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. The Voyager II encounter with Neptune, the final Pluto-Charon mutual events, and the next generation of telescopes are bound to reveal some surprises.
- Publication:
-
Geophysical Research Letters
- Pub Date:
- November 1989
- DOI:
- 10.1029/GL016i011p01217
- Bibcode:
- 1989GeoRL..16.1217D
- Keywords:
-
- Astrodynamics;
- Charon;
- Planetary Orbits;
- Pluto (Planet);
- Neptune (Planet);
- Solar System;
- Voyager 2 Spacecraft;
- Planetology: Fluid Planets: Origin and evolution;
- History of Geophysics: Planetology;
- Planetology: Solid Surface Planets and Satellites: Orbital and rotational dynamics;
- Planetology: Solid Surface Planets and Satellites: Origin and evolution