Other
Scientific paper
Apr 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986avest..19..344k&link_type=abstract
(Astronomicheskii Vestnik, vol. 19, Oct.-Dec. 1985, p. 344-353) Solar System Research (ISSN 0038-0946), vol. 19, no. 4, April 19
Other
Celestial Mechanics, Planetary Orbits, Solar Oblateness, Solar Rotation, Solar Terrestrial Interactions, Ecliptic, Inclination, Orbit Perturbation, Planetary Evolution, Precession, Solar Orbits, Terrestrial Planets
Scientific paper
Account is taken of the resonances in the solar system to characterize the forces controlling the inclinations of planetary orbits with respect to one another without requiring a severe oblateness in the sun during planetary formation. The precessional motions of the poles of the planets and the sun are analyzed in rectangular coordinates and a system of linear, homogeneous, first-order differential equations is defined to satisfy the requirements of conservation of angular momentum in the solar system. A general solution is defined for the system of equations and is examined for varying degrees of solar oblateness, particularly those at which resonance occurs. The calculations show that the orbital inclinations of the planets could have been caused by a sun with an oblateness of 0.016 and a rotational velocity in the range 48-77 km/sec.
Dzhaparidze D. R.
Kiladze Rolan I.
No associations
LandOfFree
Influence of the oblateness of the early sun on the inclination of planetary orbits. I - Linear theory does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Influence of the oblateness of the early sun on the inclination of planetary orbits. I - Linear theory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Influence of the oblateness of the early sun on the inclination of planetary orbits. I - Linear theory will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1102084