No CrossRef data available.
Article contents
Formation of the Planets
Published online by Cambridge University Press: 14 August 2015
Extract
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.
A timetable for an evolutionary sequence of processes, which begins with the formation of the solar nebula being nearly in equilibrium and ends with the planetary formation, is presented. Basic features of the processes and grounds for the estimation of time-scales are explained for each of the processes.
- Type
- Session 3: Origin of the Solar System
- Information
- Copyright
- Copyright © Reidel 1981
References
Hayashi, C., 1972, Report of the Fifth Symposium on the Moon and Planets at the Institute of Space and Aeronautical Science, University of Tokyo.Google Scholar
Hayashi, C., Nakazawa, K. and Mizuno, H., 1979, Earth and Planetary Science Letters
43, 22.Google Scholar
Mizuno, H., Nakazawa, K. and Hayashi, C., 1980, to be published in
Earth Planet. Sci. Lett.
Google Scholar
Safronov, V.S., 1969, “Evolution of the Protoplanetary Cloud and Formation of the Earth and the Planets”
(Moscow).Google Scholar
Sekiya, M., Nakazawa, K. and Hayashi, C., 1980, to be published in
Earth Planet. Sci. Lett. and also in Prog. Theor. Phys.
Google Scholar