorption spectra and mass absorption coefficients for 23 chondrites: dependence on composition and grain size
• Predicting the Dominant Formation Mechanism of Multi-Planetary Systems
• Planet Hunters NGTS: New Planet Candidates from a Citizen Science Search of the Next Generation Transit Survey Public Data
• Configuration of Single Giant Planet Systems Generating `Oumuamua-Like Interstellar Asteroids
• Planet migration in wind-fed accretion disks in binaries
• Were the Obliquities in DI Herculis Excited by an Unseen Tertiary Companion?
• Higher-Order Mean-Motion Resonances Can Form in Type-I Disk Migration
• Evidence for a Non-Dichotomous Solution to the Kepler Dichotomy: Mutual Inclinations of Kepler Planetary Systems from Transit Duration Variations
• Possible formation pathways for the low density Neptune-mass planet HAT-P-26b
• A differentiable N-body code for transit timing and dynamical modelling -- II. Photodynamics
• The architecture of multi-planet systems as a tracer of their formation mechanisms
• Quantification of Tides in Giant Planets from Observations
• Few Observation Binary Orbit Solver (FOBOS) from two (or more) astrometric observations
• Characterizing the atmosphere of Proxima b with a space-based mid-infrared nulling interferometer
• On the dynamics of pebbles in protoplanetary disks with magnetically-driven winds
• Variations in the Radius Distribution of Single- and Compact Multiple-transiting Planets
• A fast tree algorithm for multi-component coagulation equation
• Numerical approach to second-order canonical perturbation theory in the planetary 3-body problem: Application to exoplanets
• On the Ordering of Exoplanet Systems
• Ground-Based Radial Velocity as Critical Support for Future NASA Earth-Finding Missions
• Decoding the Future of Exoplanets: Asteroseismic Confirmation of Subgiant and Red Giant Hosts
• Predictions for Dusty Mass Loss from Asteroids during Close Encounters with Solar Probe Plus
• On the Habitability of Our Universe
• The TESS-Keck Survey. XIX. A Warm Transiting Sub-Saturn Mass Planet and a non-Transiting Saturn Mass Planet Orbiting a Solar Analog
• Upper limits on the probability of an interstellar civilization arising in the local Solar neighborhood
• Further Evidence for Tidal Spin-Up of Hot Jupiter Host Stars
• AU Mic b is the Youngest Planet to have a Spin-Orbit Alignment Measurement
• Accounting for Transit Timing Detectability: Biases in Planetary Radius and Orbital Period
• Spin-Orbit Geometry of AU Mic b and c from Back-to-Back Transits Observed Contemporaneously with Magellan PFS, LCOGT, and CHEOPS
• Constraints on the Obliquities of Kepler Planet-Hosting Stars
• Photoevaporation of protoplanetary disks by Far-UV photons arising from neighbouring massive stars: observation of proplyds and modelling
• A Homogeneous Catalog of Rossiter-McLaughlin Systems: Distinct $e$-$\lambda$ Trends in Three Gas-Giant Mass Regimes
• Rapid and Predictive Planet Population Synthesis Model (RAPPS) I. Upgraded model and resulting synthetic populations
• Exoplanet transit search at the detection limit: detection and false alarm vetting pipeline
• The EBLM Project XVIII. 3D Obliquities of Five Low-Mass Eclipsing Binaries
• Re-accretion of Giant Impact Ejecta Can Drive Significant Atmospheric Erosion on Terrestrial Planets
• Validating the Orbital Periods of the Coolest TESS Exoplanet Candidates
• Modeling the Solar System I: Characterization Limits from Analytic Timing Variations
• Upside down: GJ3090 b the first retrograde exoplanet around an M dwarf detected with NIRPS
• Longterm Stability of Planetary Systems formed from a Transitional Disk
• Modelling the secular evolution of proto-planetary disc dust sizes -- A comparison between the viscous and magnetic wind case
• Disentangling the stellar inclination of transiting planetary systems: fully analytic approach to the Rossiter-McLaughlin effect incorporating the stellar differential rotation
• Generating Stellar Obliquity in Systems with Broken Protoplanetary Disks
• Radio Emission from UV Cet: Auroral Emission from a Stellar Magnetosphere
• Observing transiting exoplanets with the MicroObservatory: 43 new transit light curves of the hot Jupiter HAT-P-32b
• A new formation scenario of a counter-rotating circumstellar disk: spiral-arm accretion from a circumbinary disk in a triple protostar system
• Planet formation in intermediate-separation binary systems
• PLATO Hare-and-Hounds exercise: Asteroseismic model fitting of main-sequence solar-like pulsators
• Asteroseismology of iota Draconis and Discovery of an Additional Long-Period Companion
• Constraining the mass of the planet(s) sculpting a disk cavity. The intriguing case of 2MASS J16042165-2130284
• The Influence of General Relativity on the Spins of Celestial Bodies in Inclined Orbits