Sign on

SAO/NASA ADS Astronomy Abstract Service

· Find Similar Abstracts (with default settings below)
· Full Refereed Journal Article (PDF/Postscript)
· Full Refereed Scanned Article (GIF)
· References in the article
· Citations to the Article (152) (Citation History)
· Refereed Citations to the Article
· Associated Articles
· Also-Read Articles (Reads History)
· Translate This Page
On the tidal interaction between protoplanets and the primordial solar nebula. I - Linear calculation of the role of angular momentum exchange
Papaloizou, J.; Lin, D. N. C.
AA(Queen Mary College, London, England), AB(Lick Observatory, Santa Cruz, CA)
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 285, Oct. 15, 1984, p. 818-834. (ApJ Homepage)
Publication Date:
NASA/STI Keywords:
Planetary Evolution, Protoplanets, Solar Corona, Solar System, Tides, Angular Momentum, Asymptotic Methods, Fourier Analysis, Momentum Transfer, Polytropic Processes, Rotating Disks
Bibliographic Code:


In the first paper of this series the tidal interaction between a protoplanet and a gaseous protoplanetary disk with moderate thickness is considered. Attention is given to the situation when the surface density of the disk changes on a scale length comparable to its thickness in a gap region, of comparable dimensions, containing the protoplanet. In this case it is necessary to solve for the tidal perturbations taking the surface density structure fully into account. Expressions are developed for the angular momentum exchange rate between protoplanet and disk that require simple numerical calculations only. These calculations are undertaken for simple polytropic models of the disk. The behavior of the tidal perturbation under a wide range of assumptions about dissipation in the disk is considered, and the methods are applied to calculate the strength of the tidal torque in the limit that the protoplanet is sufficiently massive to induce a gap in the nebula.

Associated Articles

Part  1     Part  2     Part  3    

Printing Options

Print whole paper
Print Page(s) through

Return 600 dpi PDF to Acrobat/Browser. Different resolutions (200 or 600 dpi), formats (Postscript, PDF, etc), page sizes (US Letter, European A4, etc), and compression (gzip,compress,none) can be set through the Printing Preferences

More Article Retrieval Options

HELP for Article Retrieval

Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)


Find Similar Abstracts:

Use: Authors
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
arXiv e-prints