Linear stability of the triangular equilibrium points in the photogravitational elliptic restricted problem.

Details Linear stability of the triangular equilibrium points in the photogravitational elliptic restricted problem. Linear stability of the triangular equilibrium points in the photogravitational elliptic restricted problem.

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.194..207m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 194, no. 2, p. 207-213.

Astronomy and Astrophysics

Astrophysics

3

Equations Of Motion, Lagrangian Equilibrium Points, Radiation Pressure, Solar System, Three Body Problem, Gravitational Fields, Riccati Equation

Scientific paper

The linear stability of the triangular equilibrium points in the photogravitational elliptic restricted problem is examined and the stability regions are determined in the space of the parameters of mass, eccentricity, and radiation pressure. It is found that radiation pressure of the larger body for solar system cases exerts only a small quantitative influence on the stability regions.

Affiliated with

Also associated with

No associations

Rating

Linear stability of the triangular equilibrium points in the photogravitational elliptic restricted problem. 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 Linear stability of the triangular equilibrium points in the photogravitational elliptic restricted problem., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Linear stability of the triangular equilibrium points in the photogravitational elliptic restricted problem. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1165573