Solar System Physics for Exoplanet Research

Abstract

Over the past three decades, we have witnessed one of the great revolutions in our understanding of the cosmos - the dawn of the Exoplanet Era. Where once we knew of just one planetary system (the Solar system), we now know of thousands, with new systems being announced on a weekly basis. Of the thousands of planetary systems we have found to date, however, there is only one that we can study up-close and personal - the Solar system. In this review, we describe our current understanding of the Solar system for the exoplanetary science community - with a focus on the processes thought to have shaped the system we see today. In section one, we introduce the Solar system as a single well studied example of the many planetary systems now observed. In section two, we describe the Solar system's small body populations as we know them today - from the two hundred and five known planetary satellites to the various populations of small bodies that serve as a reminder of the system's formation and early evolution. In section three, we consider our current knowledge of the Solar system's planets, as physical bodies. In section four, we discuss the research that has been carried out into the Solar system's formation and evolution, with a focus on the information gleaned as a result of detailed studies of the system's small body populations. In section five, we discuss our current knowledge of planetary systems beyond our own - both in terms of the planets they host, and in terms of the debris that we observe orbiting their host stars. As we learn ever more about the diversity and ubiquity of other planetary systems, our Solar system will remain the key touchstone that facilitates our understanding and modelling of those newly found systems, and we finish section five with a discussion of the future surveys that will further expand that knowledge.

Invited Review, Accepted for publication in Publications of the Astronomical Society of the Pacific; 23 figures, plus a further 18 in the appendix; 4 tables

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• Locating the Launching Region of T Tauri Winds: The Case of DG Tau
• A record of planet migration in the Main Asteroid Belt
• Evolved stars hint to an external origin of enhanced metallicity in planet-hosting stars
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• Collisional processes and size distribution in spatially extended debris discs
• The Resonant Transneptunian Populations
• Resolved images of a protostellar outflow launched by an extended disk wind
• Mars' Growth Stunted by an Early Giant Planet Instability
• Debris disks as signposts of terrestrial planet formation
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• The Detectability of High Redshift Lyman Alpha Emission Lines Prior to the Reionization of the Universe
• Origin and Evolution of Short-Period Comets
• Towards the Minimum Inner Edge Distance of the Habitable Zone
• Hot super-Earths and giant planet cores from different migration histories
• Breaking through: The effects of a velocity distribution on barriers to dust growth
• Stellar encounters as the origin of distant solar system objects in highly eccentric orbits
• Ice Lines, Planetesimal Composition and Solid Surface Density in the Solar Nebula
• Exomoon habitability constrained by illumination and tidal heating
• Resonance Occupation in the Kuiper Belt: Case Examples of the 5:2 and Trojan Resonances
• Abundant Circumstellar Silica Dust and SiO Gas Created by a Giant Hypervelocity Collision in the ~12 Myr HD172555 System
• Dynamical Constraints on the HR 8799 Planets with GPI
• HAT-P-26b: A Low-Density Neptune-Mass Planet Transiting a K Star
• Reconnaissance of the HR 8799 Exosolar System I: Near IR Spectroscopy
• The Scattered Disk as the source of the Jupiter Family comets
• Debris from terrestrial planet formation: the Moon-forming collision
• Possible ring material around centaur (2060) Chiron
• Initial characterization of interstellar comet 2I/Borisov
• Pencil-Beam Surveys for Faint Trans-Neptunian Objects
• Dust in Resonant Extrasolar Kuiper Belts - Grain Size and Wavelength Dependence of Disk Structure
• Neptune's Orbital Migration Was Grainy, Not Smooth
• Impact on asteroseismic analyses of regular gaps in Kepler data
• TESS Spots a Compact System of Super-Earths around the Naked-Eye Star HR 858
• Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems
• Debris from giant impacts between planetary embryos at large orbital radii
• Initial Characterization of Interstellar Comet 2I/2019 Q4 (Borisov)
• An Eccentric Hot Jupiter Orbiting the Subgiant HD 185269
• A Dynamical Analysis of the Kepler-80 System of Five Transiting Planets
• Circumstellar Disk Lifetimes In Numerous Galactic Young Stellar Clusters
• The Twenty-Five Year Lick Planet Search
• Collision rates in the present-day Kuiper Belt and Centaur Regions: Applications to surface activation and modification on Comets, Kuiper Belt Objects, Centaurs, and Pluto-Charon
• The ELODIE survey for northern extra-solar planets III. Three planetary candidates detected with ELODIE
• The formation of Uranus and Neptune among Jupiter and Saturn
• Did Saturn's rings form during the Late Heavy Bombardment ?
• The Edge of the Solar System
• Metallicity of M dwarfs III. Planet-metallicity and planet-stellar mass correlations of the HARPS GTO M dwarf sample
• Spectroscopy and thermal modelling of the first interstellar object 1I/2017 U1 'Oumuamua
• SPICA - a large cryogenic infrared space telescope Unveiling the obscured Universe
• The HOSTS survey for exozodiacal dust: Observational results from the complete survey
• SONS: The JCMT legacy survey of debris discs in the submillimetre
• The Hubble Wide Field Camera 3 Test of Surfaces in the Outer Solar System: The Compositional Classes of the Kuiper Belt
• Analysis of the Herschel DEBRIS Sun-like star sample
• A Super-Earth and two Neptunes Orbiting the Nearby Sun-like star 61 Virginis
• An Outer Planet Beyond Pluto and Origin of the Trans-Neptunian Belt Architecture
• The planets around NN Ser: still there
• On the detectability of habitable exomoons with Kepler-class photometry
• Two new HATNet hot Jupiters around A stars, and the first glimpse at the occurrence rate of hot Jupiters from TESS
• Detection of a planetary system orbiting the eclipsing polar HU Aqr
• A near-infrared interferometric survey of debris disc stars. III. First statistics based on 42 stars observed with CHARA/FLUOR
• The Effects of a Stellar Encounter on a Planetesimal Disk
• HEK VI: On the Dearth of Galilean Analogs in Kepler and the Exomoon Candidate Kepler-1625b I
• Kepler-445, Kepler-446 and the Occurrence of Compact Multiples Orbiting Mid-M Dwarf Stars
• Minerva-Australis I: Design, Commissioning, & First Photometric Results
• Dust Production from collisions in extrasolar planetary systems The inner Beta-Pictoris disc
• Satellites of the largest Kuiper belt objects
• Exocometary gas structure, origin and physical properties around $\beta$ Pictoris through ALMA CO multi-transition observations
• A dynamical analysis of the proposed HU Aquarii planetary system
• The History of the Solar System's Debris Disc: Observable Properties of the Kuiper Belt
• The Delivery of Water During Terrestrial Planet Formation
• Outer edges of debris discs: how sharp is sharp?
• The Habitable Zone Gallery
• Molecular gas in debris disks around young A-type stars
• On the Migration of Jupiter and Saturn: Constraints from Linear Models of Secular Resonant Coupling with the Terrestrial Planets
• On the Plutinos and Twotinos of the Kuiper Belt
• Retired A Stars and Their Companions VI. A Pair of Interacting Exoplanet Pairs Around the Subgiants 24 Sextanis and HD200964
• Hubble Space Telescope Observations of Main Belt Comet (596) Scheila
• Gas giant planets as dynamical barriers to inward-migrating super-Earths
• Resolving debris discs in the far-infrared: early highlights from the DEBRIS survey
• The Runaway Greenhouse: implications for future climate change, geoengineering and planetary atmospheres
• The Anglo-Australian Planet Search XXIV: The Frequency of Jupiter Analogs
• On the Occurrence Rate of Hot Jupiters in Different Stellar Environments
• The Formation of the Collisional Family around the Dwarf Planet Haumea
• Titan solar occultation observations reveal transit spectra of a hazy world
• Observational constraints on the orbit and location of Planet Nine in the outer solar system
• A Complete ALMA Map of the Fomalhaut Debris Disk
• Resolved Imaging of the HR 8799 Debris Disk with Herschel
• High-Resolution Simulations of a Moon-Forming Impact and Post-Impact Evolution
• The early instability scenario: terrestrial planet formation during the giant planet instability, and the effect of collisional fragmentation
• On the Frequency of Potential Venus Analogs from Kepler Data
• Rapid disappearance of a warm, dusty circumstellar disk
• A Signature of Planetary Migration: The Origin of Asymmetric Capture in the 2:1 Resonance
• The Size-Frequency Distribution of the Zodiacal Cloud: Evidence from the Solar System Dust Bands
• Venus as a Laboratory for Exoplanetary Science
• ALMA observations of the $\eta$ Corvi debris disc: inward scattering of CO-rich exocomets by a chain of 3-30 M${}_{\oplus }$ planets?
• Large Impacts around a Solar Analog Star in the Era of Terrestrial Planet Formation
• The Formation of Jupiter's Diluted Core by a Giant Impact
• Onset of giant planet migration before 4480 million years ago
• The bright end of the exo-Zodi luminosity function: Disk evolution and implications for exo-Earth detectability
• Recurrent Perihelion Activity in (3200) Phaethon
• Keck Pencil-Beam Survey for Faint Kuiper Belt Objects
• Dynamical models of Kuiper Belt dust in the inner and outer Solar System
• Glancing views of the Earth. From a lunar eclipse to an exoplanetary transit
• The CORALIE survey for southern extra-solar planets XV. Discovery of two eccentric planets orbiting HD4113 and HD156846
• The population of long-period transiting exoplanets
• Gravitational Stirring in Planetary Debris Disks
• Kuiper Belt-Like Hot and Cold Populations of Planetesimal Inclinations in the $\beta$ Pictoris Belt Revealed by ALMA
• A near-infrared interferometric survey of debris-disc stars. IV. An unbiased sample of 92 southern stars observed in H-band with VLTI/PIONIER
• CO in distantly active comets
• Sublimation Temperature of Circumstellar Dust Particles and Its Importance for Dust Ring Formation
• Terrestrial Planet Formation Constrained by Mars and the Structure of the Asteroid Belt
• The Hunt for Exomoons with Kepler (HEK): II. Analysis of Seven Viable Satellite-Hosting Planet Candidates
• Instability-Driven Dynamical Evolution Model of a Primordially 5 Planet Outer Solar System
• Main-Belt Comet P/2008 R1 (Garradd)
• On the formation of terrestrial planets in hot-Jupiter systems
• The Return of Activity in Main-Belt Comet 133P/Elst-Pizarro
• Prospects for Extrasolar "Earths" in Habitable Zones
• Secular resonance sweeping of the main asteroid belt during planet migration
• The McDonald Observatory Planet Search: New Long-Period Giant Planets, and Two Interacting Jupiters in the HD 155358 System
• Resolved Submillimeter Observations of the HR 8799 and HD 107146 Debris Disks
• A comprehensive radial velocity error budget for next generation Doppler spectrometers
• The Extraordinary Multi-Tailed Main-Belt Comet P/2013 P5
• 2I/Borisov: A C${}_2$ depleted interstellar comet
• Impact splash chondrule formation during planetesimal recycling
• First images of debris disks around TWA 7, TWA 25, HD 35650, and HD 377
• Constraining Orbital Parameters Through Planetary Transit Monitoring
• Terrestrial Planet Formation in a protoplanetary disk with a local mass depletion: A successful scenario for the formation of Mars
• A Compound model for the origin of Earth's water
• On the dynamical stability of the proposed planetary system orbiting NSVS 14256825
• Incidence of debris discs around FGK stars in the solar neighbourhood
• A Detailed Dynamical Investigation of the Proposed QS Virginis Planetary System
• Saturn's deep atmospheric flows revealed by the Cassini Grand Finale gravity measurements
• Detecting companions to extrasolar planets using mutual events
• Exomoon habitability constrained by energy flux and orbital stability
• On the Frequency of Jupiter Analogs
• The Fragility of the Terrestrial Planets During a Giant Planet Instability
• A gap in the planetesimal disc around HD 107146 and asymmetric warm dust emission revealed by ALMA
• Does the presence of planets affect the frequency and properties of extrasolar Kuiper Belts? Results from the Herschel DEBRIS and DUNES surveys
• Col-OSSOS: Colors of the Interstellar Planetesimal 1I/`Oumuamua
• Miniature Exoplanet Radial Velocity Array (MINERVA) I. Design, Commissioning, and First Science Results
• Exoplanet Classification and Yield Estimates for Direct Imaging Missions
• Detection of CN gas in Interstellar Object 2I/Borisov
• An Empirical Planetesimal Belt Radius - Stellar Luminosity Relation
• Jupiter - friend or foe? I: the asteroids
• OSSOS VI. Striking Biases in the detection of large semimajor axis Trans-Neptunian Objects
• Forming Mercury by Giant Impacts
• Possible detection of two giant extrasolar planets orbiting the eclipsing polar UZ Fornacis
• The formation of the solar system
• External photoevaporation of circumstellar disks constrains the timescale for planet formation
• Jupiter's formation and its primordial internal structure
• Determining Habitability: Which exoEarths should we search for life?
• A large lunar impact blast on September 11th 2013
• Detection of Potential Transit Signals in 17 Quarters of Kepler Data: Results of the Final Kepler Mission Transiting Planet Search (DR25)
• Origin and evolution of long-period comets
• Multiple mean motion resonances in the HR 8799 planetary system
• The HARPS search for southern extrasolar planets. XXV. Four new planets in orbit around the moderatly active dwarfs HD 63765, HD 104067, HD 125595, and HIP 70849
• A Critical Examination of the X-Wind Model for Chondrule and Calcium-rich, Aluminum-rich Inclusion Formation and Radionuclide Production
• Extreme trans-Neptunian objects and the Kozai mechanism: signalling the presence of trans-Plutonian planets
• Thermal Histories of Chondrules in Solar Nebula Shocks
• A Self-Consistent Model of the Circumstellar Debris Created by a Giant Hypervelocity Impact in the HD172555 System
• The Frequency of Low-Mass Exoplanets. III. Toward eta-Earth at Short Periods
• Where Did The Moon Come From?
• Asteroid families in the first order resonances with Jupiter
• New Constraints on the Composition of Jupiter from Galileo Measurements and Interior Models
• Eclipsing time variations in close binary systems: Planetary hypothesis vs. Applegate mechanism
• Collisional Grooming Models of the Kuiper Belt Dust Cloud
• The Decay of Debris Disks around Solar-Type Stars
• Understanding Jupiter's Interior
• The Exozodiacal Dust Problem for Direct Observations of ExoEarths
• An improved model of the Edgeworth-Kuiper debris disk
• A Dynamical Analysis of the Proposed Circumbinary HW Virginis Planetary System
• The Age of the HD 15407 System and the Epoch of Final Catastrophic Mass Accretion onto Terrestrial Planets around Sun-like Stars
• The planet search programme at the ESO CES and HARPS. IV. The search for Jupiter analogues around solar-like stars
• The Capture of Centaurs as Trojans
• A Bayesian Periodogram Finds Evidence for Three Planets in 47 Ursae Majoris
• New Extreme Trans-Neptunian Objects: Towards a Super-Earth in the Outer Solar System
• A warmer and wetter solution for early Mars and the challenges with transient warming
• The potential for tidally heated icy and temperate moons around exoplanets
• Dark Matter as a Trigger for Periodic Comet Impacts
• No Evidence for Lunar Transit in New Analysis of Hubble Space Telescope Observations of the Kepler-1625 System
• Candidate Members and Age Estimate of the Family of Kuiper Belt Object 2003 EL61
• The Mid-Infrared Spectrum of the Zodiacal and Exozodiacal Light
• The Anglo-Australian Planet Search. XXIII. Two New Jupiter Analogs
• Variability of the Infrared Excess of Extreme Debris Disks
• A Direct Imaging Survey of Spitzer detected debris disks: Occurrence of giant planets in dusty systems
• Planetary Collisions outside the Solar System: Time Domain Characterization of Extreme Debris Disks
• Pebble Accretion and the Diversity of Planetary Systems
• Consequences of Giant Impacts on Early Uranus for Rotation, Internal Structure, Debris, and Atmospheric Erosion
• Revisiting the proposed planetary system orbiting the eclipsing polar HU Aquarii
• Origin and Dynamical Evolution of Neptune Trojans - I: Formation and Planetary Migration
• Two extra-solar planets from the Anglo-Australian Planet Search
• Mass Extinctions and The Sun's Encounters with Spiral Arms
• A collisionless scenario for Uranus tilting
• Generation of Highly Inclined Trans-Neptunian Objects by Planet Nine
• An Oort cloud origin for the high-inclination, high-perihelion Centaurs
• Is the HR 8799 extrasolar system destined for planetary scattering?
• Terrestrial Planet Formation in the Presence of Migrating Super-earths
• The HU Aqr planetary system hypothesis revisited
• How to design a planetary system for different scattering outcomes: giant impact sweet spot, maximising exocomets, scattered disks
• Detection of Exomoons Through Observation of Radio Emissions
• Constraints on the Physical Properties of Main Belt Comet P/2013 R3 from its Breakup Event
• Record-breaking Storm Activity on Uranus in 2014
• The HOSTS survey - Exozodiacal dust measurements for 30 stars
• Discovery of a new branch of the Taurid meteoroid stream as a real source of potentially hazardous bodies
• The consequences of planetary migration on the minor bodies of the early Solar System
• The GAPS Programme with HARPS-N at TNG. III: The retrograde orbit of HAT-P-18b
• Does a Differentiated, Carbonate-Rich, Rocky Object Pollute the White Dwarf SDSSJ104341.53+085558.2?
• The comet 17P/Holmes 2007 outburst: the early motion of the outburst material
• The Dynamics of Interstellar Asteroids and Comets within the Galaxy: an Assessment of Local Candidate Source Regions for 1I/`Oumuamua and 2I/Borisov
• The cold origin of the warm dust around epsilon Eridani
• Persistent Evidence of a Jovian Mass Solar Companion in the Oort Cloud
• Habitability of Exomoons at the Hill or Tidal Locking Radius
• The production of short-lived radionuclides by new non-rotating and rotating Wolf-Rayet model stars
• The Populations of Comet-Like Bodies in the Solar system
• The Main-Belt Comets: The Pan-STARRS1 Perspective
• Exoplanetary atmospheric sodium revealed by the orbital motion. Narrow-band transmission spectroscopy of HD 189733b with UVES
• Correlations between the stellar, planetary and debris components of exoplanet systems observed by $\text{Herschel}$
• Simulations of the Population of Centaurs II: Individual Objects
• An alternative interpretation of the exomoon candidate signal in the combined Kepler and Hubble data of Kepler-1625
• Do Centaurs preserve their source inclinations?
• Qatar-2: A K dwarf orbited by a transiting hot Jupiter and a more massive companion in an outer orbit
• Second generation planet formation in NN Serpentis?
• Analysis of terrestrial planet formation by the Grand Tack model: System architecture and tack location
• Single Transit Candidates from K2: Detection and Period Estimation
• Transmission spectrum of Venus as a transiting exoplanet
• Solar Obliquity Induced by Planet Nine
• Dust growth in protoplanetary disks - a comprehensive experimental/theoretical approach
• Observations of fast-moving features in the debris disk of AU Mic on a three-year timescale: Confirmation and new discoveries
• Jupiter - friend or foe? II: the Centaurs
• A gap in HD 92945's broad planetesimal disc revealed by ALMA
• The Capture of Trojan Asteroids by the Giant Planets During Planetary Migration
• Atmospheric Chemistry of Venus-like Exoplanets
• A Detailed Analysis of the HD 73526 2:1 Resonant Planetary System
• A Second Giant Planet in 3:2 Mean-Motion Resonance in the HD 204313 System
• Finding the imprints of stellar encounters in long period comets
• Triggered Star Formation Inside the Shell of a Wolf-Rayet Bubble as the origin of the Solar System
• Telling twins apart: Exo-Earths and Venuses with transit spectroscopy
• Constraining the primordial orbits of the Terrestrial Planets
• A Nearly Polar Orbit for the Extrasolar Hot Jupiter WASP-79b
• Ultra Deep Survey for Irregular Satellites of Uranus: Limits to Completeness
• The effect of type I migration on the formation of terrestrial planets in hot-Jupiter systems
• Planet X revamped after the discovery of the Sedna-like object 2012 VP${}_{113}$?
• Collisional modelling of the AU Microscopii debris disc
• Gas and dust around A-type stars at tens of Myr:signatures of cometary breakup
• Collisional evolution of eccentric planetesimal swarms
• The size, density, and formation of the Orcus-Vanth system in the Kuiper belt
• An ancient and a primordial collisional family as the main sources of X-type asteroids of the inner Main Belt
• Comet C/2011 W3 (Lovejoy): Orbit Determination, Outbursts, Disintegration of Nucleus, Dust-Tail Morphology, and Relationship to New Cluster of Bright Sungrazers
• Excitation and depletion of the asteroid belt in the early instability scenario
• High-Temperature Processing of Solids Through Solar Nebular Bow Shocks: 3D Radiation Hydrodynamics Simulations with Particles
• A runaway Wolf-Rayet star as the origin of 26-Al in the early solar system
• Reconciling the dawn-dusk asymmetry in Mercury's exosphere with the micrometeoroid impact directionality
• The impact of a large object with Jupiter in July 2009
• The photophoretic sweeping of dust in transient protoplanetary disks
• The Neptune Trojans - a new source for the Centaurs?
• Resonant Removal of Exomoons During Planetary Migration
• A Jovian planet in an eccentric 11.5 day orbit around HD1397 discovered by TESS
• Resolving the cold debris disc around a planet-hosting star: PACS photometric imaging observations of q1 Eri (HD10647, HR506)
• The Creation of Haumea's Collisional Family
• Main-sequence progenitor configurations of the NN Ser candidate circumbinary planetary system are dynamically unstable
• Dynamical Evolution Induced by Planet Nine
• A Herschel resolved far-infrared dust ring around HD 207129
• Halting Planet Migration in the Evacuated Centers of Protoplanetary Disks
• Detection of a Water Tracer in Interstellar Comet 2I/Borisov
• First Scattered-Light Image of the Debris Disk around HD 131835 with the Gemini Planet Imager
• Jupiter's Phase Variations from Cassini: a testbed for future direct-imaging missions
• New millimeter CO observations of the gas-rich debris disks 49 Cet and HD 32297
• HATS-5b: A Transiting hot-Saturn from the HATSouth Survey
• Outer solar system possibly shaped by a stellar fly-by
• High Resolution Transmission Spectroscopy as a Diagnostic for Jovian Exoplanet Atmospheres: Constraints from Theoretical Models
• Constraining Saturn's Core Properties by a Measurement of Its Moment of Inertia - Implications to the Cassini Solstice Mission
• The dynamics of Plutinos
• Giant comets and mass extinctions of life
• ALMA Detection of Extended Millimeter Halos in the HD 32297 and HD 61005 Debris Disks
• Small Planetesimals in a Massive Disk Formed Mars
• On the formation location of Uranus and Neptune as constrained by dynamical and chemical models of comets
• Dynamical Constraints on the Origin of Main Belt Comets
• Jupiter - friend or foe? III: the Oort cloud comets
• Exploring Kepler Giant Planets in the Habitable Zone
• An Estimate of the Yield of Single-Transit Planetary Events from the Transiting Exoplanet Survey Satellite
• A Detailed Investigation of the Proposed NN Serpentis Planetary System
• The quest for companions to post-common envelope binaries IV: The 2:1 mean-motion resonance of the planets orbiting NN Serpentis
• Self-Stirring of Debris Discs by Planetesimals Formed by Pebble Concentration
• The cool and distant formation of Mars
• Resolving faint structures in the debris disk around TWA7
• Who Pulled the Trigger: a Supernova or an AGB Star?
• A Transiting Jupiter Analog
• The CORALIE survey for southern extrasolar planets XVIII. Three new massive planets and two low mass brown dwarfs at separation larger than 5 AU
• WISE J080822.18-644357.3 - a 45 Myr-old accreting M dwarf hosting a primordial disc
• Resonances Required: Dynamical Analysis of the 24 Sex and HD 200964 Planetary Systems
• Yarkovsky V-shape identification of asteroid families
• An Exo-Kuiper Belt and An Extended Halo around HD 191089 in Scattered Light
• The Fate of Scattered Planets
• Carbon monoxide in the distantly active Centaur (60558) 174P/Echeclus at 6 AU
• Extreme Debris Disk Variability -- Exploring the Diverse Outcomes of Large Asteroid Impacts During the Era of Terrestrial Planet Formation
• (1173) Anchises - Thermophysical and Dynamical Studies of a Dynamically Unstable Jovian Trojan
• Planetary Trojans - the main source of short period comets?
• Possibility of Detecting Moons of Pulsar Planets Through Time-of-Arrival Analysis
• 2001 QR322: a dynamically unstable Neptune Trojan?
• Two New Long-Period Giant Planets from the McDonald Observatory Planet Search and Two Stars with Long-Period Radial Velocity Signals Related to Stellar Activity Cycles
• Observational bias and the clustering of distant eccentric Kuiper belt objects
• SOHO Comets: 20-Years and 3,000 Objects Later
• The Lick-Carnegie Exoplanet Survey: HD32963 -- A New Jupiter Analog Orbiting a Sun-like Star
• YORP and Yarkovsky effects in asteroids (1685) Toro, (2100) Ra-Shalom, (3103) Eger, and (161989) Cacus
• The hot Jupiter period-mass distribution as a signature of in situ formation
• Near-resonance in a system of sub-Neptunes from TESS
• On the mass and origin of Chariklo's rings
• The Intrinsic Neptune Trojan Orbit Distribution: Implications for the Primordial Disk and Planet Migration
• Multiple Rings of Millimeter Dust Emission in the HD 15115 Debris Disk
• The Scattered Disc of HR 8799
• From scattered-light to millimeter emission: A comprehensive view of the Gyr-old system of HD 202628 and its eccentric debris ring
• Detection of Planetary and Stellar Companions to Neighboring Stars via a Combination of Radial Velocity and Direct Imaging Techniques
• Orbital clustering of distant Kuiper Belt Objects by hypothetical Planet 9. Secular or resonant ?
• The completeness-corrected rate of stellar encounters with the Sun from the first Gaia data release
• A Search for High Proper Motion T Dwarfs with Pan-STARRS1 + 2MASS + WISE
• A Potential Super-Venus in the Kepler-69 System
• 174P/Echeclus: a strange case of outburst
• Formation of Centaurs' rings through their partial tidal disruption during planetary encounters
• Tilting Saturn without tilting Jupiter: Constraints on giant planet migration
• The Pan-Pacific Planet Search VII: The most eccentric planet orbiting a giant star
• The Peculiar Debris Disk of HD 111520 as Resolved by the Gemini Planet Imager
• Jupiter as an exoplanet: UV to NIR transmission spectrum reveals hazes, a Na layer and possibly stratospheric H2O-ice clouds
• The Signature of the Ice Line and Modest Type I Migration in the Observed Exoplanet Mass-Semimajor Axis Distribution
• WFIRST Planet Masses from Microlens Parallax
• Planetary systems around close binary stars: the case of the very dusty, Sun-like, spectroscopic binary BD+20 307
• Insights into planet formation from debris disks: II. Giant impacts in extrasolar planetary systems
• That's the way the comet crumbles: Splitting Jupiter-family comets
• Saturn's Probable Interior: An Exploration of Saturn's Potential Interior Density Structures
• Exo-zodi modelling for the Large Binocular Telescope Interferometer
• q1 Eri: a solar-type star with a planet and a dust belt
• Confirmation of a Retrograde Orbit for Exoplanet WASP-17b
• Resolved Millimeter Observations of the HR 8799 Debris Disk
• A binary main belt comet
• Medium-sized satellites of large Kuiper belt objects
• Discovery of a Transiting Planet Near the Snow-Line
• Variations on Debris Disks III. Collisional Cascades and Giant Impacts in the Terrestrial Zones of Solar-type Stars
• The dynamical evolution of escaped Jupiter Trojan asteroids, link to other minor body populations
• Orbital clustering in the distant solar system
• Terrestrial planet formation in low eccentricity warm-Jupiter systems
• The Pan-Pacific Planet Search. IV. Two super-Jupiters in a 3:5 resonance orbiting the giant star HD33844
• Terrestrial planet formation: Dynamical shake-up and the low mass of Mars
• An updated estimate of the number of Jupiter-family comets using a simple fading law
• 3D Meteoroid Trajectories
• Triton's Evolution with a Primordial Neptunian Satellite System
• Capture of exocomets and the erosion of the Oort cloud due to stellar encounters in the Galaxy
• New disk discovered with VLT/SPHERE around the M star GSC 07396-00759
• The peculiar shapes of Saturn's small inner moons as evidence of mergers of similar-sized moonlets
• Not a simple relationship between Neptune's migration speed and Kuiper belt inclination excitation
• Detecting Water In the atmosphere of HR 8799 c with L-band High Dispersion Spectroscopy Aided By Adaptive Optics
• K2-146: Discovery of Planet c, Precise Masses from Transit Timing, and Observed Precession
• Analysis of Neptune's 2017 Bright Equatorial Storm
• The surprisingly low carbon mass in the debris disk around HD 32297
• Constraints on the pre-impact orbits of Solar System giant impactors
• Climate Modeling of a Potential ExoVenus
• AKARI/IRC 18 Micron Survey of Warm Debris Disks
• "TNOs are Cool": A survey of the trans-Neptunian region XIV. Size/albedo characterization of the Haumea family observed with Herschel and Spitzer
• Dynamical evolution of escaped plutinos, another source of Centaurs
• Exomoon Habitability and Tidal Evolution in Low-Mass Star Systems
• The Transit Transmission Spectrum of a Cold Gas Giant Planet
• The Hunt for Planet Nine: Atmosphere, Spectra, Evolution, and Detectability
• Instabilities in the Early Solar System due to a Self-gravitating Disk
• Checking the Compatibility of the Cold Kuiper Belt with a Planetary Instability Migration Model
• Pursuing the planet-debris disk connection: Analysis of upper limits from the Anglo-Australian Planet Search
• Results from the Wide Angle Search for Planets Prototype (WASP0) I: Analysis of the Pegasus Field
• Characterization of Exoplanet Atmospheres with the Optical Coronagraph on WFIRST
• Making Planet Nine: A Scattered Giant in the Outer Solar System
• Planetesimals and Satellitesimals: Formation of the Satellite Systems
• Enstatite-rich Warm Debris Dust around HD165014
• Where the Solar system meets the solar neighbourhood: patterns in the distribution of radiants of observed hyperbolic minor bodies
• Dynamical Constraints on Mercury's Collisional Origin
• Did the ancient egyptians record the period of the eclipsing binary Algol - the Raging one?
• Giga-Year Evolution of Jupiter Trojans and the Asymmetry Problem
• Jumping Jupiter can explain Mercury's orbit
• Predicting the incidence of planets and debris discs as a function of stellar mass
• 2008 LC18: a potentially unstable Neptune Trojan
• The Anglo-Australian Planet Search XXV: A Candidate Massive Saturn Analog Orbiting HD 30177
• Is there more than meets the eye? Presence and role of submicron grains in debris discs
• Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets
• Spitzer Detection of the Transiting Jupiter-analog Exoplanet Kepler-167e
• Constraining the Formation of the Four Terrestrial Planets in the Solar System
• The dynamical evolution of dwarf planet (136108) Haumea's collisional family: General properties and implications for the trans-Neptunian belt
• Jupiter - Friend or Foe? IV: The influence of orbital eccentricity and inclination
• Revised Exoplanet Radii and Habitability Using Gaia Data Release 2
• Large retrograde Centaurs: visitors from the Oort cloud?
• A Dynamical Investigation of the Proposed BD +20 2457 System
• Bayes' theorem and early solar short-lived radionuclides: the case for an unexceptional origin for the solar system
• Constraints from deuterium on the formation of icy bodies in the Jovian system and beyond
• Theoretical Reflectance Spectra of Earth-Like Planets through Their Evolutions: Impact of Clouds on the Detectability of Oxygen, Water, and Methane with Future Direct Imaging Missions
• Resolved Spectroscopy of a Brown Dwarf Binary at the T Dwarf/Y Dwarf Transition
• HD 104860 and HD 192758: two debris disks newly imaged in scattered-light with HST
• Gravitational scattering by giant planets
• Exploring the role of the Sun's motion in terrestrial comet impacts
• The orbital architecture and debris disks of the HR 8799 planetary system
• Biases in Cometary Catalogues and Planet X
• No Timing Variations Observed in Third Transit of Snow-Line Exoplanet Kepler-421b
• Herschel Observations of Dusty Debris Disks
• Assessment of different formation scenarios for the ring system of (10199) Chariklo
• Dynamical Evolution of the Earth-Moon Progenitors - Whence Theia?
• Is there a circumbinary planet around NSVS 14256825?
• Yarkovsky-Driven Spreading of the Eureka Family of Mars Trojans
• Rocky Planetesimal Formation Aided by Organics
• The Mysterious Dimmings of the T Tauri Star V1334 Tau
• Effects of photophoresis on the evolution of transitional circumstellar disks
• The Dynamical History of Chariklo and its Rings
• The effect of orbital evolution on the Haumea (2003 EL61) collisional family
• Detecting the Signatures of Uranus and Neptune
• Observational Window Functions in Planet Transit Surveys
• The Transit Spectra of Earth and Jupiter
• Planetary Embryo Bow Shocks as a Mechanism for Chondrule Formation
• Mass Extinction And The Structure Of The Milky Way
• An Oort cloud origin of the Halley-type comets
• Maximum Angular Separation Epochs for Exoplanet Imaging Observations
• Multiwavelength observations of a bright impact flash during the January 2019 total lunar eclipse
• Could Jupiter or Saturn Have Ejected a Fifth Giant Planet?
• Parameter degeneracies and (un)predictability of gravitational microlensing events
• Quantifying the Influence of Jupiter on the Earth's Orbital Cycles
• Small impacts on the giant planet Jupiter
• Interpreting the extended emission around three nearby debris disc host stars
• Comprehensive analysis of HD 105, a young Solar System analog
• The conjectured S-type retrograde planet in nu Octantis: more evidence including four years of iodine-cell radial velocities
• Imaging an 80 AU Radius Dust Ring Around the F5V Star HD 157587
• A Quantitative Criterion for Defining Planets
• First Resolved Scattered-Light Images of Four Debris Disks in Scorpius-Centaurus with the Gemini Planet Imager
• On the location of the ring around the dwarf planet Haumea
• The Influence of Outer Solar System Architecture on the Structure and Evolution of the Oort Cloud
• Transits of extrasolar moons around luminous giant planets
• Predictions on the core mass of Jupiter and of giant planets in general
• Prospecting for exo-Earths in multiple planet systems with a gas giant
• Impact-driven planetary desiccation: The origin of the dry Venus
• Photophoretic transport of hot minerals in the solar nebula
• It takes two planets in resonance to tango around K2-146
• Modeling the Formation of the Family of the Dwarf Planet Haumea
• The 2019 Taurid resonant swarm: prospects for ground detection of small NEOs
• Modelling the Inner Debris Disc of HR 8799
• The Applegate mechanism in Post-Common-Envelope Binaries: Investigating the role of rotation
• High-resolution Imaging of the Gegenschein and the Geometric Albedo of Interplanetary Dust
• Dust Spreading in Debris Discs: Do Small Grains Cling on to Their Birth Environment?
• Predicting multiple planet stability and habitable zone companions in the TESS era
• The shape of (7) Iris as evidence of an ancient large impact?
• Initial velocity V-shapes of young asteroid families
• Properties of the single Jovian planet population and the pursuit of Solar system analogues
• The galactic unclassified B[e] star HD 50138 III. The short-term line profile variability of its photospheric lines
• Impact of planetesimal eccentricities and material strength on the appearance of eccentric debris disks
• The HD 181433 Planetary System: Dynamics and a New Orbital Solution
• Physical properties of the extreme centaur and super-comet candidate 2013 AZ60
• Stable habitable zones of single Jovian planet systems
• The Absence of Cold Dust around Warm Debris Disk Star HD 15407A
• Enhanced activity of the Southern Taurids in 2005 and 2015
• Rebirth of X-ray Emission from the Born-Again Planetary Nebula A 30
• Results from the Wide Angle Search for Planets Prototype (WASP0) III: Planet Hunting in the Draco Field
• Results from the Wide Angle Search for Planets Prototype (WASP0) II: Stellar Variability in the Pegasus Field
• Hot debris dust around HD 106797
• On collisional capture rates of irregular satellites around the gas-giant planets and the minimum mass of the solar nebula
• A 3pi Search for Planet Nine at 3.4 microns with WISE and NEOWISE
• Migrating Jupiter up to the habitable zone: Earth-like planet formation and water delivery
• Precovery of TESS Single Transits with KELT
• Cladistical analysis of the Jovian and Saturnian satellite systems
• On the Formation of Super-Earths with Implications for the Solar System
• Population of SOHO/STEREO Kreutz Sungrazers and the Arrival of Comet C/2011 W3 (Lovejoy)
• Characterizing the Chemistry of Planetary Materials Around White Dwarf Stars
• A Six-Planet System Around the Star HD 34445
• The Surface Magnetic Activity of the Weak-Line T Tauri Stars TWA 9A and V1095 Sco
• An Orbital Stability Study of the Proposed Companions of SW Lyncis
• Trans-Neptunian objects as natural probes to the unknown solar system
• Occultations of astrophysical radio sources as probes of planetary environments: A case study of Jupiter and possible applications to exoplanets
• The Dynamical History Of 2060 Chiron And Its Proposed Ring System
• First detection of submillimeter-wave [13C I] 3P1-3P0 emission in a gaseous debris disk of 49 Ceti with ALMA
• The Relationship between Centaurs and Jupiter Family Comets with Implications for K-Pg-type Impacts
• On the RZ Draconis Sub-stellar Circumbinary Companions Stability Study of the Proposed Sub-stellar Circumbinary System
• Rising from Ashes or Dying Flash? Mega Outburst of Small Comet 289P/Blanpain in 2013
• Stability analysis of three exoplanet systems

Cited by in corpus (20)

• The Demographics of Terrestrial Planets in the Venus Zone
• On the radial distribution of giant exoplanets at Solar System scales
• Atmospheric Dynamics of a Near Tidally Locked Earth-Size Planet
• Combining astrometry and JUICE -- Europa Clipper radio science to improve the ephemerides of the Galilean moons
• Spinning up a Daze: TESS Uncovers a Hot Jupiter orbiting the Rapid-Rotator TOI-778
• HD 83443c: A highly eccentric giant planet on a 22-year orbit
• Evidence for the disruption of a planetary system during the formation of the Helix Nebula
• HD 183579b: A Warm Sub-Neptune Transiting a Solar Twin Detected by TESS
• Theoretical constraints imposed by gradient detection and dispersal on microbial size in astrobiological environments
• Astrocladistics of the Jovian Trojan Swarms
• Multi-wavelength aperture polarimetry of debris disc host stars
• The Stability of Uranus Trojans Over the Age of the Solar System
• A thermophysical and dynamical study of the Hildas (1162) Larissa and (1911) Schubart
• A sub-Neptune transiting the young field star HD 18599 at 40 pc
• Testing the Impact of Planet-stirring, Self-stirring, and Mixed-stirring on Debris Disc Architecture: A Case Study of HD 16743
• The Dynamical Viability of an Extended Jupiter Ring System
• The TESS-Keck Survey. XIX. A Warm Transiting Sub-Saturn Mass Planet and a non-Transiting Saturn Mass Planet Orbiting a Solar Analog
• AU Mic b is the Youngest Planet to have a Spin-Orbit Alignment Measurement
• The Longest-period Young Transiting Exoplanets. A Duo of Puffy Giants inside a Debris Disk
• A Near-Earth Object Model Calibrated to Earth Impactors