Published 1991
| Version v1
Report
The chaotic dynamics of comets and the problems of the Oort cloud
Creators
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
- Secondary number(s)
- NASA-CR--188165; NAS--1.26:188165; LC--90-62812; CONF-8901223--.