Published September 7, 2008 | Version v1
Journal article

Dynamics of self-gravitating dust clouds in astrophysical plasmas

  • 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

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