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Evidence for Physical Aging of Periodic Comets

Published online by Cambridge University Press:  12 April 2016

L. Kresák*
Affiliation:
Astronomical Institute, Slovak Academy of Sciences 84228 Bratislava, Czechoslovakia

Abstract

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Observational evidence for the aging processes in periodic comets is reviewed. This includes progressive changes of the comets’ absolute brightness, sudden destructive events (outbursts and splitting of cometary nuclei), temporary intermissions in activity, total disappearance, and existence of asteroidal objects moving in cometary orbits. Indirect statistical evidence is provided by the equilibrium between the aging rate and the net injection of comets into the inner planetary system. All of this information is consistent with typical active lifetimes of 200 to 500 revolutions at small perihelion distances (q < 3 AU). The active lifetimes are sometimes intermitted by dormant periods, which tend to occur especially during the latest phases of evolution. Splits and outbursts do not seem to have a decisive statistical effect on the survival time. Some periodic comets evolve into inactive asteroid-like objects, but the question of whether these still contain some supply of volatiles, and thus can renew their activity, remains open.

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

References

Bibliography and References

Andrienko, D.A., and Karpenko, A.V. (1987). Fizicheskie kharakteristiki komet 1976-1980 gg., Nauka, Moskva.Google Scholar
Babadzhanov, P.B., and Obrubov, Yu.V. (1983). “Secular perturbations of Apollo, Amor and Aten asteroid orbits and theoretical radiants of meteor showers probably associated with them,” in Lagerkvist, C.-I. and Rickman, H. (eds.), Asteroids, Comets, Meteors, Univ. Uppsala, 411417.Google Scholar
Bailey, M.E. (1983). “The structure and evolution of the solar system comet cloud,Mon. Not. Roy. Astron. Soc. 204, 603633.CrossRefGoogle Scholar
Bailey, M.E., Clube, S.V.M., and Napier, W.M. (1986). “The origin of comets,Vistas Astron. 29, 52112.CrossRefGoogle Scholar
Belyaev, N.A., Kresák, Ľ, Pittich, E.M., and Pushkarev, A.N. (1986). Catalogue of Short-Period Comets, Veda, Bratislava.Google Scholar
Bobrovnikoff, N.T. (1941). “Investigations of the brightness of comets, Part I,” Contrib. Perkins Obs. 15, 49187.Google Scholar
Bobrovnikoff, N.T. (1942). “Investigations of the brightness of comets, Part II,” Contrib. Perkins Obs. 16, 189300.Google Scholar
Carusi, A., Kresák, Ľ, Perozzi, E., and Valsecchi, G.B. (1985a). Long-Term Evolution of Short-Period Comets, A. Hilger, Bristol.Google Scholar
Carusi, A., Kresák, Ľ, Perozzi, E., and Valsecchi, G.B. (1985b). “First results of the integration of motion of short-period comets over 800 years,” in Carusi, A. and Valsecchi, G.B. (eds.), Dynamics of Comets: Their Origin and Evolution, IAU Coll. 83, D. Reidel, Dordrecht, 319340.CrossRefGoogle Scholar
Carusi, A., Kresák, Ľ, Perozzi, E., and Valsecchi, G.B. (1987). “Long-term resonances and orbital evolutions of Halley-type comets,” in Ceplecha, Z. and Pecina, P. (eds.), Interplanetary Matter, ERAM 10, Publ. Astron. Inst. Czechosl. Acad. Sci. 67, 2932.Google Scholar
Clube, S.V.M., and Napier, V.M. (1984). “Comet capture from molecular clouds: A dynamical constraint on star and planet formation,” Mon. Not. Roy. Astron. Soc. 208, 575588.Google Scholar
Crifo, J.F. (1987). “Are cometary dust mass loss rates deduced from optical emissions reliable?”, in Ceplecha, Z. and Pecina, P. (eds.), Interplanetary Matter, ERAM 10, Publ. Astron. Inst. Czechosl. Acad. Sci. 67, 5966.Google Scholar
Degewij, J., and Tedesco, E.F. (1982). “Do comets evolve into asteroids? Evidence from physical studies,” in Wilkening, L.L. and Matthews, M.S. (eds.), Comets, IAU Coll. 61, Univ. Arizona, Tucson, 665695.Google Scholar
Delsemme, A.H. (1976). “Can comets be the only source of interplanetary dust?”, in Elsässer, H. and Fechtig, H. (eds.), Interplanetary Dust and Zodiacal Light, IAU Coll. 31, Lecture Notes in Physics 48, 481484.Google Scholar
Dermott, S.F., Nicholson, P.D., Burns, J.A., and Houck, J.R. (1985). “An analysis of IRAS solar system dust bands,” in Giese, R. and Lamy, P. (eds.), Properties and Interactions of Interplanetary Dust, IAU Coll. 85, D. Reidel, Dordrecht, 395409.Google Scholar
Dobrovolsky, O.V., Ibadinov, Kh.I., Aliev, S., and Gerasimenko, S.I. (1986). “Thermal regime and surface structure of periodic comet nuclei,” in Battrick, B., Rolfe, E.J., and Reinhard, R. (eds.), Exploration of Halley’s Comet, ESA SP-250, Vol. 2, 389394.Google Scholar
Drummond, J.D. (1982). “Theoretical meteor radiants of Apollo, Amor, and Aten asteroids,” Icarus 49, 143153.Google Scholar
Duncan, M., Quinn, T., and Tremaine, S. (1987). “The formation and extent of the solar system comet cloud,” Astron. J. 94, 13301338.Google Scholar
Everhart, E. (1976). “The evolution of comet orbits,” in Donn, B., Mumma, M., Jackson, W., A’Hearn, M., and Harrington, R. (eds.), The Study of Comets, IAU Coll. 25, NASA SP-393, 445464.Google Scholar
Everhart, E. (1977). “The evolution of comet orbits as perturbed by Uranus and Neptune,” in Delsemme, A.H. (ed.), Comets, Asteroids, Meteorites, IAU Coll. 39, Univ. Toledo, 99104.Google Scholar
Fernández, J.A. (1981). “New and evolved comets in the solar system,” Astron. Astrophys. 96, 2635.Google Scholar
Fernández, J.A. (1985a). “The formation and dynamical survival of the comet cloud,” in Carusi, A. and Valsecchi, G.B. (eds.), Dynamics of Comets: Their Origin and Evolution, IAU Coll. 83, D. Reidel, Dordrecht, 4570.CrossRefGoogle Scholar
Fernández, J.A. (1985b). “Dynamical capture and physical decay of short-period comets,” Icarus 64, 308319.Google Scholar
Fernández, J.A., and Ip, W.-H. (1983). “On the time evolution of the cometary influx into the region of the terrestrial planets,” Icarus 54, 377387.Google Scholar
Galibina, I.V., and Kastel, G.R. (1982). “On possible association of the asteroid 2212 - 1978 SB with the comet Encke,” Komety i meteory 33, 4546.Google Scholar
Green, S.F., McDonnell, J.A.M., Perry, C.H., Nappo, S., and Zarnecki, J.C. (1987). “P/Halley dust coma: Grains or rocks?”, in Rolfe, E.J. and Battrick, B. (eds.), Diversity and Similarity of Comets, ESA SP-278, 379384.Google Scholar
Guliev, A.S., and Bajramov, A.Sh. (1988). “New statistical approach to the problem of cometary brightness fading,” Kinematika i fizika nebesnykh tel 4, 3034.Google Scholar
Hahn, G., and Rickman, H. (1985). “Asteroids in cometary orbits,” Icarus 61, 417442.Google Scholar
Hajduk, A. (1986). “Debris from comet Halley and the risk for space probes,” in Lagerkvist, C.-I., Lindblad, B.A., Lundstedt, H., and Rickman, H. (eds.), Asteroids, Comets, Meteors II, Univ. Uppsala, 497500.Google Scholar
Hills, J.G. (1981). “Comet showers and the steady state infall of comets from the Oort cloud,” Astron. J. 86, 17301740.Google Scholar
Holetschek, J. (1916). “Untersuchungen über die Grösse und Helligkeit der Kometen und ihrer Schweife, IV,” Wiener Denkschrifte math. nat. Klasse 93, 1105.Google Scholar
Holetschek, J. (1917). “Untersuchungen über die Grosse und Helligkeit der Kometen und ihrer Schweife, V,” Wiener Denkschrifte math. nat. Klasse 94, 1114.Google Scholar
Hughes, D.W. (1975). “Cometary outbursts: A brief survey,” Quart. Roy. Astron. Soc. 16, 410427.Google Scholar
Hughes, D.W., and Daniels, P.A. (1983). “The secular variation of cometary magnitude,” Icarus 53, 444452.Google Scholar
Jacchia, L.G., Verniani, F., and Briggs, R.E. (1967). “An analysis of the atmospheric trajectories of 413 precisely reduced photographic meteors,” Smithson. Contr. Astrophys. 10, 1139.CrossRefGoogle Scholar
Joss, P.C. (1973). “On the origin of short-period comets,” Astron. Astrophys. 25, 271273.Google Scholar
Keller, H.U. (1987). “The nucleus of comet Halley,” in Rolfe, E.J. and Battrick, B. (eds.), Diversity and Similarity of Comets, ESA SP-278, 447454.Google Scholar
Kozai, Y. (1979). “Secular perturbations of asteroids and comets,” in Duncombe, R.L. (ed.), Dynamics of the Solar System, IAU Symp. 81, 231237.Google Scholar
Kresák, Ľ (1966). “On two aspects of evolution of short-period comets,” in Swings, P. (ed.), Nature et Origine des Comètes, Mém. Soc. Roy. Sci. Liège, Ser. 5, 12, 459467.Google Scholar
Kresák, Ľ (1974). “The aging and the brightness decrease of comets,” Bull. Astron. Inst. Czechosl. 25, 87112.Google Scholar
Kresák, Ľ (1979). “Dynamical interrelations among comets and asteroids,” in Gehrels, T. and Matthews, M.S. (eds.), Asteroids, Univ. Arizona, Tucson, 289309.Google Scholar
Kresák, Ľ (1980). “Sources of interplanetary dust,” in Halliday, I. and McIntosh, B.A. (eds.). Solid Particles in the Solar System, IAU Symp. 90, 211222.Google Scholar
Kresák, Ľ (1981a). “Evolutionary aspects of the splits of cometary nuclei,” Bull. Astron. Inst. Czechosl. 32, 1940.Google Scholar
Kresák, Ľ (1981b). “The lifetimes and disappearance of periodic comets,” Bull. Astron. Inst. Czechosl. 32, 321339.Google Scholar
Kresák, Ľ (1982). “Comet discoveries, statistics, and observational selection,” in Wilkening, L.L. and Matthews, M.S. (eds.), Comets, IAU Coll. 61, Univ. Arizona, Tucson, 5682.Google Scholar
Kresák, Ľ (1984). “The lifetimes and disappearance of long-period comets,” Bull. Astron. Inst. Czechosl. 35, 129150.Google Scholar
Kresák, Ľ (1985). “The aging and lifetimes of comets,” in Carusi, A. and Valsecchi, G.B. (eds.), Dynamics of Comets: Their Origin and Evolution, IAU Coll. 83, D. Reidel, Dordrecht, 279302.CrossRefGoogle Scholar
Kresák, Ľ (1986). “On the aging process of periodic comets,” in Battrick, B., Rolfe, E.J., and Reinhard, R. (eds.), Exploration of Halley’s Comet, ESA SP-250, Vol. 2, 433438.Google Scholar
Kresák, Ľ. (eds.), The Evolution of the Small Bodies of the Solar System, Proc. Internat. School Phys. Enrico Fermi 98, North-Holland, Amsterdam, 1032.Google Scholar
Kresák, Ľ (1987b). “The 1808 apparition and the long-term physical evolution of periodic comet Grigg-Skjellerup,” Bull. Astron. Inst. Czechosl. 38, 6575.Google Scholar
Kresák, Ľ (1987c). “Dormant phases in the aging of periodic comets,” Astron. Astrophys. 187, 906908.Google Scholar
Kresák, Ľ, and Kresáková, M. (1987a). “The absolute total magnitude of periodic comets and their variations,” in Rolfe, E.J. and Battrick, B. (eds.), Diversity and Similarity of Comets, ESA SP-278, 3742.Google Scholar
Kresák, Ľ, and Kresáková, M. (1987b). “The contribution of periodic comets to the Zodiacal cloud,” in Ceplecha, Z. and Pecina, P. (eds.), Interplanetary Matter, ERAM 10, Publ. Astron. Inst. Czechosl. Acad. Sci. 67, 265271.Google Scholar
Kresák, Ľ, and Kresáková, M. (1989a). “The absolute magnitudes of periodic comets, I and II,” Bull. Astron. Inst. Czechosl. 40, 269284, and in press.Google Scholar
Kresák, Ľ, and Kresáková, M. (1989b). “On the secular brightness decrease of periodic comets,” Icarus, in press.Google Scholar
Kuiper, G.P. (1951). “On the origin of the solar system,” in Hynek, J.A. (ed.), Astrophysics, McGraw-Hill, New York, 357427.Google Scholar
Marsden, B.G. (1985). “Nongravitational forces in comets: The first fifteen years,” in Carusi, A. and Valsecchi, G.B. (eds.), Dynamics of Comets: Their Origin and Evolution, IAU Coll. 83, D. Reidel, Dordrecht, 343352.Google Scholar
Marsden, B.G., and Bardwell, C.M. (1982). Catalogue of Orbits of Unnumbered Minor Planets, IAU Minor Planet Center, Cambridge.Google Scholar
Marsden, B.G., and Roemer, E. (1982). “Basic information and references,” in Wilkening, L.L. and Matthews, M.S. (eds.), Comets, IAU Coll. 61, Univ. Arizona, Tucson, 707733.Google Scholar
McDonnell, J.A.M., Kissel, J., Grün, E., Grard, R.J.L., Langevin, Y., Olearczyk, R.E., Perry, C.H., and Zarnecki, J.C. (1986). “Giotto’s dust impact detection system DIDSY and particulate impact analyser PIA: Interim assessment of the dust distribution and properties within the coma,” in Battrick, B., Rolfe, E.J., and R. Reinhard, (eds.), Exploration of Halley’s Comet, ESA SP-250, Vol. 2, 2538.Google Scholar
McFadden, L.A., Gaffey, M.J., and McCord, T.B. (1984). “Mineralogical-petrological characterization of near-Earth asteroids,” Icarus 59, 2540.Google Scholar
Meech, K.J., and Belton, M.J.S. (1989). “2060 Chiron,” IAU Circ. No. 4770.Google Scholar
Meisel, D.D., and Morris, C.S. (1976) ‘Comet brightness parameters: Definition, determination and correlations,’ in Donn, B., Mumma, M., Jackson, W., A’Hearn, M.A. and Harrington, R., The Study of Comets, IAU Coll. 25, NASA SP-393, 410444.Google Scholar
Meisel, D.D., and Morris, C.S. (1982). “Comet head photometry: Past, present, and future,” in Wilkening, L.L. and Matthews, M.S. (eds.), Comets, IAU Coll. 61, Univ. Arizona, Tucson, 413432.Google Scholar
Milani, A., Carpino, M., Hahn, G., and Nobili, A.M. (1989). “Dynamics of planet-crossing asteroids: Classes of orbital behavior. Project Spaceguard,” Icarus 78, 212269.Google Scholar
Morris, C.S. (1973). “On aperture corrections for comet magnitude estimates,” Publ. Astron. Soc. Pacific 85, 470473.Google Scholar
Nakano, S. (1984). “Identifications of comets and minor planets,” Japan Astron. Circ. No. 409.Google Scholar
Nakano, S. (1987). “Identifications with comets,” Minor Planet Circ. 12025.Google Scholar
Nakano, S. (1988). “Identifications with a comet,” Minor Planet Circ. 12626.Google Scholar
Nakano, S. (1989). “Identifications with comets,” Minor Planet Circ. 14384.Google Scholar
Napier, W.M. (1983). “The orbital evolution of short period comets,” in Lagerkvist, C.-I. and Rickman, H. (eds.), Asteroids, Comets, Meteors, Univ. Uppsala, 391396.Google Scholar
Oikawa, S., and Everhart, E. (1979). “Past and future orbit of 1977 UB, object Chiron,” Astron. J. 84, 134139.Google Scholar
Olsson-Steel, D. (1987a). “Asteroid 5025 P-L, comet 1967 II Rudnicki, and the Taurid meteoroid complex,” Observatory 107, 157160.Google Scholar
Olsson-Steel, D. (1987b). “Meteoroid streams associated with Apollo asteroids: Evidence from the Adelaide radar orbit surveys,” in Ceplecha, Z. and Pecina, P. (eds.), Interplanetary Matter, ERAM 10, Publ. Astron. Inst. Czechosl. Acad. Sci. 67, 125129.Google Scholar
Olsson-Steel, D. (1988). “Identification of meteoroid streams from Apollo asteroids in the Adelaide radar orbit surveys,” Icarus 75, 6496.CrossRefGoogle Scholar
Pons, J.L. (1829). “Notizen über den 1808 am 6ten Februar von Pons entdeckten Cometen,” Astron. Nachr. 7, 113 Google Scholar
Rickman, H. (1985). “Interrelations between comets and asteroids,” in Carusi, A. and Valsecchi, G.B. (eds.), Dynamics of Comets: Their Origin and Evolution, IAU Coll. 83, D. Reidel, Dordrecht, 149172.Google Scholar
Rickman, H. (1986). “Masses and densities of comets Halley and Kopff,” in Melita, O. (ed.), Comet Nucleus Sample Return, ESA SP-249, 195205.Google Scholar
Rickman, H., and Vaghi, S. (1976). “A Monte Carlo simulation of the orbital evolution of comets in the inner planetary region,” Astron. Astrophys. 51, 327342.Google Scholar
Rickman, H., Kamei, L., Festou, M.C., and Froeschlé, C. (1987). “Estimates of masses, volumes and densities of short-period comet nuclei,” in Rolfe, E.J. and Battrick, B. (eds.), Diversity and Similarity of Comets, ESA SP-278, 471481.Google Scholar
Russell, C.T., Aroian, R., Arghavani, M., and Nock, K. (1984). “Interplanetary magnetic field enhancements and their association with the asteroid 2201 Oljato,” Science 226, 4345.Google Scholar
Sekanina, Z. (1964). “Secular variations in the absolute brightness of short-period comets,” Bull. Astron. Inst. Czechosl. 15, 116.Google Scholar
Sekanina, Z. (1976). “Statistical model of meteor streams, IV. A study of radio streams from the synoptic year,” Icarus 27, 265321.Google Scholar
Sekanina, Z. (1982). “The problem of split comets in review,” in Wilkening, L.L. and Matthews, M.S. (eds.), Comets, IAU Coll. 61, Univ. Arizona, Tucson, 251-287. Sekanina, Z. (1984). “Disappearance and disintegration of comets,” Icarus 58, 81100.Google Scholar
Shulman, L.M. (1972). “The evolution of cometary nuclei,” in Chebotarev, G.A., Kazimirchak-Polonskaya, E.I., and Marsden, B.G. (eds.), The Motion, Evolution of Orbits, and Origin of Comets, IAU Symp. 45, 271276.Google Scholar
Štohl, L. (1986). “On meteor contribution by short-period comets,” in Battrick, B., Rolfe, E.J., and Reinhard, R. (eds.), Exploration of Halley’s Comet, ESA SP-250, Vol. 2, 225228.Google Scholar
Štohl, L. (1987). “On meteor contribution by short-period comets,” Astron. Astrophys. 187, 933934.Google Scholar
Svoren, J. (1979). “Secular variations in the absolute brightness of periodic comets,” Contr. Astron. Obs. Skalnaté Pleso 8, 105140.Google Scholar
Vsekhsvyatskij, S.K. (1958). Fizicheskie kharakteristiki komet, Fizmatgizdat, Moskva. English translation: Physical Characteristics of Comets, Israel Program for Scientific Translations, Jerusalem, 1964.Google Scholar
Vsekhsvyatskij, S.K. (1966). Fizicheskie kharakteristiki komet nablyudavshikhsya v 1954–1960 gg., Nauka, Moskva. Abbreviated English translation: Sov. Astron. 6, 849-854.Google Scholar
Vsekhsvyatskij, S.K. (1967). Komety 1961-1965 gg., Nauka, Moskva. Abbreviated English translation: Sov. Astron. 10, 1034-1041.Google Scholar
Vsekhsvyatskij, S.K. (1972). “Cometary observations and variations in cometary brightness,” in Chebotarev, G.A., Kazimirchak-Polonskaya, E.I., and Marsden, B.G. (eds.), The Motion, Evolution of Orbits, and Origin of Comets, IAU Symp. 45, 915.Google Scholar
Vsekhsvyatskij, S.K. (1979). Fizicheskie kharakteristiki komet 1971-1975 gg., Naukova Dumka, Kiev.Google Scholar
Vsekhsvyatskij, S.K., and Ilchischina, N.I. (1974). Fizicheskie kharakteristiki komet 1965-1970 gg., Nauka, Moskva. Abbreviated English translation: Sov, Astron. 15, 310-313.Google Scholar
Weissman, P.R. (1982). “Dynamical history of the Oort cloud,” in Wilkening, L.L. and Matthews, M.S. (eds.), Comets, IAU Coll. 61, Univ. Arizona, Tucson, 637658.Google Scholar
Weissman, P.R. (1986). “The Oort cloud in transition,” in Lagerkvist, C.-I., Lindblad, B.A., Lundstedt, H., and Rickman, H. (eds.), Asteroids, Comets, Meteors II, Univ. Uppsala, 197206.Google Scholar
Whipple, F.L. (1964). “Evidence for a comet belt beyond Neptune,” Proc. Natl. Acad. Sci. 51, 711718.Google Scholar
Whipple, F.L. (1967). “On maintaining the meteoritic complex,” in Weinberg, J.L. (ed.), The Zodiacal Light and the Interplanetary Medium, NASA SP-150, 409426.Google Scholar
Whipple, F.L. (1972). “The origin of comets,” in Chebotarev, G.A., Kazimirchak-Polonskaya, E.I., and Marsden, B.G. (eds.), The Motion, Evolution of Orbits, and Origin of Comets, IAU Symp. 45, 401409.Google Scholar
Whipple, F.L. (1978a). “Comets,” in McDonnell, J.A.M. (ed.), Cosmic Dust, J. Wiley, Chichester, 173.Google Scholar
Whipple, F.L. (1978b). “Cometary brightness variation and nucleus structure,” Moon and Planets 18, 343359.Google Scholar
Whipple, F.L. (1980). “Rotation and outbursts of comet P/Schwassmann-Wachmann 1,” Astron. J. 85, 305313.Google Scholar
Whipple, F.L. (1983a). “Comets: Nature, evolution, and decay,” in West, R.M. (ed.), Highlights of Astronomy 6, D. Reidel, Dordrecht, 323331.Google Scholar
Whipple, F.L. (1983b). “1983 TB and the Geminid meteors,” IAU Circ. No. 3881.Google Scholar
Whipple, F.L. (1984). “Comet P/Holmes 1892 III — A case of duplicity?”, Icarus 60, 522531.Google Scholar
Whipple, F.L. (1986). “The cometary nucleus: Current concepts,” in Battrick, B., Rolfe, E.J., and Reinhard, R. (eds.), Exploration of Halley’s Comet, ESA SP-250, Vol. 2, 281288.Google Scholar
Whipple, F.L. (1987). “The cometary nucleus: Current concepts,” Astron. Astrophys. 187, 852858.Google Scholar
Whipple, F.L., and Douglas-Hamilton, D.H. (1966). “Brightness changes in periodic comets,” in Swings, P. (ed.), Nature et Origine des Comètes, Mém. Soc. Roy. Sci. Liège, Ser. 5, 12, 469480.Google Scholar
Whipple, F.L., and Hamid, S.E. (1972). “A search for Encke’s comet in ancient Chineserecords: A progress report,” in Chebotarev, G.A., Kazimirchak-Polonskaya, E.I., and Marsden, B.G. (eds.), The Motion, Evolution of Orbits, and Origin of Comets, IAU Symp. 45, 152154.Google Scholar