Asteroids were born big

Agnor, 1999, On the character and consequences of large impacts in the late stage of terrestrial planet formation, Icarus, 142, 219, 10.1006/icar.1999.6201

Alexander, 2008, The formation conditions of chondrules and chondrites, Science, 320, 1617, 10.1126/science.1156561

Alibert, 2004, Migration and giant planet formation, Astron. Astrophys., 417, L25, 10.1051/0004-6361:20040053

Alibert, 2005, New Jupiter and Saturn formation models meet observations, Astrophys. J., 626, L57, 10.1086/431325

Baruteau, C., 2009. Protoplanetary migration in turbulent isothermal disks. Astrophys. J., submitted for publication.

Benz, 1999, Catastrophic disruptions revisited, Icarus, 142, 5, 10.1006/icar.1999.6204

Bernstein, 2004, The size distribution of trans-neptunian bodies, Astron. J., 128, 1364, 10.1086/422919

Blum, J., and 26 colleagues, 2000. Growth and form of planetary seedlings: Results from a microgravity aggregation experiment. Phys. Rev. Lett. 85, 2426–2429.

Bogard, 1995, Impact ages of meteorites: A synthesis, Meteoritics, 30, 244, 10.1111/j.1945-5100.1995.tb01124.x

Bottke, 1994, Velocity distributions among colliding asteroids, Icarus, 107, 255, 10.1006/icar.1994.1021

Bottke, 2005, The fossilized size distribution of the main asteroid belt, Icarus, 175, 111, 10.1016/j.icarus.2004.10.026

Bottke, 2005, Linking the collisional history of the main asteroid belt to its dynamical excitation and depletion, Icarus, 179, 63, 10.1016/j.icarus.2005.05.017

Britt, 2002, Asteroid density, porosity, and structure, Asteroids, III, 485, 10.2307/j.ctv1v7zdn4.37

Chambers, 2001, Making more terrestrial planets, Icarus, 152, 205, 10.1006/icar.2001.6639

Chambers, 2006, A semi-analytic model for oligarchic growth, Icarus, 180, 496, 10.1016/j.icarus.2005.10.017

Chambers, 1998, Making the terrestrial planets: N-body integrations of planetary embryos in three dimensions, Icarus, 136, 304, 10.1006/icar.1998.6007

Chambers, 2001, Planets in the asteroid belt, Meteorit. Planet. Sci., 36, 381, 10.1111/j.1945-5100.2001.tb01881.x

Ciesla, 2002, The nebular shock wave model for chondrule formation: Shock processing in a particle–gas suspension, Icarus, 158, 281, 10.1006/icar.2002.6895

Colwell, 1999, Low-velocity microgravity impact experiments into simulated regolith, Icarus, 138, 241, 10.1006/icar.1998.6073

Connolly, 1998, The formation of chondrules: Petrologic tests of the shock wave model, Science, 280, 62, 10.1126/science.280.5360.62

Cuzzi, 2006, Particle–gas dynamics and primary accretion, Meteorit. Early Solar Syst., II, 353, 10.2307/j.ctv1v7zdmm.24

Cuzzi, 2001, Size-selective concentration of chondrules and other small particles in protoplanetary nebula turbulence, Astrophys. J., 546, 496, 10.1086/318233

Cuzzi, 2008, Toward planetesimals: Dense chondrule clumps in the protoplanetary nebula, Astrophys. J., 687, 1432, 10.1086/591239

Davis, 1985, Collisional history of asteroids: Evidence from Vesta and the Hirayama families, Icarus, 63, 30, 10.1016/0019-1035(85)90170-8

Davis, 2002, Collisional evolution of small-body populations, Asteroids, III, 545, 10.2307/j.ctv1v7zdn4.41

Desch, 2002, A model of the thermal processing of particles in solar nebula shocks: Application to the cooling rates of chondrules, Meteorit. Planet. Sci., 37, 183, 10.1111/j.1945-5100.2002.tb01104.x

Dominik, 1997, The physics of dust coagulation and the structure of dust aggregates in space, Astrophys. J., 480, 647, 10.1086/303996

Dominik, 2007, Growth of dust as the initial step toward planet formation, Protost. Planets, V, 783

Durda, 1998, Collisional models and scaling laws: A new interpretation of the shape of the main-belt asteroid size distribution, Icarus, 135, 431, 10.1006/icar.1998.5960

Durda, 2004, The formation of asteroid satellites in large impacts: Results from numerical simulations, Icarus, 170, 243, 10.1016/j.icarus.2004.04.003

Durisen, 2005, A hybrid scenario for gas giant planet formation in rings, Icarus, 173, 417, 10.1016/j.icarus.2004.08.003

Goldreich, 2004, Final stages of planet formation, Astrophys. J., 614, 497, 10.1086/423612

Gomes, 2005, Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets, Nature, 435, 466, 10.1038/nature03676

Greenberg, 1978, Planetesimals to planets – Numerical simulation of collisional evolution, Icarus, 35, 1, 10.1016/0019-1035(78)90057-X

Greenzweig, 1992, Accretion rates of protoplanets. II – Gaussian distributions of planetesimal velocities, Icarus, 100, 440, 10.1016/0019-1035(92)90110-S

Grieve, R.A., Shoemaker, E.M., 1994. The record of past impacts on Earth. In: Hazards Due to Comets and Asteroids, pp. 417–462.

Haisch, 2001, Disk frequencies and lifetimes in young clusters, Astrophys. J., 553, L153, 10.1086/320685

Hayashi, 1981, Structure of the solar nebula, growth and decay of magnetic fields and effects of magnetic and turbulent viscosities on the nebula, Progr. Theor. Phys., 70, 35, 10.1143/PTPS.70.35

Ida, 2004, Toward a deterministic model of planetary formation. I. A desert in the mass and semimajor axis distributions of extrasolar planets, Astrophys. J., 604, 388, 10.1086/381724

Ida, 2004, Toward a deterministic model of planetary formation. II. The formation and retention of gas giant planets around stars with a range of metallicities, Astrophys. J., 616, 567, 10.1086/424830

Ida, 1993, Scattering of planetesimals by a protoplanet – Slowing down of runaway growth, Icarus, 106, 210, 10.1006/icar.1993.1167

Ida, 2008, Accretion and destruction of planetesimals in turbulent disks, Astrophys. J., 686, 1292, 10.1086/591903

Jedicke, 2002, Observational selection effects in asteroid surveys, Asteroids, III, 71, 10.2307/j.ctv1v7zdn4.12

Johansen, 2006, Dust sedimentation and self-sustained Kelvin–Helmholtz turbulence in protoplanetary disk midplanes, Astrophys. J., 643, 1219, 10.1086/502968

Johansen, 2007, Rapid planetesimal formation in turbulent circumstellar disks, Nature, 448, 1022, 10.1038/nature06086

Kempf, 1999, N-particle-simulations of dust growth. I. Growth driven by Brownian motion, Icarus, 141, 388, 10.1006/icar.1999.6171

Kenyon, 2001, Gravitational stirring in planetary debris disks, Astron. J., 121, 538, 10.1086/318019

Kenyon, 2004, The size distribution of Kuiper belt objects, Astron. J., 128, 1916, 10.1086/423697

Kenyon, 2006, Terrestrial planet formation. I. The transition from oligarchic growth to chaotic growth, Astron. J., 131, 1837, 10.1086/499807

Kenyon, 1999, Accretion in the early outer Solar System, Astrophys. J., 526, 465, 10.1086/308000

Kokubo, 1998, Oligarchic growth of protoplanets, Icarus, 131, 171, 10.1006/icar.1997.5840

Kokubo, 2000, Formation of protoplanets from planetesimals in the solar nebula, Icarus, 143, 15, 10.1006/icar.1999.6237

Krasinsky, 2002, Hidden mass in the asteroid belt, Icarus, 158, 98, 10.1006/icar.2002.6837

Kring, 2008, Impact cratering on the H-chondrite parent body: Implications for the collisional evolution of the inner Solar System, Lunar Planet. Inst. Conf., 39, 1305

Kuiper, 1958, Proceedings of the celestial mechanics conference: Statistics of asteroids, Astron. J., 63, 412, 10.1086/107794

Laughlin, 2004, Type I planetary migration with MHD turbulence, Astrophys. J., 608, 489, 10.1086/386316

Leinhardt, 2009, Full numerical simulations of catastrophic small body collisions, Icarus, 199, 542, 10.1016/j.icarus.2008.09.013

Mann, 1996, The contribution of asteroid dust to the interplanetary dust cloud: The impact of ULYSSES results on the understanding of dust production in the asteroid belt and of the formation of the IRAS dust bands, Icarus, 120, 399, 10.1006/icar.1996.0059

Merline, 2002, Asteroids do have satellites, Asteroids, III, 289, 10.2307/j.ctv1v7zdn4.26

Minton, 2009, A record of planet migration in the main asteroid belt, Nature, 457, 1109, 10.1038/nature07778

Morbidelli, 2000, Source regions and timescales for the delivery of water to Earth, Meteorit. Planet. Sci., 35, 1309, 10.1111/j.1945-5100.2000.tb01518.x

Nelson, 2005, On the orbital evolution of low mass protoplanets in turbulent, magnetised disks, Astron. Astrophys., 443, 1067, 10.1051/0004-6361:20042605

O’Brien, 2005, The collisional and dynamical evolution of the main-belt and NEA size distributions, Icarus, 178, 179, 10.1016/j.icarus.2005.04.001

O’Brien, 2006, Terrestrial planet formation with strong dynamical friction, Icarus, 184, 39, 10.1016/j.icarus.2006.04.005

O’Brien, 2007, The primordial excitation and clearing of the asteroid belt revisited, Icarus, 191, 434, 10.1016/j.icarus.2007.05.005

Pan, 2005, Shaping the Kuiper belt size distribution by shattering large but strengthless bodies, Icarus, 173, 342, 10.1016/j.icarus.2004.09.004

Papaloizou, 2003, The interaction of a giant planet with a disc with MHD turbulence – I. The initial turbulent disc models, Mon. Not. Roy. Astron. Soc., 339, 983, 10.1046/j.1365-8711.2003.06246.x

Petit, 2001, The primordial excitation and clearing of the asteroid belt, Icarus, 153, 338, 10.1006/icar.2001.6702

Petit, 2002, Primordial excitation and depletion of the main belt, Asteroids, III, 711, 10.2307/j.ctv1v7zdn4.54

Podolak, 2004, A note on the snow line in protostellar accretion disks, Meteorit. Planet. Sci., 39, 1859, 10.1111/j.1945-5100.2004.tb00081.x

Pollack, 1996, Formation of the giant planets by concurrent accretion of solids and gas, Icarus, 124, 62, 10.1006/icar.1996.0190

Raymond, 2004, Making other earths: Dynamical simulations of terrestrial planet formation and water delivery, Icarus, 168, 1, 10.1016/j.icarus.2003.11.019

Raymond, 2005, Terrestrial planet formation in disks with varying surface density profiles, Astrophys. J., 632, 670, 10.1086/433179

Raymond, 2006, High-resolution simulations of the final assembly of Earth-like planets I. Terrestrial accretion and dynamics, Icarus, 183, 265, 10.1016/j.icarus.2006.03.011

Raymond, 2007, High-resolution simulations of the final assembly of Earth-like planets. 2. Water delivery and planetary habitability, Astrobiology, 7, 66, 10.1089/ast.2006.06-0126

Rice, 2004, Accelerated planetesimal growth in self-gravitating protoplanetary discs, Mon. Not. R. Astron. Soc., 355, 543, 10.1111/j.1365-2966.2004.08339.x

Scott, 2006, Meteoritical and dynamical constraints on the growth mechanisms and formation times of asteroids and Jupiter, Icarus, 185, 72, 10.1016/j.icarus.2006.06.012

Shakura, 1973, Black holes in binary systems. Observational appearance, Astron. Astrophys., 24, 337

Silverstone, M.D., and 16 colleagues, 2006. Formation and Evolution of Planetary Systems (FEPS): Primordial warm dust evolution from 3 to 30Myr around Sun-like stars. Astrophys. J. 639, 1138–1146.

Stewart, 2009, Velocity-dependent catastrophic disruption criteria for planetesimals, Astrophys. J., 691, L133, 10.1088/0004-637X/691/2/L133

Stone, 2000, Transport processes in protostellar disks, Protost. Planets, IV, 589

Strom, 2005, The origin of planetary impactors in the inner Solar System, Science, 309, 1847, 10.1126/science.1113544

Thomas, 1997, Impact excavation on Asteroid 4 Vesta: Hubble space telescope results, Science, 277, 1492, 10.1126/science.277.5331.1492

Thommes, 2003, Oligarchic growth of giant planets, Icarus, 161, 431, 10.1016/S0019-1035(02)00043-X

Weidenschilling, 1977, The distribution of mass in the planetary system and solar nebula, Astrophys. Space Sci., 51, 153, 10.1007/BF00642464

Weidenschilling, 1980, Dust to planetesimals – Settling and coagulation in the solar nebula, Icarus, 44, 172, 10.1016/0019-1035(80)90064-0

Weidenschilling, 2009, How big were the first planetesimals? Does size matter?, Lunar Planet. Inst. Sci. Conf., 40, 1760

Weidenschilling, 1997, Accretional evolution of a planetesimal swarm, Icarus, 128, 429, 10.1006/icar.1997.5747

Wetherill, 1989, Origin of the asteroid belt, Asteroids, II, 661

Wetherill, 1992, An alternative model for the formation of the asteroids, Icarus, 100, 307, 10.1016/0019-1035(92)90103-E

Wetherill, 1989, Accumulation of a swarm of small planetesimals, Icarus, 77, 330, 10.1016/0019-1035(89)90093-6

Wetherill, 1993, Formation of planetary embryos – Effects of fragmentation, low relative velocity, and independent variation of eccentricity and inclination, Icarus, 106, 190, 10.1006/icar.1993.1166

Wurm, 1998, Experiments on preplanetary dust aggregation, Icarus, 132, 125, 10.1006/icar.1998.5891

Wurm, 2000, An experimental study on the structure of cosmic dust aggregates and their alignment by motion relative to gas, Astrophys. J., 529, L57, 10.1086/312447

Wurm, 2005, Growth of planetesimals by impacts at ∼25m/s, Icarus, 178, 253, 10.1016/j.icarus.2005.04.002

Youdin, 2005, Streaming instabilities in protoplanetary disks, Astrophys. J., 620, 459, 10.1086/426895