Abstract
Models of the origins of gas giant planets and ‘ice’ giant planets are discussed and related to formation theories of both smaller objects (terrestrial planets) and larger bodies (stars). The most detailed models of planetary formation are based upon observations of our own Solar System, of young stars and their environments, and of extrasolar planets. Stars form from the collapse, and sometimes fragmentation, of molecular cloud cores. Terrestrial planets are formed within disks around young stars via the accumulation of small dust grains into larger and larger bodies until the planetary orbits become well enough separated that the configuration is stable for the lifetime of the system. Uranus and Neptune almost certainly formed via a bottom-up (terrestrial planet-like) mechanism; such a mechanism is also the most likely origin scenario for Saturn and Jupiter.
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References
Adams, F.C. and Benz, W.: 1992, ‘Gravitational instabilties in circumstellar disks and the formation of binary companions’, in H.A. McAlister and W.I. Hartkopf (eds.), Complementary approaches to double and multiple star research, ASP Conf. Ser. 32, IAU Colloquium 135, pp. 185–194.
Alencar, S.H.P. and Batalha, C.: 2002, ‘Variability of Southern T Tauri Stars. II. The Spectral Variability of the Classical T Tauri Star TW Hydrae’, Astrophys. J. 571, 378–393.
André, P., Ward-Thompson, D., and Barsony, M.: 2000, ‘From Prestellar Cores to Protostars: the Initial Conditions of Star Formation’, in V. Mannings, A. P. Boss, and S. Russells (eds.), Protostars and Planets IV, Univ. Arizona Press, Tucson, pp. 59–96.
Bate, M.R., Lubow, S.H., Ogilvie, G.I., and Miller, K.A.: 2003, ‘Three-dimensional calculations of high- and low-mass planets embedded in protoplanetary discs’, Mon. Not. Roy. Astron. Soc. 341, 213–229.
Bodenheimer, P., Burkert, A., Klein, R.I., Boss, A.P.: 2000a, ‘Multiple Fragmentation of Protostars’, in V.Mannings, A.P. Boss, and S. Russells (eds.), Protostars and Planets IV, Univ. Arizona Press, Tucson, pp. 675–701.
Bodenheimer, P., Hubickyj, O., and Lissauer, J.J.: 2000b, ‘Models of the in Situ Formation of Detected Extrasolar Giant Planets’, Icarus 143, 2–14.
Boss, A.P.: 1998, ‘Evolution of the solar nebula. IV. Giant gaseous protoplanet formation’, Astrophys. J. 503, 923–937.
Boss, A.P.: 2000, ‘Possible rapid gas giant planet formation in the solar nebula and other protoplanetary disks’, Astrophys. J. 536, L101–L104.
Boss, A.P.: 2001, ‘Gas Giant Protoplanet Formation: Disk Instability Models with Thermodynamics and Radiative Transfer’, Astrophys. J. 563, 367–373.
Burrows, A., Sudarsky, D., Hubbard, W.B.: 2003, ‘A Theory for the Radius of the Transiting Giant Planet HD 209458b’, Astrophys. J. 594, 545–551.
Cassen, P., Shu, F.H., and Terebey, S.: 1985, ‘Protostellar disks and star formation’, in D.C. Black and M.S. Matthews (eds.), Protostars and Planets II, Univ. Arizona Press, Tucson, pp. 448–483.
Chambers, J.E.: 2001, ‘Making More Terrestrial Planets’, Icarus 152, 205–224.
Chambers, J.E., Quintana, E.V., Duncan, M.J., and Lissauer, J.J.: 2002, ‘Symplectic Integrator Algorithms for Modeling Planetary Accretion in Binary Star Systems’, Astron. J. 123, 2884–2894.
Charbonneau, D., Brown, T.M., Latham, D.W., and Mayor, M.: 2000, Astrophys. J. 529, L45–L48.
Chen, C.H. and Kamp, I.: 2004, ‘Are giant planets forming around HR 4796A?’, Astrophys. J. 602, 985–992.
Chiang, E. and Goldreich, P.: 1997, ‘Spectral Energy Distributions of T Tauri Stars with Passive Circumstellar Disks’, Astrophys. J. 490, 368–376.
D’Angelo, G., Henning, T., and Kley, W.: 2002, ‘Nested-grid calculations of disk-planet interaction’, Astron. Astrophys. 385, 647–670.
D’Angelo, G., Kley, W., and Henning, T.: 2003, ‘Orbital Migration and Mass Accretion of Protoplanets in Three-dimensional Global Computations with Nested Grids’ Astrophys. J. 586, 540–561.
Fischer, D.A. and Valenti, J.A.: 2003, ‘Metallicities of stars with extrasolar planets’, in D. Deming and S. Seager (eds.), Scientific Frontiers in Research on Extrasolar Planets, ASP Conference Series 294, ASP, San Francisco, ISBN: 1-58381-141-9, pp. 117–128.
Ford, E.B., Havlickova, M., and Rasio, F.A.: 2001, ‘Dynamical instabilities in extrasolar planetary systems containing two giant planets’, Icarus 150, 303–313.
Gilliland, R.L., et al.: 2000, ‘A lack of planets in 47 Tucanae from a Hubble Space Telescope search’, Astrophys. J. 545, L47–L51.
Goldreich, P., Lithwick, Y., and Sari, R.: 2004, ‘Planet Formation by Coagulation: A Focus on Uranus and Neptune’, Ann. Rev. Astron. Astrophys. 42, in press.
Goldreich, P. and Tremaine, S.: 1980, ‘Disk-satellite interactions’, Astrophys. J. 241, 425–441.
Goldreich, P. and Ward, W.R.: 1973, ‘The Formation of Planetesimals’, Astrophys. J. 183, 1051–1062.
Goodman, A.A., Benson, P.J., Fuller, G.A., and Myers, P.C.: 1993, ‘Dense cores in dark clouds. VIII - Velocity gradients’, Astrophys. J. 406, 528–547.
Goodman, J. and Pindor, B.: 2000, ‘Secular instability and planetesimal formation in the dust layer’, Icarus 148, 537–549.
Haisch, K.E., Jr., Lada, E.A., and Lada, C.J.: 2001, ‘Disk frequencies and lifetimes in young clusters’, Astrophys. J. 553, L153–L156.
Inaba, S., Wetherill, G.W., and Ikoma, M.: 2003, ‘Formation of gas giant planets: core accretion models with fragmentation and planetary envelope’, Icarus 166, 46–62.
Hewins, R., Jones, R., and Scott, E. (eds.): 1996, Chondrules and the Protoplanetary Disk, Cambridge Univ. Press.
Hollenbach, D., Yorke, H.W., and Johnstone, D.: 2000, ‘Disk dispersal around young stars’, in V. Mannings, A.P. Boss, and S. Russell (eds.), Protostars and Planets IV, Univ. Arizona Press, Tucson, pp. 401–428.
Holman, M.J., Touma, J., and Tremaine, S.: 1997, ‘Chaotic variations in the eccentricity of the planet orbiting 16 CYG B.’, Nature 386, 254–256.
Hubbard, W.B., Podolak, M., and Stevenson, D.J.: 1995, ‘The interior of Neptune’, in D.P. Cruikshank (ed.), Neptune and Triton, Univ. Arizona Press, Tucson, pp. 109–138.
Hubickyj, O., Bodenheimer, P., and Lissauer, J.J.: 2005, in preparation.
Lada, E.A., Strom, K.M., and Myers, P.C.: 1993, ‘Environments of star formation – Relationship between molecular clouds, dense cores and young stars’, in E.H. Levy and J.I. Lunine (ed.), Protostars and Planets III, Univ. Arizona Press, Tucson, pp. 245–277.
Lada, E.A.: 2003, ‘Evolution of circumstellar disks in young stellar clusters’, Am. Astron. Soc. Meeting 202, abstract # 24.06.
Laskar, J.: 2000, ‘On the spacing of planetary systems’, Phys. Rev. Lett. 84, 3240–3243.
Laughlin, G., and Bodenheimer, P.: 1994, ‘Nonaxisymmetric evolution in protostellar disks’, Astrophys. J. 436, 335–354.
Laughlin, G. and Adams, F.C.: 1998, ‘The modification of planetary orbits in dense open clusters’, Astrophys. J. 508, L171–L174.
Levison, H.F., Lissauer, J.J., and Duncan, M.J.: 1998, ‘Modeling the diversity of outer planetary systems’, Astron. J. 116, 1998–2014.
Lin, D.N.C., Bodenheimer, P., and Richardson, D.C.: 1996, ‘Orbital migration of the planetary companion of 51 Pegasi to its present location’, Nature 380, 606–607.
Lin, D.N.C. and Papaloizou, J.C.B.: 1979, ‘Tidal torques on accretion discs in binary systems with extreme mass ratios’, Mon. Not. Royal Astron. Soc. 186, 799–812.
Lin, D.N.C., Papaloizou, J.C.B., Terquem, C., Bryden, G., and Ida, S.: 2000, ‘Orbital evolution and planet-star tidal interaction’, in V. Mannings, A. P. Boss, and S. Russell (eds.), Protostars and Planets IV, Univ. Arizona Press, Tucosn, pp. 1111–1134.
Lissauer, J.J.: 1987, ‘Timescales for planetary accretion and the structure of the protoplanetary disk’, Icarus 69, 249–265.
Lissauer, J.J.: 1993, ‘Planet formation’, Ann. Rev. Astron. Astrophys. 31, 129–174.
Lissauer, J.J.: 1995, ‘Urey prize lecture: On the diversity of plausible planetary systems’, Icarus 114, 217–236.
Lissauer, J.J.: 2004, ‘Formation of giant planets and brown dwarfs’, in J.-P. Beaulieu, A. Lecavelier des Etangs, and C. Terquem (eds.), Extrasolar Planets, Today and Tomorrow, ASP Conf. Ser. 3xx, Astron. Soc. of the Pacific, San Francisco, in press.
Lissauer, J.J., Pollack, J.B., Wetherill, G.W., and Stevenson, D.J.: 1995, ‘Formation of the Neptune System’, in D. Cruikshank (ed.), Neptune and Triton, Univ. Arizona Press, Tucson, pp. 37–108.
Livio, M. and Pringle, J.E.: 2003, ‘Metallicity, planetary formation and migration’, Mon. Not. Roy. Astron. Soc. 346, L42–L44.
Mac Low, M. and Klessen, R.S.: 2004, ‘Control of star formation by supersonic turbulence’, Rev. Modern Phys. 76, 125–194.
Marcy, G.W., Butler, R.P., Fischer, D.A., and Vogt, S.S.: 2004, in J.-P. Beaulieu, A. Lecavelier des Etangs, and C. Terquem (eds.), Extrasolar Planets, Today and Tomorrow, ASP Conf. Ser. 3xx, Astron. Soc. of the Pacific, San Francisco, in press.
Masset, F.S., and Papaloizou, J.C.B.: 2003, ‘Runaway migration and the formation of hot Jupiters’, Astrophys. J. 588, 494–508.
Mayer, L., Quinn, T., Wadsley, J., and Stadel, J.: 2002, ‘Formation of giant planets by fragmentation of protoplanetary disks’, Science 298, 1756–1759.
Mayor, M., et al.: 2004, in J.-P. Beaulieu, A. Lecavelier des Etangs, and C. Terquem (eds.), Extrasolar Planets, Today and Tomorrow, ASP Conf. Ser. 3xx, Astron. Soc. of the Pacific, San Francisco, in press.
McCaughrean, M.J., Stepelfeldt, K.R., and Close, L.M.: 2000, ‘High-resolution optical and nearinfrared imaging of young circumstellar disks’, in V. Mannings, A.P. Boss, and S. Russell (eds.), Protostars and Planets IV, Univ. Arizona Press, Tucson, pp. 485–507.
Metchev, S.A., Hillenbrand, L.A., and Meyer, M.R.: 2004, ‘Ten micron observations of nearby young stars’, Astrophys. J. 600, 435–450.
Nakano, T.: 1987, ‘Formation of planets around stars of various masses. I – Formulationand a star of one solar mass’, Mon. Not. Roy. Astron. Soc. 224, 107–130.
Podolak, M.: 2003, ‘The contribution of small grains to the opacity of protoplanetary atmospheres’, Icarus 165, 428–437.
Pollack, J.B., Hubickyj, O., Bodenheimer, P., Lissauer, J.J., Podolak, M., and Greenzweig, Y.: 1996, ‘Formation of the giant planets by concurrent accretion of solids and gas’, Icarus 124, 62–85.
Rasio, F.A. and Ford, E.B.: 1996, ‘Dynamical instabilities and the formation of extrasolar planetary systems’, Science 274, 954–956.
Safronov, V.S.: 1969, Evolution of the protoplanetary cloud and formation of the Earth and planets, in Russian, Nauka Press, Moscow, 1972 English translation: NASA TTF-677.
Santos, N.C., Israelian, G., Mayor, M., Rebolo, R., and Udry, S.: 2003, ‘Statistical properties of exoplanets. II.Metallicity, orbital parameters, and space velocities’, Astron. Astrophys. 398, 363–376.
Showalter, M.R.: 1991, ‘Visual detection of 1981S13, Saturn’s eighteenth satellite, and its role in the Encke gap’, Nature 351, 709–713.
Sigurdsson, S.: 1993, ‘Genesis of a planet in Messier 4’, Astrophys. J. 415, L43–L46.
Sigurdsson, S, Richer, H.B., Hansen, B.M., Stairs, I.H., and Thorsett, S.E.: 2003, ‘A young white dwarf companion to pulsar B1620-26: Evidence for early planet formation’, Science 301, 193–196.
Strom, S.E., Edwards, S., and Skrutskie, M.F.: 1993, ‘Evolutionary time scales for circumstellar disks associated with intermediate- and solar-type stars’, in E.H. Levy, and J.I. Lunine (eds.), Protostars and Planets III, Univ. Arizona Press, Tucson, pp. 837–866.
Thommes, E.W. and Lissauer, J.J.: 2003, in Proc. Astrophysics of Life Conf., Cambridge Univ. Press, in press.
Thommes, E.W., Duncan, M.J., and Levison, H.F.: 2003, ‘Oligarchic growth of giant planets’, Icarus 161, 431–455.
Ward, W.R.: 1986, ‘Density waves in the solar nebula – differential Lindblad torque’, Icarus 67, 164–180.
Ward, W.R.: 2000, ‘On planetesimal formation: the role of collective particle behavior’, in R.M. Canup, and K. Righter (eds.), Origin of the Earth and Moon, Univ. Arizona Press, Tucson, pp. 75–84.
Ward, W.R. and Hahn, J.M.: 2000, ‘Disk-planet interactions and the formation of planetary systems’, in V. Mannings, A.P. Boss, and S. Russell (eds.), Protostars and Planets IV, Univ. Arizona Press, Tucson, pp. 1135–1155.
Weidenschilling, S.J. and Cuzzi, J.N.: 1993, ‘Formation of planetesimals in the solar nebula’, in E.H. Levy and J.I. Lunine (eds.), Protostars and Planets III, Univ. Arizona Press, Tucson, pp. 1031–1060.
Weidenschilling, S.J. and Marzari, F.: 1996, ‘Gravitational scattering as a possible origin for giant planets at small stellar distances’, Nature 384, 619–621.
Weidenschilling, S.J., Marzari, F., Davis, D.R.: 2004, ‘Accretion of the Outer Planets: Oligarchy or Monarchy?’, Lunar and Planetary Institute Conference Abstracts 35, 1174.
Wetherill, G.W.: 1990, ‘Formation of the Earth’, Ann. Rev. Earth Plan. Sci. 18, 205–256.
Wuchterl, G. and Tscharnuter, W.M.: 2003, ‘From clouds to stars. Protostellar collapse and the evolution to the pre-main sequence I. Equations and evolution in the Hertzsprung-Russell diagram’, Astron. Astrophys. 398, 1081–1090.
Wuchterl, G., Guillot, T., and Lissauer, J.J.: 2000, ‘Giant planet formation’, in V. Mannings, A. P. Boss, and S. Russell (eds.), Protostars and Planets IV, Univ. Arizona Press, Tucson, pp. 1081–1109.
Youdin, A.N. and Shu, F.H.: 2002, ‘Planetesimal formation by gravitational instability’, Astrophys. J. 580, 494–505.
Young, R.E.: 2003, ‘The Galileo probe: how it has changed our understanding of Jupiter’, New Astron. Rev. 47, 1–51.
Zapatero Osorio, M.R., Béjar, V.J.S., Martín, E.L., Rebolo, R., Barrado y Navascués, D., Bailer- Jones, C.A.L., and Mundt, R.: 2000, ‘Discovery of young, isolated planetary mass objects in the C9-Orionis star cluster’, Science 290, 103–107.
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Lissauer, J.J. Formation of the Outer Planets. Space Sci Rev 116, 11–24 (2005). https://doi.org/10.1007/s11214-005-1945-3
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DOI: https://doi.org/10.1007/s11214-005-1945-3