Published September 7, 2008
| Version v1
Journal article
Dynamics of self-gravitating dust clouds in astrophysical plasmas
Creators
- 1. Department of Physics, Umea ring University, SE-90 187 Umea ring (Sweden)
- 2. IGPP, University of California, Riverside, CA 92521 (United States)
- 3. Theoretische Physik IV, Ruhr-Universitaet Bochum, D-44780 Bochum (Germany)
Description
Due to the gravitational force, clouds of dust and gas in the interstellar medium can contract and form stars and planet systems. We here show that if the dust grains are electrically charged then the self-gravitation can be balanced by the ion pressure, and the collapse can be halted. In this case, the dust cloud may form soft dust planets, having the weight of a small moon or satellite, but a radius larger than of our Sun. There exist a critical mass beyond which the dust cloud collapses and forms a solid planet.
Additional details
Identifiers
- DOI
- 10.1063/1.2996717;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1041
- Journal Issue
- 1
- Journal Page Range
- p. 109-112
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 5. international conference on the physics of dusty plasmas
- Dates
- 18-23 May 2008
- Place
- Ponta Degada, Azores (Portugal)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41002527
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; COSMIC DUST; COULOMB FIELD; GRAVITATION; IONS; MAGNETOHYDRODYNAMICS; PLASMA; RF SYSTEMS
- Descriptors DEC
- CHARGED PARTICLES; DUSTS; ELECTRIC FIELDS; FLUID MECHANICS; HYDRODYNAMICS; MECHANICS; PHYSICS
Optional Information
- Notes
- (c) 2008 American Institute of Physics