Hostname: page-component-7479d7b7d-m9pkr Total loading time: 0 Render date: 2024-07-11T18:21:13.496Z Has data issue: false hasContentIssue false

Cometary and Asteroidal Sources of Interplanetary Dust

Published online by Cambridge University Press:  12 April 2016

Mark V. Sykes*
Affiliation:
Steward ObservatoryUniversity of ArizonaTucson AZ 85721USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Infrared Astronomical Satellite has provided extensive observations of the zodiacal cloud at high spatial resolution which will not be matched in the forseeable future. Within the zodiacal cloud, IRAS discovered extended dust structures providing the link between the interplanetary dust complex and the asteroids and comets which are its source. These are the asteroid dust bands and the cometary dust trails.

Type
Origin of Interplanetary Dust: from Comets and Asteroids, Back to Interstellar Dust
Copyright
Copyright © Kluwer 1991

References

[1] Whipple, F. (1955) ‘A comet model. III. The zodiacal light’, Astroph. J. 121, 750770.Google Scholar
[2] Whipple, F. (1967) ‘On maintaining the meteoritic complex’, in Weinberg, J.L. (ed.), The Zodiacal Light and the Interplanetary Medium, pp. 409426. NASA SP-150.Google Scholar
[3] Whipple, F. (1976) ‘Sources of interplanetary dust’, in Elsässer, H. and Fechtig, H. (eds.), Lecture Notes in Physics No. 48, Interplanetary Dust and Zodiacal Light, Springer-Verlag, New York, pp. 403415.Google Scholar
[4] Delsemme, A. H. (1976) ‘The production rate of dust by comets’, in Elsässer, H. and Fechtig, H. (eds.), Lecture Notes in Physics No. 48, Interplanetary Dust and Zodiacal Light, Springer-Verlag, New York, pp. 314318.Google Scholar
[5] Röser, S. (1976) ‘Can short period comets maintain the zodiacal cloud?’, in Elsässer, H. and Fechtig, H. (eds.), Lecture Notes in Physics No. 48, Interplanetary Dust and Zodiacal Light, Springer-Verlag, New York, pp. 319322.Google Scholar
[6] Dohnanyi, J.S. (1976) ‘Sources of interplanetary dust: Asteroids’, in Elsässer, H. and Fechtig, H. (eds.), Lecture Notes in Physics No. 48, Interplanetary Dust and Zodiacal Light, Springer-Verlag, New York, pp. 187205.Google Scholar
[7] Neugebauer, G. et al. (1984) ‘The Infrared Astronomical Satellite (IRAS)mission’, Astrophys. J. 278, L1L6.CrossRefGoogle Scholar
[8] Sykes, M. (1986) ‘The discovery of dust trails in the orbits of periodic cometsScience 232, 11151117.Google Scholar
[9] Low, F.J. et al. (1984) ‘Infrared cirrus: New components of the extended infrared emission’, Astrophys. J. 278, L19L22.Google Scholar
[10] Bulyaev, N., Kresák, Ľ Pittich, E., and Pushkarev, A. (1986) Catalog of Short-Period Comets, Astronomical Institute of the Slovak Academy of Sciences, Bratislava.Google Scholar
[11] Sykes, M. and Walker, R. (1991) ‘Cometary Dust Trails. I. The IRAS Survey’, Submitted to Icarus. Google Scholar
[12] Keller, H. et al. (1986) ‘First Halley Multicolour Camera imaging results from Giotto’, Nature 321, 320325.Google Scholar
[13] Sagdeev, R. et al. (1986) ‘Television observations of comet Halley from Vega spacecraft’, Nature 321, 262266.Google Scholar
[14] Campine, H., A’Hearn, M., and McFadden, L.-A. (1987) ‘The bare nucleus of Comet Neujmin 1’, Astrophys. J. 316, 847857.Google Scholar
[15] Millis, R., A’Hearn, M., and Campine, H. (1988) ‘An investigation of the nucleus and coma of P/Arend-Rigaux’, Astrophys. J. 324, 11941209.Google Scholar
[16] A’Hearn, M., Campins, H., Schleicher, D., and Millis, R. (1989) ‘The nucleus of comet P/Tempel 2’, Astrophys. J. 347, 11551166.Google Scholar
[17] Kresák, Ľ and Kresáková, M. (1987) in Rofe, E. J. and Battrick, B., Symposium on the Diversity and Similarity of Comets, ESA SP-278, pp. 729744.Google Scholar
[18] Reach, W. (1988) ‘Zodiacal emission. I. Dust near the Earth’s orbit’, Astrophys. J. 335, 468485.CrossRefGoogle Scholar
[19] Good, J. (1991) ‘Zodiacal dust cloud modelling using IRAS data’, submitted to Astrophys. J.Google Scholar
[20] Gustafson, B., Misconi, N. and Rusk, E. (1987) ‘Interplanetary dust dynamics. II. Poynting-Robertson drag and planetary perturbations on cometary dust’, Icarus 72, 568581.Google Scholar
[21] Sykes, M. (1990) ‘Zodiacal dust bands: Their relation to asteroid families’, Icarus 85, 267289.Google Scholar
[22] Dermott, S., Nicholson, P., Burns, J., and Houck, J. (1984) ‘Origin of the solar system dust bands discovered by IRAS’, Nature 312, 505509.Google Scholar
[23] Sykes, M. (1988) ‘IRAS observations of extended zodiacal structures’, Astrophys. J. 334, L55L58.Google Scholar
[24] Sykes, M. and Greenberg, R. (1986) ‘The formation and origin of the IRAS zodiacal dust bands as a consequence of single collisions between asteroids’, Icarus 65, 5169.Google Scholar
[25] Sykes, M. (1989) ‘Asteroidal sources of dust at the Earth’s orbit’, Meteoritics 24, 330.Google Scholar