Published November 1989
| Version v1
Journal article
Dynamics of Pluto and Charon
Description
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 escape 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
Additional details
Publishing Information
- Journal Title
- Geophysical Research Letters
- Journal Volume
- 16
- Journal Issue
- 11
- Series
- Geophys. Res. Lett.
- Journal Page Range
- 1217-1220
- ISSN
- 0094-8276
- CODEN
- GPRLA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 22053330
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- DISTANCE; DYNAMICS; GRAVITATIONAL INTERACTIONS; NEPTUNE PLANET; ORBITS; PLUTO PLANET; PRECESSION; RESONANCE; ROTATION; SATELLITES; SOLAR SYSTEM; SOLAR SYSTEM EVOLUTION; TIDE
- Descriptors DEC
- BASIC INTERACTIONS; MECHANICS; PLANETS