Published November 1989 | Version v1
Journal article

Dynamics of Pluto and Charon

  • 1. NASA Ames Research Center, IA (USA)

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