Published 1991 | Version v1
Report

The chaotic dynamics of comets and the problems of the Oort cloud

Description

The dynamic properties of comets entering the planetary zone from the Oort cloud are discussed. Even a very slight influence of the large planets can trigger stochastic cometary dynamics. Multiple interactions of comets with the large planets produce diffusion of the parameters of cometary orbits and a mean increase in the semi-major axis of comets. Comets are lifted towards the Oort cloud, where collisions with stars begin to play a substantial role. The transport of comets differs greatly from the customary law of diffusion and noticeably alter cometary distribution

Additional details

Publishing Information

Imprint Title
Planetary Sciences: American and Soviet Research
Imprint Pagination
vp.
Journal Page Range
p. 259-269.
Report number
N--91-22960

Conference

Title
American and Soviet research.
Acronym
Planetary sciences
Dates
2-6 Jan 1989.
Place
Moscow (USSR).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
22087183
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference, Numerical Data
Descriptors DEI
COLLISIONS; COMETS; COSMOLOGICAL MODELS; DYNAMICS; ORBITS; PLANETS; SOLAR SYSTEM; SOLAR SYSTEM EVOLUTION; STOCHASTIC PROCESSES; THEORETICAL DATA
Descriptors DEC
DATA; INFORMATION; MATHEMATICAL MODELS; MECHANICS; NUMERICAL DATA

Optional Information