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The Accumulation and Structure of Comets

Published online by Cambridge University Press:  12 April 2016

Bertram Donn*
Affiliation:
Laboratory for Extraterrestrial Physics NASA/Goddard Space Flight Center

Abstract

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The evidence for the accumulation of the terrestrial planets and comets from solid grains is reviewed briefly. The various proposals for formation of cometary nuclei are described and commented upon. With three exceptions, all hypotheses conclude or imply that a single compact object forms. It has been almost universally assumed that grain accretion produced compact aggregates as is the case with liquid drops, and that this process continued. Several hypotheses start with Goldreich-Ward-type gravitational instabilities. The collapse for this case also occurs at low velocities in the cm·s−1 to m·s−1 range. Experiment and theory show that under these conditions, low-density, filamentary clusters form that are fractal aggregates with a fractal dimension approximately equal to two. Agglomeration of these clusters produces larger, compressible planetesimals or cometesimals, which efficiently combine upon colliding. In order to form cometary nuclei, the initial temperature must be about 50 K and not undergo a significant temperature rise during the accumulation process. The collision process can be analyzed with some simplifying assumptions using the limited experimental data available for the compaction of low-density powders. The calculations show that accumulation will occur at low temperatures. For a more refined analysis, experiments to study impacts on low-density powders are required. Models of cometary nuclei are reviewed, and a simple model of the structure that results from the accumulation of fluffy aggregates is described.

Type
Section III: Comets, Origins, and Evolution
Copyright
Copyright © Kluwer 1991

References

Abergel, A., Bertaux, J.L., and Dimarellis, E. (1987). ‘Image Processing on Vega Pictures,’ in Symposium on the Diversity and Similarity of Comets, ESA SP-278,Paris, France, pp. 689694.Google Scholar
A’Hearn, M.F., and Millis, R.L. (1980). ‘Abundance Correlations Among Comets,’ Astron. J. 85, 15281537.CrossRefGoogle Scholar
A’Hearn, M.F., Millis, R.L., and Birch, P.V. (1979). ‘Gas and Dust in Some Recent Comets,’ Astron. J. 84, 570579.CrossRefGoogle Scholar
Alfven, M., and Arrhenius, G. (1970). ‘Accretion of Celestial Bodies,’ Astrophys. Space Sci. 9, 333.Google Scholar
Anders, E. (1965). ‘Fragmentation History of Asteroids,’ Icarus 4, 399408.CrossRefGoogle Scholar
Bailey, M.E. (1987). ‘The Formation of Comets in Wind-Driven Shells Around Protostars,’ Icarus 69, 270282.CrossRefGoogle Scholar
Bailey, M.E., Clube, S.V.M., and Napier, W.M. (1986). ‘The Origin of Comets,’ Vistas in Astron. 29, 53112.CrossRefGoogle Scholar
Bailey, M.E., Clube, S.V.M., and Napier, W.M. (1990). Origin of Comets, Pergamon Press, New York.Google Scholar
Biermann, L., and Michel, K.W. (1978). ‘On the Origin of Cometary Nuclei in the Presolar Nebula,’ Moon and Planets 18, 447.Google Scholar
Bourdon, E.B., Prince, R.H., and Duley, W.W. (1982). ‘An Experimental Determination of the Cross Section for Photodesorption,’ Astrophys. J. 260, 909913.CrossRefGoogle Scholar
Brown, H. (1952). ‘Rare Gases and the Formation of the Earth’s Atmosphere,’ in The Atmospheres of the Earth and Planets, Kuiper, G.P. (ed.), University of Chicago Press, Chicago, pp. 260268.Google Scholar
Brownlee, D.E., Pilachowski, L., Olszewski, E., and Hodge, P.W. (1980). ‘Analysis of Interplanetary Dust Collections’ in Solid Particles in the Solar System, Halliday, I. and McIntosh, B.A. (eds.), D. Reidel Publishing Company, Boston, pp. 333342.CrossRefGoogle Scholar
Cameron, A.G.W. (1973). ‘Accumulation Processes in the Primitive Solar Nebula,’ Icarus 18, 407450.CrossRefGoogle Scholar
Cameron, A.G.W. (1975). ‘Clumping of Interstellar Grains During Formation of the Primitive Solar Nebula,’ Icarus 24, 128133.CrossRefGoogle Scholar
Clube, S.V.M., and Napier, W.M. (1985). ‘Comet Formation in Molecular Clouds,’ Icarus 62, 384388.CrossRefGoogle Scholar
Daniels, P.A., and Hughes, D.W. (1981). ‘The Accretion of Cosmic Dust—A Computer Simulation,’ Mon. Not. Roy. Astron Soc. 195, 10011009.CrossRefGoogle Scholar
Dexter, A.R., and Tanner, D.W. (1971). ‘Packing Density of Ternary Mixtures of Spheres,’ Nature Physical Science 230, 177179.CrossRefGoogle Scholar
Donn, B. (1963). ‘The Origin and Structure of Icy Cometary Nuclei,’ Icarus 2, 396402.CrossRefGoogle Scholar
Donn, B. (1977). ‘A Comparison of the Composition of New and Evolved Comets’ in Comets, Asteroids, Meteorites Delsemme, A.H. (ed.), University of Toledo Press, Toledo, pp. 1523.Google Scholar
Donn, B. (1981). ‘Comet Nucleus: Some Characteristics and a Hypothesis on Origin and Structure,’ in Comets and the Origin of Life, Ponnomperoma, C. (ed.), D. Reidel Publishing Company, Dordrecht, Holland, 2129.CrossRefGoogle Scholar
Donn, B. (1989). ‘The Formation and Structure of Fluffy Cometary Nuclei From Random Accumulation of Grains’ submitted to Astron. Astrophys.Google Scholar
Donn, B., and Meakin, P.(1989). ‘Collisions of Macroscopic Fluffy Aggregates in the Primordial Solar Nebular and the Formation of the Planetesimals,’ Proc. 19th Lunar and Planetary Science Conf., Houston, 577580.Google Scholar
Donn, B., and Rahe, J. (1982). ‘Structure and Origin of Cometary Nuclei,’ in Comets, Wilkening, L. (ed.), University of Arizona Press, Tucson, pp. 203266.CrossRefGoogle ScholarPubMed
Donn, B., and Sears, G.W. (1963). ‘Planets and Comets, the Role of Crystal Growth in their Formation,’ Science 140, 12081211.CrossRefGoogle ScholarPubMed
Donn, B., Daniels, P.A., and Hughes, D.W. (1985). ‘On the Structure of the Cometary Nucleus’ (Abstract), Bull. Am. Astron. Soc. 17, 520 Google Scholar
Fesenkov, V.G. (1963). ‘On the Nature and Origin of Comets,’ Sov. Astron. A. J. 459464.Google Scholar
Forrest, S.R., and Witten, T.A. (1979). ‘Long-Range Correlations in Smoke Particle Aggregates,’ J. Phys. A Math. Gen. 18, 21092117.Google Scholar
Fuchs, N.A. (1964). The Mechanics of Aerosols, McMillan, New York.Google Scholar
Geiss, J. (1987). ‘Composition Measurements and the History of Cometary Matter,’ Astron. Astrophys. 187, 859866.Google Scholar
Goldreich, P., and Ward, W.R. (1973). ‘The Formation of Planetesimals,’ Astron. Astrophys. 183, 10511061.Google Scholar
Gombosi, T.I., and Houpis, H.L.F. (1986) ‘An Icy-Glue Model of Cometary Nuclei,’ Nature 324, 4344.CrossRefGoogle Scholar
Greenberg, J.M. (1986a) ‘Evidence for the Pristine Nature of Comet Halley,’ in The Comet Nucleus Sample Return Mission, ESA SP-249, pp. 4756.Google Scholar
Greenberg, J.M. (1986b) ‘Fluffy Comets’ in Asteroids, Comets, Meteors II, Lagerkvist, C.-I., Lindblad, B.A., Lunstedt, H., and Rickman, H. (eds.), Uppsala Universitet, Uppsala, Sweden, pp. 221223.Google Scholar
Greenberg, J.M., Grim, R., and van Ijzendoorn, L. (1986). ‘Interstellar S2 in Comets,’ in Asteroids, Comets, Meteors II, Lagerkvist, C.-I., B.A.Lindblad, , Lunstedt, H., and Rickman, H. (eds.), Uppsala Universitet, Uppsala, Sweden, pp. 225227.Google Scholar
Greenberg, R., Wacker, T.F., Hartmann, W.K., and Chapman, C.R. (1978). ‘Planetesimals to Planets: Numerical Simulation of Collisional Evolution,’ Icarus 35, 126.CrossRefGoogle Scholar
Hartmann, W.K. (1978). ‘The Planet-Forming State: Toward a Modern Theory,’ in Protostars and Planets, Gehrels, T. (ed.), University of Arizona Press, Tucson,pp. 5873.Google Scholar
Hayashi, C., and Nakagawa, Y. (1975). ‘Size Distribution of Grains Growing by Thermal Grain-Grain Collision,’ Prog. Theor. Phys. 54, 93103.CrossRefGoogle Scholar
Hills, J.G. (1973). ‘On the Process of Accretion in the Formation of the Planets and Comets,’ Icarus 18, 505522.CrossRefGoogle Scholar
Hills, J.G. (1982). ‘The Formation of Comets by Radiation Pressure in the Outer Protosun,’ Astron. J. 87, 906910.CrossRefGoogle Scholar
Horanyi, M., and Kecskeméty, K. (1983). ‘Percolation Theory and the Origin of Comets,’ in International Conference of Cometary Exploration, Gombosi, T.I. (ed.), Hungarian Acad. Sci., pp. 2125.Google Scholar
Jewitt, D.C., and Meech, K.J. (1988). ‘Optical Properties of Cometary Nuclei and a Preliminary Comparison With Asteroids,’ Astrophys. J. 328, 974986.CrossRefGoogle Scholar
Julien, R., and Meakin, P. (1987). ‘Simple Three-Dimensional Models for Ballistic Deposition With Restructuring,’ Europhys. Lett. 4, 13851390.CrossRefGoogle Scholar
Keller, H.U. (1990) ‘The Nucleus of Comet Halley,’ in Symposium on the Similarity and Diversity of Comets, ESA SP-278, Paris, France, pp. 447454.Google Scholar
Keller, H.U., Delamere, W.A., Huebner, W.F., Reitsema, H.J., Schmidt, H.U., Whipple, F.L., Wilhelm, K., Curdt, W., Kramm, R., Thomas, N. Arpigny, C., Barbieri, C., Bonnet, R.M., Cazes, S., Coradini, M., Cosmovici, C.B., Hughes, D.W., Jamar, C., Malaise, D., Schmidt, K., Schmidt, W.K.H., and Seige, P. (1990). ‘Comet P/Halley’s Nucleus and Its Activity,’ Astron. Astrophys. 187, 807823.Google Scholar
Markiewicz, W.J., and Volk, H.J. (1988). ‘Pre-Planetary Disks and Planet Formation,’ in Formation and Evolution of Low Mass Stars, Dupree, A.K. and Lago, M.J.V. (eds.), Kluwer Academic Publishers, Boston, pp. 181192.CrossRefGoogle Scholar
Meakin, P. (1984). ‘Computer Simulation of Cluster-Cluster Aggregation Using Linear TrajectoriesJ. Coll. Interface Sci. 102, 505512.CrossRefGoogle Scholar
Meakin, P., and Donn, B. (1988). ‘Aerodynamics of Fractal Grains: Implications for the Primordial Solar Nebula,’ Astrophys J. Lett. 329, L39L41.CrossRefGoogle Scholar
Meakin, P., and Julien, R. (1989). ‘The Effects of Restructuring on the Geometry of Clusters Formed by Diffusion Limited, Ballistic and Reaction Limited Cluster-Cluster Aggregation’ to be published.CrossRefGoogle Scholar
Meakin, P., Vicsek, T., and Family, F. (1985). ‘Dynamic Cluster-Size Distribution in Cluster-Cluster Aggregation: Effects of Cluster Diffusivity,’ Phys. Rev. B 31, 564568.CrossRefGoogle ScholarPubMed
Mulholland, G.W. (1989). Private communications, to be published.Google Scholar
Napier, W.M., and Humphries, C.M. (1986). ‘Interstellar Planetesimals—II. Radiative Instability in Dense Molecular Clouds,’ Mon. Not. R. Astr. Soc. 221, 105117.CrossRefGoogle Scholar
O’Dell, C.R. (1973). ‘A New Model for Cometary Nuclei,’ Icarus 19, 137146.CrossRefGoogle Scholar
O’Dell, C.R. (1986). ‘A Possible Comet and Asteroid Link in the Formation of Comets,’ Icarus 67, 7179.CrossRefGoogle Scholar
Opik, E.J. (1966) ‘Sun Grazing Comets and Tidal Disruption,’ Irish Astron J. 7, 141—161.Google Scholar
Opik, E.J. (1973). ‘Comets and the Formation of Planets,’ Astrophys. Space Sci. 21, 307398.CrossRefGoogle Scholar
Oudemans, G.J. (1965). ‘Compaction of Dynamic Powders’ in Science of Ceramics, Stewart, G.H. (ed.), Academic Press, New York, pp. 133146.Google Scholar
Peak, D. (1989). ‘Dust Experiments’ Progress Report, NASA GSFC Grant 5-938, to be published.Google Scholar
Rodriguez, J., Allibert, C.H., and Chaix, J.M. (1986). ‘A Computer Method for Random Packing of Spheres of Unequal Size,’ Powder Technology 47, 2533.CrossRefGoogle Scholar
Russell, H.N., and Menzel, D.H. (1933). ‘The Terrestrial Abundance of the Permanent Gases,’ Proc. Acad. Sci. 19, 9971001.CrossRefGoogle ScholarPubMed
Safronov, V.S. (1969). Evolution of the Protoplanetary Cloud and Formation of the Earth and the Planets, Nauka Press, Moscow (in Russian). Translated in NASA TTF-677 (1972).Google Scholar
Safronov, V.S., and Vityazev, A.V. (1985). Origin of the Solar System,’ Sov Sci. Rev. E. Astrophys. Space Phys. 4, 198.Google Scholar
Samson, R.J., Mulholland, A.W., and Gentry, J.W. (1987). ‘Structural Analysis of Soot Agglomerates,’ Languir 3, 272281.CrossRefGoogle Scholar
Schmidt, O.J. (1955). ‘Role des Particules Solides Dans La Cosmogonie Planetaire,’ Mem. Soc. Roy. Liege, 4 ser, Vol. 15, 638649.Google Scholar
Sekanina, Z. (1981). ‘Rotation and Precession of Cometary Nuclei,’ Ann. Rev. Earth Planet. Sci. 9, 113145.CrossRefGoogle Scholar
Sekanina, Z. (1982). ‘The Problem of Split Comets in Review,’ in Comets, Wilkening, L. (ed.), University of Arizona Press, Tucson, pp. 251287.CrossRefGoogle Scholar
Sekanina, Z. (1990). ‘Gas and Dust Emission From Comets and Life Spans of Active Areas on Their Rotating Nuclei,’ submitted to Astron. J.Google Scholar
Stauffer, D. (1979). ‘Scaling Theory of Percolation Clusters,’ Phys. Rep. 54, 175.CrossRefGoogle Scholar
Stephens, J.R., and Russell, R.W. (1979). ‘Emission and Extinction of Ground and Vapor Condensed Silicates from 4 to 14 Microns and the 10 Micron Silicate Feature,’Astrophys. J. 228, 780786.CrossRefGoogle Scholar
Tielens, A.G.G.M., and Allamandola, L.J. (1987). ‘Composition, Structure, and Chemistry of Interstellar Dust’ in Interstellar Processes, Hollenbach, D.J. and Thronsom, H.A. (eds.), D. Reidel Publishing Company, Boston, pp. 397469.CrossRefGoogle Scholar
Vanysek, V., and Rahe, J. (1978). ‘The 12C/13C Isotope Ratio in Comets, Stars, and Interstellar Matter,’ Moon and Planets 18, 441446.CrossRefGoogle Scholar
Volk, H.J., Jones, F.C., Morfill, G., and Roser, S. (1980). ‘Collisions Between Grains in a Turbulent Gas,’ Astron. Astrophys. 85, 316325.Google Scholar
Weidenschilling, S. J. (1980). ‘Dust to Planetesimals: Settling and Coagulation in the Solar Nebula,’ Icarus 44, 172183.CrossRefGoogle Scholar
Weidenschilling, S. J. (1984). ‘Evolution of Grains in a Turbulent Solar Nebula,’ Icarus 60, 553-567.CrossRefGoogle Scholar
Weissman, P.R. (1985). ‘The Origin of Comets: Implications for Planetary Formation,’ in Protostars and Planets II, Gehreis, T. (ed.), University of Arizona Press, Tucson, pp. 895919.Google Scholar
Weissman, P.R. (1986). ‘Are Cometary Nuclei Primordial Rubble Piles?,’ Nature 320,242244.CrossRefGoogle Scholar
Weitz, D.A., and Oliveria, M. (1984). ‘Fractal Structures Formed by Kinetic Aggregation of Aqueous Gold Colloids,’ Phys. Rev. Letters 52, 14331436.CrossRefGoogle Scholar
Wetherill, G.W. (1980). ‘Formation of the Terrestrial Planets,’ Ann. Rev. Astron. Astrophys. 18 77113.CrossRefGoogle Scholar
Whitlaw-Gray, R., and Patterson, H.S. (1932). Smoke, Edward Arnold Co., London.Google Scholar
Yamamoto, T., and Kozasa, T. (1988). ‘The Cometary Nucleus as an Aggregate of Planetesimals,’ Icarus 75, 540551.CrossRefGoogle Scholar
Yerazunis, S., Bartlett, J.W., and Nissan, A.H. (1962). ‘Packing of Binary Mixtures of Spheres and Irregular Particles,’ Nature 195, 3335.CrossRefGoogle Scholar