Debris disks as signposts of terrestrial planet formation
Open accessAbstract
There exists strong circumstantial evidence from their eccentric orbits that most of the known extra-solar planetary systems are the survivors of violent dynamical instabilities. Here we explore the effect of giant planet instabilities on the formation and survival of terrestrial planets. We numerically simulate the evolution of planetary systems around Sun-like stars that include three components: (i) an inner disk of planetesimals and planetary embryos; (ii) three giant planets at Jupiter-Saturn distances; and (iii) an outer disk of planetesimals comparable to estimates of the primitive Kuiper belt. We calculate the dust production and spectral energy distribution of each system by assuming that each planetesimal particle represents an ensemble of smaller bodies in collisional equilibrium. Our main result is a strong correlation between the evolution of the inner and outer parts of planetary systems, i.e. between the presence of terrestrial planets and debris disks. Strong giant planet instabilities – that produce very eccentric surviving planets – destroy all rocky material in the system, including fully-formed terrestrial planets if the instabilities occur late, and also destroy the icy planetesimal population. Stable or weakly unstable systems allow terrestrial planets to accrete in their inner regions and significant dust to be produced in their outer regions, detectable at mid-infrared wavelengths as debris disks. Stars older than ~100 Myr with bright cold dust emission (in particular at λ ~ 70 μm) signpost dynamically calm environments that were conducive to efficient terrestrial accretion. Such emission is present around ~16% of billion-year old Solar-type stars. Our simulations yield numerous secondary results: 1) the typical eccentricities of as-yet undetected terrestrial planets are ~0.1 but there exists a novel class of terrestrial planet system whose single planet undergoes large amplitude oscillations in orbital eccentricity and inclination; 2) by scaling our systems to match the observed semimajor axis distribution of giant exoplanets, we predict that terrestrial exoplanets in the same systems should be a few times more abundant at ~0.5 AU than giant or terrestrial exoplanets at 1 AU; 3) the Solar System appears to be unusual in terms of its combination of a rich terrestrial planet system and a low dust content. This may be explained by the weak, outward-directed instability that is thought to have caused the late heavy bombardment.
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Planet-planet scattering among gas giant planets likely produces a pulse of ejected planetesimals.
“while planet-planet scattering among gas giant planets is likely to produce a pulse of ejected planetesimals (Raymond et al. 2011;Marzari 2014)”
From Implications for Planetary System Formation from Interstellar Object 1I/2017 U1 (‘Oumuamua) (2017) · cites this paper as Raymond et al. 2011
Systems with gas giants on stable orbits can eject planetesimals on longer timescales.
“and while systems with gas giants on stable orbits can eject planetesimals on longer timescales (Raymond et al. 2011;Barclay et al. 2017)”
From Implications for Planetary System Formation from Interstellar Object 1I/2017 U1 (‘Oumuamua) (2017) · cites this paper as Raymond et al. 2011
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A Search for Protoplanetary Disks Around Naked T Tauri Stars
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Debris disc stirring by secular perturbations from giant planets
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Self-citationHABITABLE CLIMATES: THE INFLUENCE OF ECCENTRICITY
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Self-citationNew Debris Disks around Nearby Main-Sequence Stars: Impact on the Direct Detection of Planets
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Gas Disks to Gas Giants: Simulating the Birth of Planetary Systems
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Accretion in the Early Kuiper Belt. I. Coagulation and Velocity Evolution
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Constructing the secular architecture of the solar system II: the terrestrial planets
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High Orbital Eccentricities of Extrasolar Planets Induced by the Kozai Mechanism
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PLANETS AND DEBRIS DISKS: RESULTS FROM ASPITZER/MIPS SEARCH FOR INFRARED EXCESS
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Self-citationIncidence and survival of remnant disks around main-sequence stars
Habing, H. J., Dominik, C., De Muizon, M. J., Laureijs, R. J., Kessler, M. F., Leech, K. J., Metcalfe, L., Salama, A., Siebenmorgen, R., Trams, N. R., et al. (2000) · UvA-DARE (University of Amsterdam) · doi:10.1051/0004-6361:20000075/pdf · Cited by 145 · see citing works
Nearby debris disk systems with high fractional luminosity reconsidered
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Circumstellar material in the Vega inner system revealed by CHARA/FLUOR
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Prospects for Detection of Catastrophic Collisions in Debris Disks
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Final Stages of Planet Formation
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Evolution of planetary systems in resonance
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Fragmentation model dependence of collision cascades
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Detecting the Dusty Debris of Terrestrial Planet Formation
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Terrestrial Planet Formation. I. The Transition from Oligarchic Growth to Chaotic GrowthPreprint
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Formation of Terrestrial Planets from Protoplanets. I. Statistics of Basic Dynamical Properties
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Formation of Earth-like Planets During and After Giant Planet Migration
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Giant planet migration through the action of disk torques and planet–planet scattering
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STELLAR MASS DEPENDENT DISK DISPERSAL
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PLANET-PLANET SCATTERING IN PLANETESIMAL DISKS
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Self-citationThe history of the Solar system's debris disc: observable properties of the Kuiper belt
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Self-citationMean Motion Resonances from Planet-Planet Scattering
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Self-citationCircumstellar material in the Vega inner system revealed by CHARA/FLUORPreprint
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Debris disc stirring by secular perturbations from giant planetsPreprint
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Self-citationTurbulence Implies that Mean Motion Resonances are Rare
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PLANET-PLANET SCATTERING LEADS TO TIGHTLY PACKED PLANETARY SYSTEMS
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Self-citationFar‐Infrared Properties of M Dwarfs
Gautier, T. N., III, Rieke, G. H., Stansberry, J., Bryden, G., Stapelfeldt, K. R., Werner, M. W., Beichman, C., Chen, C., Su, K. Y. L., Trilling, D. E., et al. (2007) · The Astrophysical Journal · doi:10.1086/520667 · Cited by 105 · see citing works
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Williams, D. M., & Pollard, D. (2003) · International Journal of Astrobiology · doi:10.1017/s1473550403001356 · Cited by 105 · see citing works
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Self-citationThe Role of Giant Planets in Terrestrial Planet Formation
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The Size–Frequency Distribution of the Zodiacal Cloud: Evidence from the Solar System Dust Bands
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Proplyds and Massive Disks in the Orion Nebula Cluster Imaged with CARMA and SMA
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Formation of Earth-like Planets During and After Giant Planet Migration
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Self-citationEvolution of Planetary Systems in Resonance
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A NEW HYBRIDN-BODY-COAGULATION CODE FOR THE FORMATION OF GAS GIANT PLANETS
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GENERALIZED MILANKOVITCH CYCLES AND LONG-TERM CLIMATIC HABITABILITY
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Statistical Properties of Exoplanets
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Detecting the Dusty Debris of Terrestrial Planet Formation
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Post-main-sequence evolution of A star debris discs
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The Stellar Mass-Accretion Rate Relation in T Tauri Stars and Brown Dwarfs
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Self-citationON THE RELATIONSHIP BETWEEN DEBRIS DISKS AND PLANETS
Kóspál, Á., Ardila, D. R., Moór, A., & Ábrahám, P. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/700/2/l73 · Cited by 66 · see citing works
Resolving the hot dust around HD69830 and η Corvi with MIDI and VISIR
Smith, R., Wyatt, M. C., & Haniff, C. A. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200911626 · Cited by 65 · see citing works
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Cold DUst around NEarby Stars (DUNES). First results
Eiroa, C., Fedele, D., Maldonado, J., González-García, B. M., Rodmann, J., Heras, A. M., Pilbratt, G. L., Augereau, J. ‐., Mora, A., Montesinos, B., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201014594 · Cited by 63 · see citing works
Influence of an inner disc on the orbital evolution of massive planets migrating in resonance
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On the formation of terrestrial planets in hot-Jupiter systems
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Collisional evolution of eccentric planetesimal swarms
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Self-citationDUST IN THE INNER REGIONS OF DEBRIS DISKS AROUND A STARS
Akeson, R. L., Ciardi, D. R., Millan-Gabet, R., Mérand, A., Folco, E. D., Monnier, J. D., Beichman, C. A., Absil, O., Aufdenberg, J., McAlister, H., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/691/2/1896 · Cited by 54 · see citing works
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Self-citationThe detectability of extrasolar terrestrial and giant planets during their luminous final accretion
Stern, S. A. (1994) · The Astronomical Journal · doi:10.1086/117243 · Cited by 46 · see citing works
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Self-citationMetallicity, debris discs and planets
Greaves, J., Fischer, D., & Wyatt, M. (2006) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09848.x · Cited by 44 · see citing works
Self-citationThe clearing of discs around late-type T Tauri stars: constraints from the infrared two-colour plane
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FORMING CLOSE-IN EARTH-LIKE PLANETS VIA A COLLISION-MERGER MECHANISM IN LATE-STAGE PLANET FORMATION
Ji, J., Jin, S., & Tinney, C. G. (2010) · The Astrophysical Journal Letters · doi:10.1088/0004-637x/727/1/l5 · Cited by 37 · see citing works
Distribution of Circumstellar Disk Masses in the Young Cluster NGC 2024
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Dust in the inner regions of debris disks around A starsPreprint
Akeson, R., Ciardi, D. R., Millan-Gabet, R., Mérand, A., Folco, E. D., Monnier, J. D., Beichman, C., Absil, O., Aufdenberg, J. P., McAlister, H. A., et al. (2012) · Cited by 35 · see citing works
Orbital Stability of a Protoplanet System under a Drag Force Proportional to the Random Velocity
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The Gas-Drag Effect on the Orbital Instability of a Protoplanet System
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MEAN MOTION RESONANCES IN EXTRASOLAR PLANETARY SYSTEMS WITH TURBULENCE, INTERACTIONS, AND DAMPING
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Forming Close-in Earth-like Planets via a Collision-Merger Mechanism in Late-stage Planet FormationPreprint
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Predicting the incidence of planet and debris discs as a function of stellar mass
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Detecting Exoplanets in the Presence of Exozodiacal Dust ProfilesPreprint
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Steady-state evolution of debris disks around solar-type starsPreprint
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Self-citation
Flagged first, then by citations
Research works printed but not linked: 2
- Armitage, P. J. 2011, ARA&A, in press
- Ford, E. B., Rasio, F. A., & Yu, K. 2003, in Scientific Frontiers in Research on Extrasolar Planets, ed. D. Deming, & S. Seager, ASP Conf. Ser., 294, 181
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Perryman, M. A. C. (2011) · Cambridge University Press eBooks · doi:10.1017/9781108304160 · Cited by 343 · see citing works
SOAR TESS Survey. I. Sculpting of TESS Planetary Systems by Stellar Companions
Ziegler, C., Tokovinin, A. A., Briceño, C. A., Mang, J. J., Law, N., & Mann, A. W. (2019) · The Astronomical Journal · doi:10.3847/1538-3881/ab55e9 · Cited by 267 · see citing works
Formation of planetary systems by pebble accretion and migration: growth of gas giants
Bitsch, B., Izidoro, A., Johansen, A., Raymond, S. N., Morbidelli, A., Lambrechts, M., & Jacobson, S. A. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201834489 · Cited by 181 · see citing works
Self-citationThe empty primordial asteroid belt
Raymond, S. N., & Izidoro, A. (2017) · Science Advances · doi:10.1126/sciadv.1701138 · Cited by 153 · see citing works
Self-citationThe Nature and Origins of Sub‐Neptune Size Planets
Bean, J. L., Raymond, S. N., & Owen, J. E. (2020) · Journal of Geophysical Research Planets · doi:10.1029/2020je006639 · Cited by 152 · see citing works
Self-citationHot super-Earths and giant planet cores from different migration histories
Cossou, C., Raymond, S. N., Hersant, F., & Pierens, A. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201424157 · Cited by 149 · see citing works
Self-citationDebris from terrestrial planet formation: the Moon-forming collision
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Self-citationTHE DESTRUCTION OF INNER PLANETARY SYSTEMS DURING HIGH-ECCENTRICITY MIGRATION OF GAS GIANTS
Mustill, A. J., Davies, M. B., & Johansen, A. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/808/1/14 · Cited by 135 · see citing works
Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems
Wyatt, M. C., Kennedy, G. M., Sibthorpe, B., Moro‐Martín, A., Lestrade, J.-F., Ivison, R. J., Matthews, B. C., Udry, S., Greaves, J. S., Kalas, P., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21298.x · Cited by 127 · see citing works
Self-citationPlanet–planet scattering alone cannot explain the free-floating planet population
Veras, D., & Raymond, S. N. (2012) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1111/j.1745-3933.2012.01218.x · Cited by 130 · see citing works
Self-citationHot super-Earths and giant planet cores from different migration histories
Cossou, C., Raymond, S. N., Hersant, F., & Pierens, A. (2014) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201424157/pdf · Cited by 128 · see citing works
Self-citationTHE GEMINI PLANET-FINDING CAMPAIGN: THE FREQUENCY OF GIANT PLANETS AROUND DEBRIS DISK STARS
Wahhaj, Z., Liu, M. C., Nielsen, E. L., Biller, B. A., Hayward, T. L., Close, L. M., Males, J. R., Skemer, A. J. I., Ftaclas, C., Chun, M., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/773/2/179 · Cited by 125 · see citing works
Debris disks as signposts of terrestrial planet formation
Raymond, S. N., Armitage, P. J., Moro‐Martín, A., Booth, M., Wyatt, M. C., Armstrong, J., Mandell, A. M., Selsis, F., & West, A. A. (2012) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201117049 · Cited by 110 · see citing works
Self-citationDISK RADII AND GRAIN SIZES INHERSCHEL-RESOLVED DEBRIS DISKS
Pawellek, N., Krivov, A. V., Marshall, J. P., Montesinos, B., Ábrahám, P., Moór, A., Bryden, G., & Eiroa, C. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/792/1/65 · Cited by 116 · see citing works
Unstable low-mass planetary systems as drivers of white dwarf pollution
Mustill, A. J., Villaver, E., Veras, D., Gänsicke, B. T., & Bonsor, A. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty446 · Cited by 115 · see citing works
Detectable close-in planets around white dwarfs through late unpacking
Veras, D., & Gänsicke, B. T. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2475 · Cited by 108 · see citing works
Kopparapu, R. K., Wolf, E. T., & Meadows, V. S. (2005) · University of Arizona Press eBooks · doi:10.2458/azu_uapress_9780816540068 · Cited by 116 · see citing works
The effects of dynamical interactions on planets in young substructured star clusters
Parker, R. J., & Quanz, S. P. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19911.x · Cited by 108 · see citing works
Dynamical evidence for an early giant planet instability
de Sousa, R. R., Morbidelli, A., Raymond, S. N., Izidoro, A., Gomes, R. S., & Neto, E. V. (2019) · Icarus · doi:10.1016/j.icarus.2019.113605 · Cited by 102 · see citing works
Self-citationDETAILED ABUNDANCES OF THE SOLAR TWINS 16 CYGNI A AND B: CONSTRAINING PLANET FORMATION MODELS
Schuler, S. C., Cunha, K., Smith, V. V., Ghezzi, L., King, J. R., Deliyannis, C. P., & Boesgaard, A. M. (2011) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/737/2/l32 · Cited by 97 · see citing works
SPITZER EVIDENCE FOR A LATE-HEAVY BOMBARDMENT AND THE FORMATION OF UREILITES IN η CORVI At ∼1 Gyr
Lisse, C. M., Wyatt, M. C., Chen, C. H., Morlok, A., Watson, D. M., Manoj, P., Sheehan, P., Currie, T. M., Thébault, P., & Sitko, M. L. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/747/2/93 · Cited by 92 · see citing works
Self-citationPRECISE INFRARED RADIAL VELOCITIES FROM KECK/NIRSPEC AND THE SEARCH FOR YOUNG PLANETS
Bailey, J., White, R., Blake, C., Charbonneau, D., Barman, T., Tanner, A., & Torres, G. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/749/1/16 · Cited by 62 · see citing works
Metallicity of solar-type stars with debris discs and planets
Maldonado, J., Eiroa, C., Villaver, E., Montesinos, B., & Mora, A. (2012) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201218800 · Cited by 93 · see citing works
PLANET FORMATION AROUND BINARY STARS: TATOOINE MADE EASY
Bromley, B. C., & Kenyon, S. J. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/806/1/98 · Cited by 92 · see citing works
Bitsch, B., Raymond, S., & Izidoro, A. (2019) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201935007 · Cited by 69 · see citing works
Self-citationThe effects of dynamical interactions on planets in young substructured star clusters
Parker, R. J., & Quanz, S. P. (2012) · reroDoc Digital Library · doi:10.3929/ethz-b-000046402 · Cited by 89 · see citing works
Moro‐Martín, A., Marshall, J. P., Kennedy, G. M., Sibthorpe, B., Matthews, B. C., Eiroa, C., Wyatt, M. C., Lestrade, J.-F., Maldonado, J., Rodriguez, D. R., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/801/2/143 · Cited by 85 · see citing works
Self-citationA DEBRIS disk around the planet hosting M-star GJ 581 spatially resolved withHerschel
Lestrade, J.-F., Matthews, B. C., Sibthorpe, B., Kennedy, G. M., Wyatt, M. C., Bryden, G., Greaves, J. S., Thilliez, E., Moro‐Martín, A., Booth, M., et al. (2012) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201220325 · Cited by 87 · see citing works
Self-citationPerryman, M. A. C. (2018) · Cambridge University Press eBooks · doi:10.1017/9781108304160.017 · Cited by 89 · see citing works
Primordial Origins of Earth's Carbon
Marty, B. M., Alexander, C. M. O., & Raymond, S. N. (2013) · Reviews in Mineralogy and Geochemistry · doi:10.2138/rmg.2013.75.6 · Cited by 86 · see citing works
Self-citationBonsor, A., Raymond, S. N., Augereau, J. ‐., & Ormel, C. W. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu721 · Cited by 79 · see citing works
Self-citationFull-lifetime simulations of multiple unequal-mass planets across all phases of stellar evolution
Veras, D., Mustill, A. J., Gänsicke, B. T., Redfield, S., Georgakarakos, N., Bowler, A. B., & Lloyd, M. J. S. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw476 · Cited by 82 · see citing works
Planet Formation: Key Mechanisms and Global Models
Raymond, S. N., & Morbidelli, A. (2022) · Astrophysics and space science library · doi:10.1007/978-3-030-88124-5_1 · Cited by 99 · see citing works
Self-citationMustill, A. J., Davies, M. B., & Johansen, A. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx693 · Cited by 80 · see citing works
Solution to the debris disc mass problem: planetesimals are born small?
Krivov, A. V., & Wyatt, M. C. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa2385 · Cited by 79 · see citing works
Self-citationEFFECTS OF DYNAMICAL EVOLUTION OF GIANT PLANETS ON SURVIVAL OF TERRESTRIAL PLANETS
Matsumura, S., Ida, S., & Nagasawa, M. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/767/2/129 · Cited by 79 · see citing works
Raymond, S. N., Armitage, P. J., Veras, D., Quintana, E. V., & Barclay, T. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty468 · Cited by 78 · see citing works
Self-citationHERSCHEL's “COLD DEBRIS DISKS”: BACKGROUND GALAXIES OR QUIESCENT RIMS OF PLANETARY SYSTEMS?
Krivov, A. V., Eiroa, C., Löhne, T., Marshall, J. P., Montesinos, B., del Burgo, C., Absil, O., Ardila, D. R., Augereau, J. ‐., Bayo, A., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/772/1/32 · Cited by 74 · see citing works
Implications for Planetary System Formation from Interstellar Object 1I/2017 U1 (‘Oumuamua)
Trilling, D. E., Robinson, T., Roegge, A., Chandler, C. O., Smith, N., Loeffler, M., Trujillo, C., Navarro-Meza, S., & Glaspie, L. M. (2017) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/aa9989 · Cited by 76 · see citing works
THE CURIOUS CASE OF ELEMENTAL ABUNDANCE DIFFERENCES IN THE DUAL HOT JUPITER HOSTS WASP-94A AND B*
Teske, J. K., Khanal, S., & Ramírez, I. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/819/1/19 · Cited by 73 · see citing works
Planet–planet scattering as the source of the highest eccentricity exoplanets
Carrera, D., Raymond, S. N., & Davies, M. B. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201935744 · Cited by 73 · see citing works
Self-citationKral, Q., Thébault, P., & Charnoz, S. (2013) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321398 · Cited by 73 · see citing works
Bitsch, B., Raymond, S. N., & Izidoro, A. (2019) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201935007/pdf · Cited by 72 · see citing works
Self-citationDynamical and collisional constraints on a stochastic late veneer on the terrestrial planets
Raymond, S. N., Schlichting, H. E., Hersant, F., & Selsis, F. (2013) · Icarus · doi:10.1016/j.icarus.2013.06.019 · Cited by 70 · see citing works
Self-citationTeske, J. K., Ghezzi, L., Cunha, K., Smith, V. V., Schuler, S. C., & Bergemann, M. (2015) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/801/1/l10 · Cited by 70 · see citing works
THE COMPOSITIONAL DIVERSITY OF EXTRASOLAR TERRESTRIAL PLANETS. II. MIGRATION SIMULATIONS
Bond, J. C., O'Brien, D. P., & Raymond, S. N. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/760/1/44 · Cited by 69 · see citing works
Self-citationSearching for signatures of planet formation in stars with circumstellar debris discs
Maldonado, J., Eiroa, C., Villaver, E., Montesinos, B., & Mora, A. (2015) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201525764 · Cited by 68 · see citing works
The GAPS programme with HARPS-N at TNG
Biazzo, K., Gratton, R., Desidera, S., Lucatello, S., Sozzetti, A., Bonomo, A. S., Damasso, M., Gandolfi, D., Affer, L., Boccato, C., et al. (2015) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201526375 · Cited by 68 · see citing works
Debris from terrestrial planet formation: the Moon-forming collision
Jackson, A. P., & Wyatt, M. C. (2015) · Cited by 83 · see citing works
Self-citationPREDICTIONS FOR SHEPHERDING PLANETS IN SCATTERED LIGHT IMAGES OF DEBRIS DISKS
Rodigas, T. J., Malhotra, R., & Hinz, P. M. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/780/1/65 · Cited by 67 · see citing works
Bonsor, A., Raymond, S. N., & Augereau, J. ‐. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt933 · Cited by 65 · see citing works
Self-citationSolar System Physics for Exoplanet Research
Horner, J., Kane, S. R., Marshall, J. P., Dalba, P. A., Holt, T. R., Wood, J., Maynard-Casely, H. E., Wittenmyer, R., Lykawka, P. S., Hill, M., et al. (2020) · Publications of the Astronomical Society of the Pacific · doi:10.1088/1538-3873/ab8eb9 · Cited by 68 · see citing works
Marshall, J. P., Moro‐Martín, A., Eiroa, C., Kennedy, G. M., Mora, A., Sibthorpe, B., Lestrade, J.-F., Maldonado, J., Sanz‐Forcada, J., Wyatt, M. C., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201323058 · Cited by 61 · see citing works
Self-citationMack, C. E., Schuler, S. C., Stassun, K. G., & Norris, J. E. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/787/2/98 · Cited by 59 · see citing works
PLANETESIMALS IN DEBRIS DISKS OF SUN-LIKE STARS
Shannon, A., & Wu, Y. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/739/1/36 · Cited by 55 · see citing works
Cieza, L. A., Olofsson, J., Harvey, P. M., Evans, N. J., Najita, J., Henning, T. K., Merín, B., Liebhart, A., Güdel, M., Augereau, J. ‐., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/762/2/100 · Cited by 55 · see citing works
Damasso, M., Biazzo, K., Bonomo, A., Desidera, S., Lanza, A. F., Nascimbeni, V., Esposito, M., Scandariato, G., Sozzetti, A., Cosentino, R., et al. (2015) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201425332 · Cited by 59 · see citing works
Confusion limited surveys: usingWISEto quantify the rarity of warm dust aroundKeplerstars
Kennedy, G. M., & Wyatt, M. C. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21621.x · Cited by 54 · see citing works
Self-citationMetallicity of solar-type stars with debris discs and planets
Maldonado, J., Eiroa, C., Villaver, E., Montesinos, B., & Mora, A. (2012) · LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) · doi:10.1051/0004-6361/201218800/pdf · Cited by 54 · see citing works
TERRESTRIAL PLANET FORMATION DURING THE MIGRATION AND RESONANCE CROSSINGS OF THE GIANT PLANETS
Lykawka, P. S., & Itô, T. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/773/1/65 · Cited by 53 · see citing works
Harrison, T. M. (2020) · doi:10.1007/978-3-030-46687-9 · Cited by 53 · see citing works
Vega's hot dust from icy planetesimals scattered inwards by an outward-migrating planetary system
Raymond, S. N., & Bonsor, A. (2014) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/slu048 · Cited by 52 · see citing works
Self-citationIs there an exoplanet in the solar system?
Mustill, A. J., Raymond, S. N., & Davies, M. B. (2016) · Monthly Notices of the Royal Astronomical Society: Letters · doi:10.1093/mnrasl/slw075 · Cited by 52 · see citing works
Self-citationDesch, S. J., & Jackson, A. P. (2021) · Journal of Geophysical Research Planets · doi:10.1029/2020je006807 · Cited by 52 · see citing works
Inner mean-motion resonances with eccentric planets: a possible origin for exozodiacal dust clouds
Faramaz, V., Ertel, S., Booth, M., Cuadra, J., & Simmonds, C. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2846 · Cited by 50 · see citing works
Self-citationPlanet–planet scattering as the source of the highest eccentricity exoplanets
Carrera, D., Raymond, S. N., & Davies, M. B. (2019) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201935744/pdf · Cited by 50 · see citing works
Self-citationThe Demographics of Rocky Free-floating Planets and their Detectability by WFIRST
Barclay, T., Quintana, E. V., Raymond, S. N., & Penny, M. T. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa705b · Cited by 48 · see citing works
Self-citationALMA Discovery of Dust Belts around Proxima Centauri
Anglada, G., Amado, P., Ortiz, J. L., Gómez, J. F., Macías, E., Alberdi, A., Osorio, M., Gómez, J., de Gregorio-Monsalvo, I., P'erez-Torres, M., et al. (2017) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/aa978b · Cited by 35 · see citing works
Formation of planetary systems by pebble accretion and migration: growth of gas giants
Bitsch, B., Izidoro, A., Johansen, A., Raymond, S. N., Morbidelli, A., Lambrechts, M., & Jacobson, S. A. (2019) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201834489/pdf · Cited by 47 · see citing works
Self-citationInterstellar Object ’Oumuamua as an Extinct Fragment of an Ejected Cometary Planetesimal
Raymond, S. N., Armitage, P. J., & Veras, D. (2018) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/aab4f6 · Cited by 47 · see citing works
Self-citationYoudin, A. N., & Kenyon, S. J. (2013) · Springer eBooks · doi:10.1007/978-94-007-5606-9_1 · Cited by 51 · see citing works
Influence of planetary gas accretion on the shape and depth of gaps in protoplanetary discs
Bergez-Casalou, C., Bitsch, B., Pierens, A., Crida, A., & Raymond, S. N. (2020) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202038304 · Cited by 43 · see citing works
Self-citationSolar System Physics for Exoplanet Research
Horner, J., Kane, S. R., Marshall, J. P., Dalba, P. A., Holt, T. R., Wood, J., Maynard-Casely, H. E., Wittenmyer, R. A., Lykawka, P. S., Hill, M. L., et al. (2020) · Cited by 42 · see citing works
FORMATION OF SUPER-EARTH MASS PLANETS AT 125–250 AU FROM A SOLAR-TYPE STAR
Kenyon, S. J., & Bromley, B. C. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/806/1/42 · Cited by 41 · see citing works
Mini-Oort clouds: compact isotropic planetesimal clouds from planet–planet scattering
Raymond, S. N., & Armitage, P. J. (2012) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/sls033 · Cited by 41 · see citing works
Self-citationSurvival of habitable planets in unstable planetary systems
Carrera, D., Davies, M. B., & Johansen, A. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2218 · Cited by 41 · see citing works
The Demographics of Rocky Free-floating Planets and their Detectability by WFIRST
Barclay, T., Quintana, E. V., Raymond, S. N., & Penny, M. T. (2017) · Civil War Book Review · Cited by 41 · see citing works
Self-citationMoore, A., & Quillen, A. C. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sts625 · Cited by 38 · see citing works
High-resolution ALMA and HST images of q1 Eri: an asymmetric debris disc with an eccentric Jupiter
Lovell, J. B., Marino, S., Wyatt, M. C., Kennedy, G. M., MacGregor, M. A., Stapelfeldt, K. R., Dent, B., Krist, J., Matrà, L., Kral, Q., et al. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab1678 · Cited by 38 · see citing works
Self-citationTheGaia-ESO Survey: chemical signatures of rocky accretion in a young solar-type star
Spina, L., Palla, F., Randich, S., Sacco, G. G., Jeffries, R. D., Magrini, L., Franciosini, E., Meyer, M. R., Tautvaišienė, G., Gilmore, G. F., et al. (2015) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201526896 · Cited by 38 · see citing works
BANYAN. VIII. NEW LOW-MASS STARS AND BROWN DWARFS WITH CANDIDATE CIRCUMSTELLAR DISKS
Boucher, A., Lafreniére, D., Gagné, J., Malo, L., Faherty, J. K., Doyon, R., & Chen, C. H. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/832/1/50 · Cited by 38 · see citing works
Lawler, S., Francesco, J. D., Kennedy, G. M., Sibthorpe, B., Booth, M., Vandenbussche, B. K., Matthews, B. C., Holland, W. S., Greaves, J. S., Wilner, D. J., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu1641 · Cited by 37 · see citing works
Self-citationTeske, J. K., Ghezzi, L., Cunha, K., Smith, V. V., Schuler, S. C., & Bergemann, M. (2015) · Max Planck Institute for Plasma Physics · Cited by 37 · see citing works
Searching for signatures of planet formation in stars with circumstellar debris discs
Maldonado, J., Eiroa, C., Villaver, E., Montesinos, B., & Mora, A. (2015) · LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) · doi:10.1051/0004-6361/201525764/pdf · Cited by 37 · see citing works
Innocent Bystanders: Orbital Dynamics of Exomoons During Planet–Planet Scattering
Hong, Y.-C., Raymond, S. N., Nicholson, P. D., & Lunine, J. I. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aaa0db · Cited by 37 · see citing works
Self-citationNew disk discovered with VLT/SPHERE around the M star GSC 07396−00759
Sissa, E., Olofsson, J., Vigan, A., Augereau, J. ‐., D’Orazi, V., Desidera, S., Gratton, R., Langlois, M., Rigliaco, E., Boccaletti, A., et al. (2018) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201832740 · Cited by 36 · see citing works
Kenyon, S. J., & Bromley, B. C. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/817/1/51 · Cited by 35 · see citing works
HD 80606: searching for the chemical signature of planet formation
Saffe, C., Flores, M., & Buccino, A. (2015) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201526644 · Cited by 34 · see citing works
Plausible Home Stars of the Interstellar Object ‘Oumuamua Found in Gaia DR2
Bailer‐Jones, C. A. L., Farnocchia, D., Meech, K. J., Brasser, R., Micheli, M., Chakrabarti, S., Buie, M. W., & Hainaut, O. (2018) · The Astronomical Journal · doi:10.3847/1538-3881/aae3eb · Cited by 34 · see citing works
Influence of planetary gas accretion on the shape and depth of gaps in protoplanetary discs
Bergez-Casalou, C., Bitsch, B., Pierens, A., Crida, A., & Raymond, S. N. (2020) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/202038304/pdf · Cited by 34 · see citing works
Self-citationExtrasolar planets and false atmospheric biosignatures: The role of micrometeoroids
Court, R., & Sephton, M. (2012) · Planetary and Space Science · doi:10.1016/j.pss.2012.08.026 · Cited by 11 · see citing works
Habitability in Different Milky Way Stellar Environments: A Stellar Interaction Dynamical Approach
Jiménez-Torres, J. J., Pichardo, B., Lake, G., & Segura, A. (2013) · Astrobiology · doi:10.1089/ast.2012.0842 · Cited by 32 · see citing works
ALMA observations of the multiplanet system 61 Vir: what lies outside super-Earth systems?
Marino, S., Wyatt, M. C., Kennedy, G. M., Holland, W. S., Matrà, L., Shannon, A., & Ivison, R. J. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1102 · Cited by 32 · see citing works
Self-citationHD 80606: Searching for the chemical signature of planet formation
Saffe, C., Flores, M., & Buccino, A. P. (2015) · Americanae (AECID Library) · doi:10.1051/0004-6361/201526644/pdf · Cited by 32 · see citing works
ROCKY PLANET FORMATION: QUICK AND NEAT
Kenyon, S. J., Najita, J. R., & Bromley, B. C. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/831/1/8 · Cited by 31 · see citing works
CROWDING-OUT OF GIANTS BY DWARFS: AN ORIGIN FOR THE LACK OF COMPANION PLANETS IN HOT JUPITER SYSTEMS
Ogihara, M., Inutsuka, S., & Kobayashi, H. (2013) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/778/1/l9 · Cited by 30 · see citing works
Stirring up the dust: a dynamical model for halo-like dust clouds in transitional disks
Krijt, S., & Dominik, C. (2011) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201116757 · Cited by 30 · see citing works
Was Planet 9 captured in the Sun’s natal star-forming region?
Parker, R. J., Lichtenberg, T., & Quanz, S. P. (2017) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/slx141 · Cited by 30 · see citing works
Zain, P., de Elía, G. D., Ronco, M. P., & Guilera, O. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201730848 · Cited by 20 · see citing works
Did Jupiter's core form in the innermost parts of the Sun's protoplanetary disc?
Raymond, S. N., Izidoro, A., Bitsch, B., & Jacobson, S. A. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw431 · Cited by 27 · see citing works
Self-citation
- Authors
- Raymond, S. N., Armitage, P. J., Moro-Martín, A., Booth, M., Wyatt, M. C., Armstrong, J. C., Mandell, A. M., Selsis, F., & West, A. A.
- Affiliations
- Centre National de la Recherche Scientifique (FR)
- Joint Institute for Laboratory Astrophysics (US)
- University of Victoria (CA)
- University of Cambridge (GB)
- Weber State University (US)
- Goddard Space Flight Center (US)
- Boston University (US)
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2011-05-12
- Volume
- 530
- Pages
- A62
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W1964193027
- Cited by
- 194
- References
- 184
- Citations by year
- 2026: 2 · 2025: 5 · 2024: 6 · 2023: 4 · 2022: 4 · 2021: 7 · 2020: 13 · 2019: 12 · 2018: 41 · 2017: 11 · 2016: 12 · 2015: 15 · 2014: 13 · 2013: 20 · 2012: 15
- FWCI
- 9.52
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Astronomy and Astrophysics (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- HAL (submittedVersion)
- Oskar-Bordeaux (Universite de Bordeaux) (submittedVersion)
- Funders
- National Science Foundation (0807471)
- National Aeronautics and Space Administration (NNX07AH08G, NNX09AB90G)
- Purdue University
- Weber State University
- University of Washington
- Centre National de la Recherche Scientifique
- NASA Astrobiology Institute
- Science and Technology Facilities Council (ST/H00243X/1, ST/G00269X/1)
- Division of Astronomical Sciences
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Keywords
- debris disks, terrestrial planet formation, giant planet instability, dynamical instability, dust formation, mid-infrared dust emission, eccentric planets, terrestrial exoplanets, giant exoplanets, Kuiper belt analog, Late Heavy Bombardment, solar-type stars
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
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