Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28.1373s&link_type=abstract
Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 373.
Astronomy and Astrophysics
Astronomy
1
Solar Corona, Astronomical Models, Solar System Evolution, Protoplanets, T Tauri Stars, Boundary Conditions, Time Dependence, Opacity, Mathematical Models
Scientific paper
According to the current concepts, the solar nebula was an active and changing environment. It appears that it is the evolutionary aspect of the nebula that shapes the global character of the solar system. Thus, solar system origin studies require an evolutionary model of the nebula. To address this situation we have constructed an analytic model of the evolving solar nebula based on the same set of physical principles used in numerical time-dependent models of protoplanetary disks. Final formulas are explicit and readily available to provide the structure of the gaseous solar nebula on demand. The analytic model is conceptually transparent; thus, in comparison with its numerical counterparts, it gives much deeper insights into the inner working of the evolving nebula. It also provides an 'easy-to-use', but physically solid, theoretical framework within which numerous 'origins' issues can be discussed.
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