Collinear equilibrium points of Hill's problem with radiation and oblateness and their fractal basins of attraction

Details Collinear equilibrium points of Hill's problem with radiation and oblateness and their fractal basins of attraction Collinear equilibrium points of Hill's problem with radiation and oblateness and their fractal basins of attraction

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ap%26ss.326..263d&link_type=abstract

Astrophysics and Space Science, Volume 326, Issue 2, pp.263-271

Astronomy and Astrophysics

Astrophysics

3

Hill Problem, Collinear Equilibria, Oblateness, Radiation, Fractal Basins

Scientific paper

We discuss the existence, location, and stability of the collinear equilibrium points of a generalized Hill problem with radiation of the primary (the Sun) and oblateness of the secondary (the planet), and present some remarkable fractals created as basins of attraction of Newton’s method applied for their computation in several cases of the parameters.

Affiliated with

Also associated with

No associations

Rating

Collinear equilibrium points of Hill's problem with radiation and oblateness and their fractal basins of attraction 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 Collinear equilibrium points of Hill's problem with radiation and oblateness and their fractal basins of attraction, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Collinear equilibrium points of Hill's problem with radiation and oblateness and their fractal basins of attraction will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1802605