Second-Order Normalization in the Generalized Restricted Problem of Three Bodies, Smaller Primary Being an Oblate Spheroid

Details Second-Order Normalization in the Generalized Restricted Problem of Three Bodies, Smaller Primary Being an Oblate Spheroid Second-Order Normalization in the Generalized Restricted Problem of Three Bodies, Smaller Primary Being an Oblate Spheroid

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aj....110.1901m&link_type=abstract

Astronomical Journal v.110, p.1901

Astronomy and Astrophysics

Astronomy

3

Celestial Mechanics, Instabilities

Scientific paper

We have normalized H3, the third-order part of the
Hamiltonian, of our problem by Birkhoff's normalization process. We
conclude that all odd-order Hamiltonian's will be zero. Our problem is
generalized in the sense that the effects of perturbations in coriolis
and centrifugal forces have been taken into consideration.

Affiliated with

Also associated with

No associations

Rating

Second-Order Normalization in the Generalized Restricted Problem of Three Bodies, Smaller Primary Being an Oblate Spheroid 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 Second-Order Normalization in the Generalized Restricted Problem of Three Bodies, Smaller Primary Being an Oblate Spheroid, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Second-Order Normalization in the Generalized Restricted Problem of Three Bodies, Smaller Primary Being an Oblate Spheroid will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1352179