Engineering PapersโŒ• Search

NASA NTRS ยท 19900027049

Dynamics of Pluto and Charon

Abstract

The dynamics of the Pluto-Charon system are reviewed from a historical perspective. Although Pluto's orbit crosses Neptune's, an intricate system of nested resonances keeps these planets apart. Pluto's orbit is apparently chaotic as well. Pluto always keeps the same face turned toward Charon, and vice versa. Tides also damp Charon's orbital eccentricity and inclination. Precession of Pluto's orbital plane causes Pluto's obliquity to vary periodically from formally prograde to retrograde. Pluto is probably an original member of the Solar system, but not an escaped satellite of Neptune.

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Dobrovolskis, Anthony R.. 1989-11-01. Dynamics of Pluto and Charon. https://ntrs.nasa.gov/citations/19900027049

Cite the original work for its findings. Save a collection to share your selection of sources.