Effects of the mass ratio on the existence of retrograde satellites in the circular plane restricted problem. III

Details Effects of the mass ratio on the existence of retrograde satellites in the circular plane restricted problem. III Effects of the mass ratio on the existence of retrograde satellites in the circular plane restricted problem. III

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....53..231b&link_type=abstract

Astronomy and Astrophysics, vol. 53, no. 2, Dec. 1976, p. 231-236.

Astronomy and Astrophysics

Astrophysics

10

Celestial Mechanics, Circular Orbits, Mass Ratios, Orbital Mechanics, Three Body Problem, Astrophysics, Dynamic Stability

Scientific paper

The existence of stable retrograde satellite orbits at a large distance from the heavier of two massive bodies is investigated numerically within the framework of the circular plane restricted three-body problem. Stability properties and the characteristic of the family of single-periodic symmetric orbits are analyzed for 15 different values of the parameter mu between 0.5 and 1.0. The boundary of the stability zone for general nonperiodic orbits is determined for values of mu ranging from 0.60 to 0.999.

Affiliated with

Also associated with

No associations

Rating

Effects of the mass ratio on the existence of retrograde satellites in the circular plane restricted problem. III 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 Effects of the mass ratio on the existence of retrograde satellites in the circular plane restricted problem. III, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Effects of the mass ratio on the existence of retrograde satellites in the circular plane restricted problem. III will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1047662