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Properties of Ices and Grains: An experimental study

Published online by Cambridge University Press:  30 March 2016

Bertram Dorm*
Affiliation:
Laboratory for Extraterrestrial Physics, Goddard Space Flight Center, Greenbelt, MD 20771

Abstract

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Proton irradiation of a variety of ice mixtures were carried out to study the effect of galactic cosmic ray irradiation of comets in the Oort Cloud. Three significant effects were noted (1) production of new molecules; (2) production of a more energetic ice at low temperatures; (3) production of a non-volatile, complex organic residue. These phenomena suggest various effects on new comets approaching the sun including enhanced activity. Experiments on the condensation of silicate grains provide information on the condensation mechanism and properties of grains. Controlled annealing of the amorphous condensates shows how crystallization occurs. Infrared spectra of different stages of crystallization contain features that may identify composition, structure and history of refractory material.

Type
Joint Discussions
Copyright
Copyright © Reidel 1983

References

Cameron, A.G.W.: 1978, Protostars and Planets, ed. Gehrels, T., Univ. Arizona Press, Tucson, USA, pp. 453487 Google Scholar
Day, K., and Donn, B. : 1978, Astrophys. J. 222, pp. L45L48 Google Scholar
Donn, B.: 1976, The Study of Comets, ed. Donn, B., Murama, M., Jackson, W., Mearn, M.A. and Harrington, R., NASA SP- 393, pp. 611621.Google Scholar
Donn, B., Hecht, J., Khanna, R., Nuth, J., Stranz, D., and Anderson, A.B.: 1981, Surface Sci. 106, pp. 576581.Google Scholar
Fraundorf, P., McKeegan, K.D., Patel, R.I., Sandford, S.A., Swan, P., and Walker, R.M.: 1982, Lunar and Planetary Science XIII, Abstracts, NASA, pp. 229230.Google Scholar
Giese, R.H.: 1980, Solid Particles in the Solar System, eds. Halliday, I. and Mclntosh, B.A., D. Reidel Publ. Co. (Dordrecht, Holland; Boston, USA; London, England), pp. 113.Google Scholar
Greenberg, J.M., and Gustafson, B.A.S.: 1980, Astron. Astrophys. 93, pp. 3542.Google Scholar
Knacke, R., and Kratschmer, W.: 1980, Astron. Astrophys. 92, pp. 281288.Google Scholar
McSween, H.Y.: 1979, Rev. Geophys. Space Phys., pp. 10591078.Google Scholar
Nuth, J., and Donn, B.: 1982a, Astrophys. J. 257, pp. L103L105.Google Scholar
Nuth, J., and Donn, B.: 1982b, J. Chem. Phys. 77, pp. 26392646.Google Scholar
Protostars and Planets: 1978, ed. Gehrels, T., Univ. Arizona Press, Tucson, USA, pp. 488624.Google Scholar
Shul’man, L.M.: 1972, The Motion, Evolution of Orbits and the Origin of Comets, eds. Chebotarev, G.A., Kazimirchak-Polonskaya, E.I. and Marsden, B.G., D. Reidel Publ. Co. (Dordrecht, Holland), pp. 265270.Google Scholar
Wetherill, G.W.: 1980, Ann. Rev. Astron. Astrophys. 18, pp. 77113.Google Scholar
Whipple, F.L.: 1977, Comets-Asteroids-Meteorites, ed. Delsemme, A.H., Univ. Toledo Press, Toledo, USA, pp. 2536.Google Scholar
Wood, J.A.: 1981, Earth Planet. Sci. Letters 56, pp. 3244.Google Scholar