On the RTBP with oblate primary and radiating secondary

Details On the RTBP with oblate primary and radiating secondary On the RTBP with oblate primary and radiating secondary

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..848..748d&link_type=abstract

RECENT ADVANCES IN ASTRONOMY AND ASTROPHYSICS: 7th International Conference of the Hellenic Astronomical Society. AIP Conferenc

Astronomy and Astrophysics

Astrophysics

Celestial Mechanics, Celestial Mechanics, Few- And Many-Body Systems

Scientific paper

We consider a version of the restricted three-body problem which includes the effects of oblateness of the primary body and radiation of the secondary body, determine the equilibrium points and their stability and discuss the zero-velocity curves. We find that both oblateness of the primary and radiation of the secondary reduce the stability region of the isosceles triangle equilibrium points in the parameter space. These effects also reduce the Roche lobe, and thus the sphere of influence, of the secondary.

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