Cited by 194Stellar, planetary, and galactic studiesAstro and Planetary ScienceAstrophysics and Star Formation Studies

The DOI matches its Crossref record; 186 of the 186 references it cites were found in a registry or an index.

Debris disks as signposts of terrestrial planet formation

Open access

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.·2011·Astronomy & Astrophysics

DOI 10.1051/0004-6361/201116456

Open this paper in CoChat — free account Open PDF

Abstract

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.

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

Integrity signals

Registry

Crossref · 10.1051/0004-6361/201116456

Cites

186 of 186 references verified0 citation errors · 0 not checkable

Statistics

Claims the paper makes

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
Pollack, J. B., Hubickyj, O., Bodenheimer, P. H., Lissauer, J. J., Podolak, M., & Greenzweig, Y. (1996) · Icarus · doi:10.1006/icar.1996.0190 · Cited by 3,152
Secular perturbations of asteroids with high inclination and eccentricity
Kozai, Y. (1962) · The Astronomical Journal · doi:10.1086/108790 · Cited by 2,588
Habitable Zones around Main Sequence Stars
Kasting, J. F., Whitmire, D. P., & Reynolds, R. T. (1993) · Icarus · doi:10.1006/icar.1993.1010 · Cited by 2,501 · cited 1×
“The terrestrial planet’s final mass is 0.72 M⊕ and its semimajor axis of 0.935 AU places it in the circumstellar habitable zone (Kasting et al. 1993; Selsis et al. 2007).”
BackgroundInfluential
A hybrid symplectic integrator that permits close encounters between massive bodies
Chambers, J. E. (1999) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.1999.02379.x · Cited by 1,820
Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets
Gomes, R., Levison, H. F., Tsiganis, K., & Morbidelli, A. (2005) · Nature · doi:10.1038/nature03676 · Cited by 1,737
Disk frequencies and lifetimes in Young clusters
Haisch, Jr., Lada, E. A., & Lada, C. J. (2001) · The Astrophysical Journal · doi:10.1086/320685 · Cited by 1,723
The Planet‐Metallicity Correlation
Fischer, D. A., & Valenti, J. A. (2005) · The Astrophysical Journal · doi:10.1086/428383 · Cited by 1,641
Origin of the orbital architecture of the giant planets of the Solar System
Tsiganis, K., Gomes, R., Morbidelli, A., & Levison, H. F. (2005) · Nature · doi:10.1038/nature03539 · Cited by 1,476
A low mass for Mars from Jupiter’s early gas-driven migration
Walsh, K. J., Morbidelli, A., Raymond, S. N., O'Brien, D. P., & Mandell, A. M. (2011) · Nature · doi:10.1038/nature10201 · Cited by 1,241
Self-citation
Collisional model of asteroids and their debris
Dohnanyi, J. S. (1969) · Journal of Geophysical Research Atmospheres · doi:10.1029/jb074i010p02531 · Cited by 1,220
Layered Accretion in T Tauri Disks
Gammie, C. F. (1996) · The Astrophysical Journal · doi:10.1086/176735 · Cited by 1,215
Symplectic maps for the n-body problem
Wisdom, J., & Holman, M. J. (1991) · The Astronomical Journal · doi:10.1086/115978 · Cited by 1,205
Dynamical Instabilities and the Formation of Extrasolar Planetary Systems
Rasio, F. A., & Ford, E. B. (1996) · Science · doi:10.1126/science.274.5289.954 · Cited by 1,203
Disk Frequencies and Lifetimes in Young Clusters
Haisch, K. E., & Lada, C. J. (2001) · CERN Document Server (European Organization for Nuclear Research) · Cited by 1,074
Dynamical Outcomes of Planet‐Planet Scattering
Chatterjee, S., Ford, E. B., Matsumura, S., & Rasio, F. A. (2008) · The Astrophysical Journal · doi:10.1086/590227 · Cited by 964
Evolution of Debris Disks
Wyatt, M. C. (2008) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.45.051806.110525 · Cited by 927
Self-citation
Catalog of Nearby Exoplanets
Butler, R. P., Wright, J. T., Marcy, G. W., Fischer, D. A., Vogt, S. S., Tinney, C. G., Jones, H. R. A., Carter, B. D., Johnson, J. A., McCarthy, C., et al. (2006) · The Astrophysical Journal · doi:10.1086/504701 · Cited by 914
The Keck Planet Search: Detectability and the Minimum Mass and Orbital Period Distribution of Extrasolar Planets
Cumming, A., Butler, R. P., Marcy, G. W., Vogt, S. S., Wright, J. T., & Fischer, D. A. (2008) · Publications of the Astronomical Society of the Pacific · doi:10.1086/588487 · Cited by 892
Catastrophic Disruptions Revisited
Benz, W. (1999) · Icarus · doi:10.1006/icar.1999.6204 · Cited by 851
The distribution of mass in the planetary system and solar nebula
Weidenschilling, S. (1977) · Astrophysics and Space Science · doi:10.1007/bf00642464 · Cited by 718
Circumstellar Dust Disks in Taurus-Auriga: The Submillimeter Perspective
Andrews, S., & Williams, J. P. (2005) · The Astrophysical Journal · doi:10.1086/432712 · Cited by 693
Models of giant planet formation with migration and disc evolution
Alibert, Y., Mordasini, C., Benz, W., & Winisdoerffer, C. (2005) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20042032 · Cited by 685
Dynamics of Systems of Two Close Planets
Gladman, B. (1993) · Icarus · doi:10.1006/icar.1993.1169 · Cited by 641
The Occurrence and Mass Distribution of Close-in Super-Earths, Neptunes, and Jupiters
Howard, A. W., Marcy, G. W., Johnson, J. A., Fischer, D. A., Wright, J. T., Isaacson, H., Valenti, J. A., Anderson, J., Lin, D. N. C., & Ida, S. (2010) · Science · doi:10.1126/science.1194854 · Cited by 635
Statistical Properties of Exoplanets
Udry, S., & Santos, N. C. (2007) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.45.051806.110529 · Cited by 622
Transiting exoplanets from the CoRoT space mission
Leger, A. M., Rouan, D., Schneider, J. L., Barge, P., Fridlund, M. C., Samuel, B., Ollivier, M., Guenther, E. W., Deleuil, M., Deeg, H. J., et al. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200911933 · Cited by 608
Dynamical Origin of Extrasolar Planet Eccentricity Distribution
Jurić, M., & Tremaine, S. D. (2008) · The Astrophysical Journal · doi:10.1086/590047 · Cited by 584
The Stability of Multi-Planet Systems
Chambers, J., Wetherill, G. W., & Boss, A. P. (1996) · Icarus · doi:10.1006/icar.1996.0019 · Cited by 557
Making More Terrestrial Planets
Chambers, J. (2001) · Icarus · doi:10.1006/icar.2001.6639 · Cited by 557
The fossilized size distribution of the main asteroid belt
Bottke, W., Durda, D., Nesvorný, D., Jedicke, R., Morbidelli, A., Vokrouhlický, D., & Levison, H. (2003) · Icarus · doi:10.1016/j.icarus.2004.10.026 · Cited by 552
Gravitational scattering as a possible origin for giant planets at small stellar distances
WEIDENSCHILLING, S. J., & Marzari, F. (1996) · Nature · doi:10.1038/384619a0 · Cited by 551
COMETARY ORIGIN OF THE ZODIACAL CLOUD AND CARBONACEOUS MICROMETEORITES. IMPLICATIONS FOR HOT DEBRIS DISKS
Nesvorný, D., Jenniskens, P. M., Levison, H. F., Bottke, W. F., Vokrouhlický, D., & Gounelle, M. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/713/2/816 · Cited by 535
KEPLER'S FIRST ROCKY PLANET: KEPLER-10b
Batalha, N. M., Borucki, W. J., Bryson, S. T., Buchhave, L. A., Caldwell, D. A., Christensen-Dalsgaard, J., Ciardi, D., Dunham, E. W., Fressin, F., Gautier, T. N., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/729/1/27 · Cited by 531
Habitable planets around the star Gliese 581?
Selsis, F., Kasting, J. F., Levrard, B., Paillet, J., Ribas, I., & Delfosse, X. (2007) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20078091 · Cited by 527
Self-citation
Dynamics and Origin of the 2 : 1 Orbital Resonances of the GJ 876 Planets
Lee, M. H., & Peale, S. J. (2002) · The Astrophysical Journal · doi:10.1086/338504 · Cited by 525
The stellar metallicity—giant planet connection
González, G. (1997) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/285.2.403 · Cited by 517
The metal-rich nature of stars with planets
Santos, N. C., Israelian, G., & Mayor, M. (2001) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20010648 · Cited by 502
On the Luminosity of Young Jupiters
Marley, M. S., Fortney, J. J., Hubickyj, O., Bodenheimer, P. H., & Lissauer, J. J. (2007) · The Astrophysical Journal · doi:10.1086/509759 · Cited by 502
Planet Formation around Stars of Various Masses: The Snow Line and the Frequency of Giant Planets
Kennedy, G. M., & Kenyon, S. J. (2008) · The Astrophysical Journal · doi:10.1086/524130 · Cited by 488
Toward a Deterministic Model of Planetary Formation. III. Mass Distribution of Short‐Period Planets around Stars of Various Masses
Ida, S., & Lin, D. N. C. (2005) · The Astrophysical Journal · doi:10.1086/429953 · Cited by 481
Hf–W–Th evidence for rapid growth of Mars and its status as a planetary embryo
Dauphas, N., & Pourmand, A. (2011) · Nature · doi:10.1038/nature10077 · Cited by 476
Timescales for planetary accretion and the structure of the protoplanetary disk
Lissauer, J. J. (1987) · Icarus · doi:10.1016/0019-1035(87)90104-7 · Cited by 468
Terrestrial planet formation with strong dynamical friction
OBRIEN, D., MORBIDELLI, A., & LEVISON, H. (2006) · Icarus · doi:10.1016/j.icarus.2006.04.005 · Cited by 467
The HARPS search for southern extra-solar planets
Udry, S., Bonfils, X., Delfosse, X., Forveille, T., Mayor, M., Perrier, C., Bouchy, F., Lovis, C., Pepe, F. A., Queloz, D. P., et al. (2007) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20077612 · Cited by 460
Forming Planetesimals in Solar and Extrasolar Nebulae
Chiang, E., & Youdin, A. N. (2010) · Annual Review of Earth and Planetary Sciences · doi:10.1146/annurev-earth-040809-152513 · Cited by 446
Building the terrestrial planets: Constrained accretion in the inner Solar System
Raymond, S. N., O’Brien, D. P., Morbidelli, A., & Kaib, N. A. (2009) · Icarus · doi:10.1016/j.icarus.2009.05.016 · Cited by 437
Self-citation
High‐Resolution Submillimeter Constraints on Circumstellar Disk Structure
Andrews, S. M., & Williams, J. P. (2007) · The Astrophysical Journal · doi:10.1086/511741 · Cited by 426
Binarity in Brown Dwarfs: T Dwarf Binaries Discovered with theHubble Space TelescopeWide Field Planetary Camera 2
Burgasser, A. J., Kirkpatrick, J. D., Reid, I. N., Brown, M. E., Miskey, C. L., & Gizis, J. E. (2003) · The Astrophysical Journal · doi:10.1086/346263 · Cited by 420
The Origin of Planetary Impactors in the Inner Solar System
STROM, R. G., Malhotra, R., Itô, T., Yoshida, F., & KRING, D. A. (2005) · Science · doi:10.1126/science.1113544 · Cited by 418
Formation of Protoplanet Systems and Diversity of Planetary Systems
Kokubo, E., & Ida, S. (2002) · The Astrophysical Journal · doi:10.1086/344105 · Cited by 417
How Observations of Circumstellar Disk Asymmetries Can Reveal Hidden Planets: Pericenter Glow and Its Application to the HR 4796 Disk
Wyatt, M. C., Dermott, S. F., Telesco, C. M., Fisher, R. S., Grogan, K., Holmes, E. K., & Pina, R. K. (1999) · The Astrophysical Journal · doi:10.1086/308093 · Cited by 410
Self-citation
Making other earths: dynamical simulations of terrestrial planet formation and water delivery
Raymond, S., Quinn, T., & Lunine, J. (2003) · Icarus · doi:10.1016/j.icarus.2003.11.019 · Cited by 403
Self-citation
Debris Disk Evolution around A Stars
Su, K. Y. L., Rieke, G. H., Stansberry, J. A., Bryden, G., Stapelfeldt, K. R., Trilling, D. E., Muzerolle, J., Beichman, C. A., Moro‐Martin, A., Hines, D. C., et al. (2006) · The Astrophysical Journal · doi:10.1086/508649 · Cited by 385
High-resolution simulations of the final assembly of Earth-like planets I. Terrestrial accretion and dynamics
Raymond, S. N., Quinn, T., & Lunine, J. I. (2006) · Icarus · doi:10.1016/j.icarus.2006.03.011 · Cited by 383
Self-citation
THE LUMINOSITY AND MASS FUNCTIONS OF LOW-MASS STARS IN THE GALACTIC DISK. II. THE FIELD
Bochanski, J. J., Hawley, S. L., Covey, K. R., West, A. A., Reid, I. N., Golimowski, D. A., & Ivezić, Ž. (2010) · The Astronomical Journal · doi:10.1088/0004-6256/139/6/2679 · Cited by 356
Self-citation
Transience of Hot Dust around Sun‐like Stars
Wyatt, M. C., Smith, R., Greaves, J. S., Beichman, C., Bryden, G., & Lisse, C. M. (2007) · The Astrophysical Journal · doi:10.1086/510999 · Cited by 334
Self-citation
Kepler's First Rocky Planet: Kepler-10b
Seager, S. (2010) · DSpace@MIT (Massachusetts Institute of Technology) · Cited by 332
A Submillimeter View of Circumstellar Dust Disks in ρ Ophiuchi
Andrews, S. M., & Williams, J. P. (2007) · The Astrophysical Journal · doi:10.1086/522885 · Cited by 328
Debris Disks around Sun‐like Stars
Trilling, D. E., Bryden, G., Beichman, C. A., Rieke, G. H., Su, K. Y. L., Stansberry, J. A., Blaylock, M., Stapelfeldt, K. R., Beeman, J. W., & Haller, E. E. (2008) · The Astrophysical Journal · doi:10.1086/525514 · Cited by 314
THE LICK-CARNEGIE EXOPLANET SURVEY: A URANUS-MASS FOURTH PLANET FOR GJ 876 IN AN EXTRASOLAR LAPLACE CONFIGURATION
Rivera, E. J., Laughlin, G., Butler, R. P., Vogt, S. S., Haghighipour, N., & Meschiari, S. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/719/1/890 · Cited by 305
PROTOPLANETARY DISK STRUCTURES IN OPHIUCHUS. II. EXTENSION TO FAINTER SOURCES
Andrews, S., Wilner, D., Hughes, A., Qi, C., & Dullemond, C. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/723/2/1241 · Cited by 300
The formation of Uranus and Neptune in the Jupiter–Saturn region of the Solar System
Thommes, E. W., Duncan, M. J., & Levison, H. F. (1999) · Nature · doi:10.1038/45185 · Cited by 295
Eccentric Extrasolar Planets: The Jumping Jupiter Model
Marzari, F. (2002) · Icarus · doi:10.1006/icar.2001.6786 · Cited by 293
A Three Million Year Integration of the Earth's Orbit
Quinn, T., Tremaine, S., & Duncan, M. (1991) · The Astronomical Journal · doi:10.1086/115850 · Cited by 272
Earth-like worlds on eccentric orbits: excursions beyond the habitable zone
Williams, D. M., & Pollard, D. (2002) · International Journal of Astrobiology · doi:10.1017/s1473550402001064 · Cited by 266
Frequency of Debris Disks around Solar‐Type Stars: First Results from aSpitzerMIPS Survey
Bryden, G., Beichman, C., Trilling, D. E., Rieke, G. H., Holmes, E., Lawler, S., Stapelfeldt, K. R., Werner, M. W., Gautier, T. N., III, Blaylock, M., et al. (2006) · The Astrophysical Journal · doi:10.1086/498093 · Cited by 264
FREQUENCY OF SOLAR-LIKE SYSTEMS AND OF ICE AND GAS GIANTS BEYOND THE SNOW LINE FROM HIGH-MAGNIFICATION MICROLENSING EVENTS IN 2005–2008
Gould, A., Dong, S., Gaudi, B., Udalski, A., Bond, I., Greenhill, J., Street, R., Dominik, M., Sumi, T., Szymański, M., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/720/2/1073 · Cited by 255
Steady State Evolution of Debris Disks around A Stars
Wyatt, M. C., Smith, R., Su, K. Y. L., Rieke, G. H., Greaves, J. S., Beichman, C., & Bryden, G. (2007) · The Astrophysical Journal · doi:10.1086/518404 · Cited by 252
Self-citation
The Structure of the Kuiper Belt: Size Distribution and Radial Extent
Gladman, B., Kavelaars, J. J., Petit, J.-M., Morbidelli, A., Holman, M. J., & Loredo, T. J. (2001) · The Astronomical Journal · doi:10.1086/322080 · Cited by 244
The effects of fly-bys on planetary systems
Malmberg, D., Davies, M. B., & Heggie, D. C. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.17730.x · Cited by 244
Protoplanetary disk structures in Ophiuchus. II. Extension to fainter sourcesPreprint
Andrews, S. M., Wilner, D. J., Hughes, A. M., Qi, C., & Dullemond, C. P. (2010) · Cited by 236
How Observations of Circumstellar Disk Asymmetries Can Reveal Hidden Planets: Pericenter Glow and its Application to the HR 4796 DiskPreprint
Wyatt, M. C., Dermott, S. F., Telesco, C. M., Fisher, R. S., Grogan, K., Holmes, E., & Piña, R. K. (1999) · Cited by 232
Self-citation
The Complete Census of 70 μm–Bright Debris Disks within “The Formation and Evolution of Planetary Systems”SpitzerLegacy Survey of Sun‐like Stars
Hillenbrand, L. A., Carpenter, J. M., Kim, J. S., Meyer, M. R., Backman, D. E., Moro‐Martín, A., Hollenbach, D. J., Hines, D. C., Pascucci, I., & Bouwman, J. (2008) · The Astrophysical Journal · doi:10.1086/529027 · Cited by 230
Self-citation
Variations on Debris Disks: Icy Planet Formation at 30–150 AU for 1–3M⊙Main‐Sequence Stars
Kenyon, S. J., & Bromley, B. C. (2008) · The Astrophysical Journal Supplement Series · doi:10.1086/591794 · Cited by 229
Hill stability and distance curves for the general three-body problem
Marchal, C., & Bozis, G. (1982) · Celestial Mechanics and Dynamical Astronomy · doi:10.1007/bf01230725 · Cited by 229
Debris Disk Evolution Around A Stars
Su, K. Y. L., Rieke, G. H., Stansberry, J. A., Bryden, G., Stapelfeldt, K. R., Trilling, D. E., Muzerolle, J., Beichman, C. A., Moro-Martin, A., Hines, D. C., et al. (2006) · CERN Document Server (European Organization for Nuclear Research) · Cited by 228
Detection of Earth-like planets around nearby stars using a petal-shaped occulter
Cash, W. (2006) · Nature · doi:10.1038/nature04930 · Cited by 226
Nearby Debris Disk Systems with High Fractional Luminosity Reconsidered
Moor, A., Abraham, P., Derekas, A., Kiss, C., Kiss, L. L., Apai, D., Grady, C., & Henning, T. K. (2006) · The Astrophysical Journal · doi:10.1086/503381 · Cited by 224
Age Dependence of the Vega Phenomenon: Theory
Dominik, C., & Decin, G. (2003) · The Astrophysical Journal · doi:10.1086/379169 · Cited by 220
The Primordial Excitation and Clearing of the Asteroid Belt
Petit, J., Morbidelli, A., & Chambers, J. (2001) · Icarus · doi:10.1006/icar.2001.6702 · Cited by 218
EVIDENCE FROM THE ASTEROID BELT FOR A VIOLENT PAST EVOLUTION OF JUPITER'S ORBIT
Morbidelli, A., Brasser, R., Gomes, R. S., Levison, H. F., & Tsiganis, K. (2010) · The Astronomical Journal · doi:10.1088/0004-6256/140/5/1391 · Cited by 216
Five Planets Orbiting 55 Cancri
Fischer, D., Marcy, G., Butler, R. P., Vogt, S., Laughlin, G., Henry, G., Abouav, D., Peek, K. M. G., Wright, J. T., Johnson, J. A., et al. (2007) · The Astrophysical Journal · doi:10.1086/525512 · Cited by 216
Dynamical Instabilities in Extrasolar Planetary Systems Containing Two Giant Planets
Ford, E. B. (2001) · Icarus · doi:10.1006/icar.2001.6588 · Cited by 212
A Decreased Probability of Habitable Planet Formation around Low‐Mass Stars
Raymond, S. N., Scalo, J., & Meadows, V. S. (2007) · The Astrophysical Journal · doi:10.1086/521587 · Cited by 210 · cited 1×
“…between the dust mass and the stellar mass such that the typical protoplanetary disk contains a few percent of the stellar mass (Andrews & Williams 2007a), which has important implications for the planet frequency as a function of stellar mass (Ida & Lin 2005; Raymond et al. 2007; Greaves 2010).”
BackgroundSelf-citation
Final stages of planet formation
Goldreich, P., Lithwick, Y., & Sari, R. (2004) · The Astrophysical Journal · doi:10.1086/423612 · Cited by 207
Dust distributions in debris disks: effects of gravity, radiation pressure and collisions
Krivov, A. V., Löhne, T., & Sremčević, M. (2006) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20064907 · Cited by 204
Formation of Jupiter using opacities based on detailed grain physics
Movshovitz, N., Bodenheimer, P. H., Podolak, M., & Lissauer, J. J. (2010) · Icarus · doi:10.1016/j.icarus.2010.06.009 · Cited by 204
Exotic Earths: Forming Habitable Worlds with Giant Planet Migration
Raymond, S. N., Mandell, A. M., & Sigurðsson, S. (2006) · Science · doi:10.1126/science.1130461 · Cited by 203
Self-citation
The insignificance of P-R drag in detectable extrasolar planetesimal belts
Wyatt, M. C. (2005) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20042073 · Cited by 203
Self-citation
The Formation and Evolution of Planetary Systems: Grain Growth and Chemical Processing of Dust in T Tauri Systems
Bouwman, J., Henning, T. K., Hillenbrand, L. A., Meyer, M. R., Pascucci, I., Carpenter, J. M., Hines, D. C., Kim, J. S., Silverstone, M. D., Hollenbach, D. J., et al. (2008) · The Astrophysical Journal · doi:10.1086/587793 · Cited by 200
Debris disks: seeing dust, thinking of planetesimals and planets
Krivov, A. V. (2010) · Research in Astronomy and Astrophysics · doi:10.1088/1674-4527/10/5/001 · Cited by 198
Incidence 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., Metcalfe, L., Salama, A., Siebenmorgen, R., Trams, N., et al. (2001) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20000075 · Cited by 194
FORMATION AND EVOLUTION OF PLANETARY SYSTEMS: PROPERTIES OF DEBRIS DUST AROUND SOLAR-TYPE STARS
Carpenter, J. M., Bouwman, J., Mamajek, E. E., Meyer, M. R., Hillenbrand, L. A., Backman, D. E., Henning, T. K., Hines, D. C., Hollenbach, D. J., Kim, J. S., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/181/1/197 · Cited by 193
Self-citation
Long‐Term Collisional Evolution of Debris Disks
Lohne, T., Krivov, A. V., & Rodmann, J. (2008) · The Astrophysical Journal · doi:10.1086/524840 · Cited by 185
Formation of Earth‐like Planets During and After Giant Planet Migration
Mandell, A. M., Raymond, S. N., & Sigurðsson, S. (2007) · The Astrophysical Journal · doi:10.1086/512759 · Cited by 182
Self-citation
On the Eccentricity Distribution of Exoplanets from Radial Velocity Surveys
Shen, Y. G., & Turner, E. L. (2008) · The Astrophysical Journal · doi:10.1086/590548 · Cited by 182
THE LAST GASP OF GAS GIANT PLANET FORMATION: ASPITZERSTUDY OF THE 5 Myr OLD CLUSTER NGC 2362
Currie, T., Lada, C. J., Plavchan, P. P., Robitaille, T., Irwin, J. M., & Kenyon, S. J. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/698/1/1 · Cited by 181
The collisional and dynamical evolution of the main-belt and NEA size distributions
O'Brien, D. P., & Greenberg, R. J. (2005) · Icarus · doi:10.1016/j.icarus.2005.04.001 · Cited by 174
A semi-analytic model for oligarchic growth
Chambers, J. (2005) · Icarus · doi:10.1016/j.icarus.2005.10.017 · Cited by 173
On disc driven inward migration of resonantly coupled planets with application to the system around GJ876
Snellgrove, M. D., Papaloizou, J. C. B., & Nelson, R. P. (2001) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20010779 · Cited by 172
ABUNDANT CIRCUMSTELLAR SILICA DUST AND SiO GAS CREATED BY A GIANT HYPERVELOCITY COLLISION IN THE ∼12 MYR HD172555 SYSTEM
Lisse, C. M., Chen, C. H., Wyatt, M. C., Morlok, A., Song, I., Bryden, G., & Sheehan, P. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/701/2/2019 · Cited by 170
Self-citation
Terrestrial Planet Formation. I. The Transition from Oligarchic Growth to Chaotic Growth
Kenyon, S. J., & Bromley, B. C. (2006) · The Astronomical Journal · doi:10.1086/499807 · Cited by 170
A Search for Protoplanetary Disks Around Naked T Tauri Stars
Wolk, S. J., & Walter, F. M. (1996) · The Astronomical Journal · doi:10.1086/117942 · Cited by 168
INVESTIGATING PLANET FORMATION IN CIRCUMSTELLAR DISKS: CARMA OBSERVATIONS OF RY Tau AND DG Tau
Isella, A., Carpenter, J. M., & Sargent, A. I. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/714/2/1746 · Cited by 167
Observable consequences of planet formation models in systems with close-in terrestrial planets
Raymond, S. N., Barnes, R., & Mandell, A. M. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12712.x · Cited by 167
Self-citation
HABITABLE CLIMATES: THE INFLUENCE OF OBLIQUITY
Spiegel, D. S., Menou, K., & Scharf, C. A. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/691/1/596 · Cited by 164
Debris disc stirring by secular perturbations from giant planets
Mustill, A. J., & Wyatt, M. C. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15360.x · Cited by 164
Self-citation
PLANET-PLANET SCATTERING IN PLANETESIMAL DISKS. II. PREDICTIONS FOR OUTER EXTRASOLAR PLANETARY SYSTEMS
Raymond, S. N., Armitage, P. J., & Gorelick, N. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/711/2/772 · Cited by 163
Self-citation
HABITABLE CLIMATES: THE INFLUENCE OF ECCENTRICITY
Dressing, C. D., Spiegel, D. S., Scharf, C. A., Kristen Menou, A., & Raymond, S. N. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/721/2/1295 · Cited by 161
Self-citation
New Debris Disks around Nearby Main-Sequence Stars: Impact on the Direct Detection of Planets
Beichman, C., Bryden, G., Stapelfeldt, K., Gautier, T., Grogan, K., Shao, M., Velusamy, T., Lawler, S., Blaylock, M., Rieke, G., et al. (2006) · The Astrophysical Journal · doi:10.1086/508449 · Cited by 157
Self-citation
Accretion in the Early Kuiper Belt. I. Coagulation and Velocity Evolution
Kenyon, S. J., & Luu, J. X. (1998) · The Astronomical Journal · doi:10.1086/300331 · Cited by 147
Constructing the secular architecture of the solar system II: the terrestrial planets
Brasser, R., Morbidelli, A., Gomes, R. S., Tsiganis, K., & Levison, H. F. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200912878 · Cited by 146
Migration and dynamical relaxation in crowded systems of giant planets
Adams, F. C., & Laughlin, G. (2003) · Icarus · doi:10.1016/s0019-1035(03)00081-2 · Cited by 146
High Orbital Eccentricities of Extrasolar Planets Induced by the Kozai Mechanism
Takeda, G., & Rasio, F. A. (2005) · The Astrophysical Journal · doi:10.1086/430467 · Cited by 145
Gas Disks to Gas Giants: Simulating the Birth of Planetary Systems
Thommes, E. W., Matsumura, S., & Rasio, F. A. (2008) · Science · doi:10.1126/science.1159723 · Cited by 145
PLANETS AND DEBRIS DISKS: RESULTS FROM ASPITZER/MIPS SEARCH FOR INFRARED EXCESS
Bryden, G., Beichman, C., Carpenter, J. M., Rieke, G. H., Stapelfeldt, K. R., Werner, M. W., Tanner, A. M., Lawler, S., Wyatt, M. C., Trilling, D. E., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/705/2/1226 · Cited by 145
Self-citation
Incidence 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
Nearby debris disk systems with high fractional luminosity reconsidered
Moór, A., Ábrahám, P., Apai, D., Derekas, A., Grady, C., Henning, T. K., Kiss, C., & Kiss, L. L. (2006) · CERN Document Server (European Organization for Nuclear Research) · Cited by 144
Circumstellar material in the Vega inner system revealed by CHARA/FLUOR
Absil, O., Folco, E. D., Mérand, A., Augereau, J. ‐., du Foresto, V. C., Aufdenberg, J. P., Kervella, P., Ridgway, S. T., Berger, D. H., ten Brummelaar, T. A., et al. (2006) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20054522 · Cited by 139
Final Stages of Planet Formation
Goldreich, P., Lithwick, Y., & Sari, R. (2004) · CERN Document Server (European Organization for Nuclear Research) · Cited by 137
Evolution of planetary systems in resonance
Kley, W., Peitz, J., & Bryden, G. (2004) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20031589 · Cited by 136
Fragmentation model dependence of collision cascades
Kobayashi, H., & Tanaka, H. (2009) · Icarus · doi:10.1016/j.icarus.2009.10.004 · Cited by 135
From planetesimals to terrestrial planets: N-body simulations including the effects of nebular gas and giant planets
Morishima, R., Stadel, J., & Moore, B. (2009) · Icarus · doi:10.1016/j.icarus.2009.11.038 · Cited by 135
Prospects for Detection of Catastrophic Collisions in Debris Disks
Kenyon, S. J., & Bromley, B. C. (2005) · The Astronomical Journal · doi:10.1086/430461 · Cited by 135
Detecting the Dusty Debris of Terrestrial Planet Formation
Kenyon, S. J., & Bromley, B. C. (2004) · The Astrophysical Journal · doi:10.1086/382693 · Cited by 133
Formation and Evolution of Planetary Systems: Upper Limits to the Gas Mass in Disks around Sun‐like Stars
Pascucci, I., Gorti, U., Hollenbach, D. J., Najita, J., Meyer, M. R., Carpenter, J. M., Hillenbrand, L. A., Herczeg, G. J., Padgett, D. L., Mamajek, E. E., et al. (2006) · The Astrophysical Journal · doi:10.1086/507761 · Cited by 132
Terrestrial Planet Formation. I. The Transition from Oligarchic Growth to Chaotic GrowthPreprint
Kenyon, S. J., & Bromley, B. C. (2006) · Cited by 131
Formation of Terrestrial Planets from Protoplanets. I. Statistics of Basic Dynamical Properties
Kokubo, E., Kominami, J., & Ida, S. (2006) · The Astrophysical Journal · doi:10.1086/501448 · Cited by 128
STELLAR MASS DEPENDENT DISK DISPERSAL
Kennedy, G. M., & Kenyon, S. J. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/695/2/1210 · Cited by 126
Size Distribution of Collisionally Evolved Asteroidal Populations: Analytical Solution for Self-Similar Collision Cascades
Williams, D. R., & Wetherill, G. W. (1994) · Icarus · doi:10.1006/icar.1994.1010 · Cited by 125
Dynamical Shake‐up of Planetary Systems. I. Embryo Trapping and Induced Collisions by the Sweeping Secular Resonance and Embryo‐Disk Tidal Interaction
Nagasawa, M., Lin, D. N. C., & Thommes, E. W. (2005) · The Astrophysical Journal · doi:10.1086/497386 · Cited by 119
Giant planet migration through the action of disk torques and planet–planet scattering
Moorhead, A. V., & Adams, F. C. (2005) · Icarus · doi:10.1016/j.icarus.2005.05.005 · Cited by 117
PLANET-PLANET SCATTERING IN PLANETESIMAL DISKS
Raymond, S. N., Armitage, P. J., & Gorelick, N. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/699/2/l88 · Cited by 116
Self-citation
The history of the Solar system's debris disc: observable properties of the Kuiper belt
Booth, M., Wyatt, M. C., Morbidelli, A., Moro‐Martín, A., & Levison, H. F. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15286.x · Cited by 115
Self-citation
Mean Motion Resonances from Planet-Planet Scattering
Raymond, S. N., Barnes, R., Armitage, P. J., & Gorelick, N. (2008) · The Astrophysical Journal · doi:10.1086/593301 · Cited by 113
Self-citation
Circumstellar material in the Vega inner system revealed by CHARA/FLUORPreprint
Absil, O., Folco, E. D., Mérand, A., Augereau, J. ‐., du Foresto, V. C., Aufdenberg, J. P., Kervella, P., Ridgway, S. T., Berger, D. H., Brummelaar, T. A. T., et al. (2005) · Cited by 111
Debris disc stirring by secular perturbations from giant planetsPreprint
Mustill, A. J., & Wyatt, M. C. (2009) · Cited by 111
Self-citation
Turbulence Implies that Mean Motion Resonances are Rare
Adams, F. C., Laughlin, G., & Bloch, A. M. (2008) · The Astrophysical Journal · doi:10.1086/589986 · Cited by 110
PLANET-PLANET SCATTERING LEADS TO TIGHTLY PACKED PLANETARY SYSTEMS
Raymond, S. N., Barnes, R., Veras, D., Armitage, P. J., Gorelick, N., & Greenberg, R. J. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/696/1/l98 · Cited by 107
Self-citation
Far‐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
Constraining the Lifetime of Circumstellar Disks in the Terrestrial Planet Zone: A Mid‐Infrared Survey of the 30 Myr old Tucana‐Horologium Association
Mamajek, E. E., Meyer, M. R., Hinz, P. M., Hoffmann, W. F., Cohen, M., & Hora, J. L. (2004) · The Astrophysical Journal · doi:10.1086/422550 · Cited by 105
Extraordinary climates of Earth-like planets: three-dimensional climate simulations at extreme obliquity
Williams, D. M., & Pollard, D. (2003) · International Journal of Astrobiology · doi:10.1017/s1473550403001356 · Cited by 105
Evolution of Mid-Infrared Excess around Sun-like Stars: Constraints on Models of Terrestrial Planet Formation
Meyer, M. R., Carpenter, J. M., Mamajek, E. E., Hillenbrand, L. A., Hollenbach, D. J., Moro‐Martín, A., Kim, J. S., Silverstone, M. D., Najita, J., Hines, D. C., et al. (2008) · The Astrophysical Journal · doi:10.1086/527470 · Cited by 105
Self-citation
The Role of Giant Planets in Terrestrial Planet Formation
Levison, H., Dones, L., Agnor, C., Canup, R., & Duncan, M. (2000) · The Astronomical Journal · doi:10.1086/374625 · Cited by 104
The Size–Frequency Distribution of the Zodiacal Cloud: Evidence from the Solar System Dust Bands
Grogan, K. (2001) · Icarus · doi:10.1006/icar.2001.6638 · Cited by 104
Proplyds and Massive Disks in the Orion Nebula Cluster Imaged with CARMA and SMA
Eisner, J. A., Plambeck, R. L., Carpenter, J. M., Corder, S. A., Qi, C., & Wilner, D. J. (2008) · The Astrophysical Journal · doi:10.1086/588524 · Cited by 100
Influence of an inner disc on the orbital evolution of massive planets migrating in resonance
Crida, A., Sándor, Z., & Kley, W. (2008) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20079291 · Cited by 97
Formation of Earth-like Planets During and After Giant Planet Migration
Mandell, A. M., Raymond, S. N., & Sigurdsson, S. (2007) · CERN Document Server (European Organization for Nuclear Research) · Cited by 97
Self-citation
On the formation of terrestrial planets in hot-Jupiter systems
Fogg, M. J., & Nelson, R. P. (2006) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20066171 · Cited by 92
Evolution of Planetary Systems in Resonance
Kley, W., Peitz, J., & Bryden, G. (2003) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361:20031589/pdf · Cited by 92
A NEW HYBRIDN-BODY-COAGULATION CODE FOR THE FORMATION OF GAS GIANT PLANETS
Bromley, B. C., & Kenyon, S. J. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/731/2/101 · Cited by 91
GENERALIZED MILANKOVITCH CYCLES AND LONG-TERM CLIMATIC HABITABILITY
Spiegel, D., Raymond, S., Dressing, C., Scharf, C. A., & Mitchell, J. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/721/2/1308 · Cited by 89
Self-citation
Evolution of a Keplerian disk of colliding and fragmenting particles: a kinetic model with application to the Edgeworth–Kuiper belt
Krivov, A. V., Sremčević, M., & Spahn, F. (2005) · Icarus · doi:10.1016/j.icarus.2004.10.003 · Cited by 87
High Orbital Eccentricities of Extrasolar Planets Induced by the Kozai MechanismPreprint
Takeda, G., & Rasio, F. A. (2005) · Cited by 82
The HARPS search for southern extra-solar planets: XVIII. An Earth-mass planet in the GJ 581 planetary system
Mayor, M., Bonfils, X., Forveille, T., Delfosse, X., Udry, S., Bertaux, J., Beust, H., Bouchy, F., Lovis, C., Pepe, F., et al. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200912172 · Cited by 81
Detecting the Dusty Debris of Terrestrial Planet Formation
Kenyon, S. J., & Bromley, B. C. (2004) · CERN Document Server (European Organization for Nuclear Research) · Cited by 79
VARIATIONS ON DEBRIS DISKS. II. ICY PLANET FORMATION AS A FUNCTION OF THE BULK PROPERTIES AND INITIAL SIZES OF PLANETESIMALS
Kenyon, S. J., & Bromley, B. C. (2010) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/188/1/242 · Cited by 78
Post-main-sequence evolution of A star debris discs
Bonsor, A., & Wyatt, M. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.17412.x · Cited by 75
Self-citation
Nulling interferometry: impact of exozodiacal clouds on the performance of future life-finding space missions
Defrère, D., Absil, O., den Hartog, R., Hanot, C., & Stark, C. C. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200912973 · Cited by 75
The effects of nebula surface density profile and giant‐planet eccentricities on planetary accretion in the inner solar system
Chambers, J., & Cassen, P. (2002) · Meteoritics and Planetary Science · doi:10.1111/j.1945-5100.2002.tb00808.x · Cited by 72
LOCATING PLANETESIMAL BELTS IN THE MULTIPLE-PLANET SYSTEMS HD 128311, HD 202206, HD 82943, AND HR 8799
Moro‐Martín, A., Malhotra, R., Bryden, G., Rieke, G. H., Su, K. Y. L., Beichman, C., & Lawler, S. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/717/2/1123 · Cited by 71
Self-citation
The Stellar Mass-Accretion Rate Relation in T Tauri Stars and Brown Dwarfs
Alexander, R., & Armitage, P. (2006) · The Astrophysical Journal · doi:10.1086/503030 · Cited by 68
Self-citation
ON 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
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
Self-citation
THE LOW LEVEL OF DEBRIS DISK ACTIVITY AT THE TIME OF THE LATE HEAVY BOMBARDMENT: ASPITZERSTUDY OF PRAESEPE
Gáspár, A., Rieke, G. H., Su, K. Y. L., Balog, Z., Trilling, D. E., Muzerolle, J. C., Apai, D., & Kelly, B. C. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/697/2/1578 · Cited by 63
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
Influence of an inner disc on the orbital evolution of massive planets migrating in resonance
Crida, A., Sándor, Z., & Kley, W. (2008) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361:20079291/pdf · Cited by 62
Collisional evolution of eccentric planetesimal swarms
Wyatt, M. C., Booth, M., Payne, M. J., & Churcher, L. J. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15930.x · Cited by 55
Self-citation
DUST 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
The Search for Other Earths: Limits on the Giant Planet Orbits That Allow Habitable Terrestrial Planets to Form
Raymond, S. (2006) · The Astrophysical Journal · doi:10.1086/505596 · Cited by 52
Self-citation
The 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
Predictions for the Correlation between Giant and Terrestrial Extrasolar Planets in Dynamically Evolved Systems
Veras, D., & Armitage, P. J. (2006) · The Astrophysical Journal · doi:10.1086/504582 · Cited by 44
Self-citation
Metallicity, 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
Self-citation
The clearing of discs around late-type T Tauri stars: constraints from the infrared two-colour plane
Ercolano, B., Clarke, C. J., & Hall, A. C. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.17473.x · Cited by 43
Variations on Debris Disks II. Icy Planet Formation as a Function of the Bulk Properties and Initial Sizes of PlanetesimalsPreprint
Kenyon, S. J., & Bromley, B. C. (2016) · Cited by 42
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
Distribution of Circumstellar Disk Masses in the Young Cluster NGC 2024
Eisner, J. A., & Carpenter, J. (2003) · The Astrophysical Journal · doi:10.1086/379102 · Cited by 36
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
Orbital Stability of a Protoplanet System under a Drag Force Proportional to the Random Velocity
Iwasaki, K., Emori, H., Nakazawa, K., & Tanaka, H. (2002) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/54.3.471 · Cited by 34
The Gas-Drag Effect on the Orbital Instability of a Protoplanet System
Iwasaki, K., Tanaka, H., Nakazawa, K., & Emori, H. (2001) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/53.2.321 · Cited by 29
MEAN MOTION RESONANCES IN EXTRASOLAR PLANETARY SYSTEMS WITH TURBULENCE, INTERACTIONS, AND DAMPING
Lecoanet, D., Adams, F. C., & Bloch, A. M. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/692/1/659 · Cited by 19
Forming Close-in Earth-like Planets via a Collision-Merger Mechanism in Late-stage Planet FormationPreprint
Ji, J., Jin, S., & Tinney, C. G. (2016) · Cited by 13
Monthly Notices Letters
(2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.11957.x · Cited by 11
Predicting the incidence of planet and debris discs as a function of stellar mass
Greaves, J. (2010) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1111/j.1745-3933.2010.00943.x · Cited by 6
Detecting Exoplanets in the Presence of Exozodiacal Dust ProfilesPreprint
Noecker, C., & Kuchner, M. J. (2010) · arXiv (Cornell University) · doi:10.48550/arxiv.1012.0977 · Cited by 1
Steady-state evolution of debris disks around solar-type starsPreprint
Kains, N., Wyatt, M. C., & Greaves, J. S. (2011) · arXiv (Cornell University) · doi:10.48550/arxiv.1102.4341 · Cited by 1
Self-citation

Research works printed but not linked: 4

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
Kennedy, 2010, MNRAS, 405, 1253
Laskar, 1993, A&A, 270, 522

Sorted by citations

The Exoplanet Handbook
Perryman, M. A. C. (2011) · Cambridge University Press eBooks · doi:10.1017/9781108304160 · Cited by 380
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
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 195
Self-citation
The empty primordial asteroid belt
Raymond, S. N., & Izidoro, A. (2017) · Science Advances · doi:10.1126/sciadv.1701138 · Cited by 165
Self-citation
The 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
Self-citation

See all 194

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)
ORCID: Raymond, S. N.
Armitage, P. J.
Booth, M.
Wyatt, M. C.
Mandell, A. M.
Selsis, F.
West, A. A.
Venue: Astronomy & Astrophysics
Publisher: EDP Sciences
Published: 2011-05-12
Volume: 530
Pages: A62
ISSN: 0004-6361 (ISSN-L)
1432-0746
DOI: 10.1051/0004-6361/201116456
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 › Earth and Planetary Sciences › Space and Planetary Science › 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 ›

Are you an author, or do you see a problem with this page? Request a review

Debris disks as signposts of terrestrial planet formation

Abstract

Overview

Integrity signals

Verification

Claims the paper makes

Claims other papers make about this one

Self-check

Citations

Cites

Cited by

Related

Metadata

Record

About these checks