| 1 | Dynamics of the <i>β</i> Pictoris planetary system and its falling evaporating bodies | 5.9 | 13 | Citations (PDF) |
| 2 | Dating the Solar System’s giant planet orbital instability using enstatite meteorites | 36.4 | 20 | Citations (PDF) |
| 3 | The Solar System could have formed in a low-viscosity disc: A dynamical study from giant planet migration to the Nice model | 5.9 | 12 | Citations (PDF) |
| 4 | Formation and evolution of a protoplanetary disk: Combining observations, simulations, and cosmochemical constraints | 5.9 | 20 | Citations (PDF) |
| 5 | Breakdown of planetary systems in embedded clusters | 4.7 | 16 | Citations (PDF) |
| 6 | In situ enrichment in heavy elements of hot Jupiters | 5.9 | 14 | Citations (PDF) |
| 7 | Identification of a 4.3 billion year old asteroid family and planetesimal population in the Inner Main Belt | 5.9 | 11 | Citations (PDF) |
| 8 | Migration of Jupiter mass planets in discs with laminar accretion flows | 5.9 | 20 | Citations (PDF) |
| 9 | Dynamical origin of the Dwarf Planet Ceres | 2.8 | 16 | Citations (PDF) |
| 10 | Stochastic accretion of the Earth | 13.2 | 37 | Citations (PDF) |
| 11 | A re-assessment of the Kuiper belt size distribution for sub-kilometer objects, revealing collisional equilibrium at small sizes | 2.8 | 39 | Citations (PDF) |
| 12 | Migration of Jupiter-mass planets in low-viscosity discs | 5.9 | 35 | Citations (PDF) |
| 13 | Formation of planetary systems by pebble accretion and migration | 5.9 | 157 | Citations (PDF) |
| 14 | Constraints on Planetesimal Accretion Inferred from Particle-size Distribution in CO Chondrites | 11.4 | 20 | Citations (PDF) |
| 15 | Common feedstocks of late accretion for the terrestrial planets | 13.2 | 18 | Citations (PDF) |
| 16 | Probing the impact of varied migration and gas accretion rates for the formation of giant planets in the pebble accretion scenario | 4.7 | 22 | Citations (PDF) |
| 17 | Terrestrial planet formation from lost inner solar system material | 11.0 | 118 | Citations (PDF) |
| 18 | Dynamical evidence for an early giant planet instability | 2.8 | 85 | Citations (PDF) |
| 19 | Isotopic Evolution of the Inner Solar System Inferred from Molybdenum Isotopes in Meteorites | 11.4 | 64 | Citations (PDF) |
| 20 | No evidence for interstellar planetesimals trapped in the Solar system | 3.9 | 27 | Citations (PDF) |
| 21 | On the Origin and Evolution of the Material in 67P/Churyumov-Gerasimenko | 5.4 | 55 | Citations (PDF) |
| 22 | Effects of early intense bombardment on megaregolith evolution and on lunar (and planetary) surface samples | 2.0 | 11 | Citations (PDF) |
| 23 | The Non-carbonaceous–Carbonaceous Meteorite Dichotomy | 5.4 | 163 | Citations (PDF) |
| 24 | Formation of Giant Planet Satellites | 5.2 | 80 | Citations (PDF) |
| 25 | Planet formation by pebble accretion in ringed disks | 5.9 | 78 | Citations (PDF) |
| 26 | Origin and Evolution of Cometary Nuclei | 5.4 | 38 | Citations (PDF) |
| 27 | A low-mass planet candidate orbiting Proxima Centauri at a distance of 1.5 AU | 11.0 | 73 | Citations (PDF) |
| 28 | Subsolar Al/Si and Mg/Si ratios of non-carbonaceous chondrites reveal planetesimal formation during early condensation in the protoplanetary disk | 4.8 | 42 | Citations (PDF) |
| 29 | A study of 3-dimensional shapes of asteroid families with an application to Eos | 2.8 | 9 | Citations (PDF) |
| 30 | Formation of planetary systems by pebble accretion and migration | 5.9 | 225 | Citations (PDF) |
| 31 | Ancient and primordial collisional families as the main sources of X-type asteroids of the inner main belt | 5.9 | 49 | Citations (PDF) |
| 32 | Are the Moon's Nearside‐Farside Asymmetries the Result of a Giant Impact? | 3.6 | 53 | Citations (PDF) |
| 33 | Formation of planetary systems by pebble accretion and migration: growth of gas giants | 5.9 | 150 | Citations (PDF) |
| 34 | Dynamical effects on the classical Kuiper belt during the excited-Neptune model | 2.8 | 7 | Citations (PDF) |
| 35 | Compositional distributions and evolutionary processes for the near-Earth object population: Results from the MIT-Hawaii Near-Earth Object Spectroscopic Survey (MITHNEOS) | 2.8 | 194 | Citations (PDF) |
| 36 | Debiased orbit and absolute-magnitude distributions for near-Earth objects | 2.8 | 232 | Citations (PDF) |
| 37 | The timeline of the lunar bombardment: Revisited | 2.8 | 236 | Citations (PDF) |
| 38 | Reconstructing the size distribution of the primordial Main Belt | 2.8 | 25 | Citations (PDF) |
| 39 | Toward a new paradigm for Type II migration | 5.9 | 65 | Citations (PDF) |
| 40 | Why do protoplanetary disks appear not massive enough to form the known exoplanet population? | 5.9 | 217 | Citations (PDF) |
| 41 | Pebble-isolation mass: Scaling law and implications for the formation of super-Earths and gas giants | 5.9 | 264 | Citations (PDF) |
| 42 | Formation of the terrestrial planets in the solar system around 1 au via radial concentration of planetesimals | 5.9 | 32 | Citations (PDF) |
| 43 | Size-dependent modification of asteroid family Yarkovsky V-shapes | 5.9 | 17 | Citations (PDF) |
| 44 | How primordial is the structure of comet 67P? | 5.9 | 52 | Citations (PDF) |
| 45 | Cometary impact rates on the Moon and planets during the late heavy bombardment | 5.9 | 19 | Citations (PDF) |
| 46 | Yarkovsky V-shape identification of asteroid families | 2.8 | 40 | Citations (PDF) |
| 47 | Secular orbital evolution of Jupiter family comets | 5.9 | 23 | Citations (PDF) |
| 48 | Origin and Evolution of Short-period Comets | 5.2 | 142 | Citations (PDF) |
| 49 | Breaking the chains: hot super-Earth systems from migration and disruption of compact resonant chains | 4.7 | 343 | Citations (PDF) |
| 50 | Magnitude and timing of the giant planet instability: A reassessment from the perspective of the asteroid belt | 5.9 | 12 | Citations (PDF) |
| 51 | The radial dependence of pebble accretion rates: A source of diversity in planetary systems | 5.9 | 147 | Citations (PDF) |
| 52 | Evolution of protoplanetary discs with magnetically driven disc winds | 5.9 | 185 | Citations (PDF) |
| 53 | Is the Grand Tack model compatible with the orbital distribution of main belt asteroids? | 2.8 | 50 | Citations (PDF) |
| 54 | Challenges in planet formation | 3.6 | 148 | Citations (PDF) |
| 55 | Fossilized condensation lines in the Solar System protoplanetary disk | 2.8 | 179 | Citations (PDF) |
| 56 | Origins of volatile elements (H, C, N, noble gases) on Earth and Mars in light of recent results from the ROSETTA cometary mission | 4.8 | 172 | Citations (PDF) |
| 57 | The structure of protoplanetary discs around evolving young stars | 5.9 | 260 | Citations (PDF) |
| 58 | Dynamical Problems in Extrasolar Planetary Science | 0.0 | 0 | Citations (PDF) |
| 59 | The great dichotomy of the Solar System: Small terrestrial embryos and massive giant planet cores | 2.8 | 217 | Citations (PDF) |
| 60 | Accretion of Uranus and Neptune from inward-migrating planetary embryos blocked by Jupiter and Saturn | 5.9 | 74 | Citations (PDF) |
| 61 | A reassessment of the in situ formation of close-in super-Earths | 5.9 | 106 | Citations (PDF) |
| 62 | Terrestrial planet formation constrained by Mars and the structure of the asteroid belt | 4.7 | 108 | Citations (PDF) |
| 63 | GAS GIANT PLANETS AS DYNAMICAL BARRIERS TO INWARD-MIGRATING SUPER-EARTHS | 11.4 | 112 | Citations (PDF) |
| 64 | Comets as collisional fragments of a primordial planetesimal disk | 5.9 | 79 | Citations (PDF) |
| 65 | Suppression of type I migration by disk winds | 5.9 | 41 | Citations (PDF) |
| 66 | Separating gas-giant and ice-giant planets by halting pebble accretion | 5.9 | 376 | Citations (PDF) |
| 67 | Stellar irradiated discs and implications on migration of embedded planets | 5.9 | 89 | Citations (PDF) |
| 68 | Migration of Earth-sized planets in 3D radiative discs | 4.7 | 105 | Citations (PDF) |
| 69 | TERRESTRIAL PLANET FORMATION IN THE PRESENCE OF MIGRATING SUPER-EARTHS | 5.2 | 65 | Citations (PDF) |
| 70 | The Grand Tack model: a critical review | 0.0 | 34 | Citations (PDF) |
| 71 | THE ABSOLUTE MAGNITUDE DISTRIBUTION OF KUIPER BELT OBJECTS | 5.2 | 226 | Citations (PDF) |
| 72 | Lunar and terrestrial planet formation in the Grand Tack scenario | 2.6 | 106 | Citations (PDF) |
| 73 | Earth-like habitats in planetary systems | 1.6 | 37 | Citations (PDF) |
| 74 | Origin of the peculiar eccentricity distribution of the inner cold Kuiper belt | 2.8 | 28 | Citations (PDF) |
| 75 | Meridional circulation of gas into gaps opened by giant planets in three-dimensional low-viscosity disks | 2.8 | 127 | Citations (PDF) |
| 76 | Constraining the cratering chronology of Vesta | 1.6 | 48 | Citations (PDF) |
| 77 | Stellar irradiated discs and implications on migration of embedded planets | 5.9 | 54 | Citations (PDF) |
| 78 | Oort cloud and Scattered Disc formation during a late dynamical instability in the Solar System | 2.8 | 213 | Citations (PDF) |
| 79 | The Eos family halo | 2.8 | 38 | Citations (PDF) |
| 80 | CAPTURE OF TROJANS BY JUMPING JUPITER | 5.2 | 231 | Citations (PDF) |
| 81 | Constraining the cometary flux through the asteroid belt during the late heavy bombardment | 5.9 | 117 | Citations (PDF) |
| 82 | A METHOD TO CONSTRAIN THE SIZE OF THE PROTOSOLAR NEBULA | 5.0 | 22 | Citations (PDF) |
| 83 | STATISTICAL STUDY OF THE EARLY SOLAR SYSTEM'S INSTABILITY WITH FOUR, FIVE, AND SIX GIANT PLANETS | 5.0 | 325 | Citations (PDF) |
| 84 | Dynamical capture in the Pluto–Charon system | 1.3 | 16 | Citations (PDF) |
| 85 | Building Terrestrial Planets | 10.9 | 440 | Citations (PDF) |
| 86 | The onset of the lunar cataclysm as recorded in its ancient crater populations | 4.8 | 112 | Citations (PDF) |
| 87 | A sawtooth-like timeline for the first billion years of lunar bombardment | 4.8 | 250 | Citations (PDF) |
| 88 | Dynamics of pebbles in the vicinity of a growing planetary embryo: hydro-dynamical simulations | 5.9 | 177 | Citations (PDF) |
| 89 | Did the Hilda collisional family form during the late heavy bombardment? | 4.7 | 47 | Citations (PDF) |
| 90 | LATE ORBITAL INSTABILITIES IN THE OUTER PLANETS INDUCED BY INTERACTION WITH A SELF-GRAVITATING PLANETESIMAL DISK | 5.0 | 221 | Citations (PDF) |
| 91 | A coherent and comprehensive model of the evolution of the outer Solar System | 1.0 | 39 | Citations (PDF) |
| 92 | THE IRREGULAR SATELLITES: THE MOST COLLISIONALLY EVOLVED POPULATIONS IN THE SOLAR SYSTEM | 5.0 | 118 | Citations (PDF) |
| 93 | EVIDENCE FROM THE ASTEROID BELT FOR A VIOLENT PAST EVOLUTION OF JUPITER'S ORBIT | 5.0 | 206 | Citations (PDF) |
| 94 | Constructing the secular architecture of the solar system II: the terrestrial planets | 5.9 | 135 | Citations (PDF) |
| 95 | Building the terrestrial planets: Constrained accretion in the inner Solar System | 2.8 | 398 | Citations (PDF) |
| 96 | Asteroids were born big | 2.8 | 468 | Citations (PDF) |
| 97 | Did Saturn's rings form during the Late Heavy Bombardment? | 2.8 | 116 | Citations (PDF) |
| 98 | Considerations on the magnitude distributions of the Kuiper belt and of the Jupiter Trojans | 2.8 | 58 | Citations (PDF) |
| 99 | Constructing the secular architecture of the solar system | 5.9 | 92 | Citations (PDF) |
| 100 | Origin of the structure of the Kuiper belt during a dynamical instability in the orbits of Uranus and Neptune | 2.8 | 421 | Citations (PDF) |
| 101 | ON A SCATTERED-DISK ORIGIN FOR THE 2003 EL<sub>61</sub>COLLISIONAL FAMILY—AN EXAMPLE OF THE IMPORTANCE OF COLLISIONS ON THE DYNAMICS OF SMALL BODIES | 5.0 | 55 | Citations (PDF) |
| 102 | Capture of Irregular Satellites during Planetary Encounters | 5.0 | 201 | Citations (PDF) |
| 103 | Dynamics of the Giant Planets of the Solar System in the Gaseous Protoplanetary Disk and Their Relationship to the Current Orbital Architecture | 5.0 | 293 | Citations (PDF) |
| 104 | Models of the collisional damping scenario for ice-giant planets and Kuiper belt formation | 2.8 | 39 | Citations (PDF) |
| 105 | The dynamics of Jupiter and Saturn in the gaseous protoplanetary disk | 2.8 | 227 | Citations (PDF) |
| 106 | The primordial excitation and clearing of the asteroid belt—Revisited | 2.8 | 157 | Citations (PDF) |
| 107 | Cavity opening by a giant planet in a protoplanetary disc and effects on planetary migration | 4.7 | 171 | Citations (PDF) |
| 108 | Disk Surface Density Transitions as Protoplanet Traps | 5.2 | 309 | Citations (PDF) |
| 109 | Yarkovsky/YORP chronology of asteroid families | 2.8 | 172 | Citations (PDF) |
| 110 | Terrestrial planet formation with strong dynamical friction | 2.8 | 401 | Citations (PDF) |
| 111 | The population of faint Jupiter family comets near the Earth | 2.8 | 30 | Citations (PDF) |
| 112 | On the width and shape of gaps in protoplanetary disks | 2.8 | 542 | Citations (PDF) |
| 113 | Yarkovsky footprints in the Eos family | 2.8 | 97 | Citations (PDF) |
| 114 | The population of Near Earth Asteroids in coorbital motion with Venus | 2.8 | 24 | Citations (PDF) |
| 115 | The fossilized size distribution of the main asteroid belt | 2.8 | 530 | Citations (PDF) |
| 116 | Planetary migration in a planetesimal disk: why did Neptune stop at 30 AU? | 2.8 | 205 | Citations (PDF) |
| 117 | The Yarkovsky-driven origin of near-Earth asteroids | 2.8 | 137 | Citations (PDF) |
| 118 | The Flora Family: A Case of the Dynamically Dispersed Collisional Swarm? | 2.8 | 143 | Citations (PDF) |
| 119 | Numerous Weak Resonances Drive Asteroids toward Terrestrial Planets Orbits | 2.8 | 169 | Citations (PDF) |
| 120 | Dynamical Lifetimes of Objects Injected into Asteroid Belt Resonances | 36.4 | 417 | Citations (PDF) |
| 121 | Slow crossing of a stochastic layer | 2.9 | 14 | Citations (PDF) |