Planet masses and radii from physical principles-Reference-Cited by-同舟云学术

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Planet masses and radii from physical principles

Published:2010-10 Issue:S276 Volume:6 Page:76-81
ISSN:1743-9213
Container-title:Proceedings of the International Astronomical Union
language:en
Short-container-title:Proc. IAU

Author:

Wuchterl Guenther

Abstract

AbstractMasses and radii are the primary observables to characterize exoplanets today. A self-consistent theoretical approach is presented that allows to calculate mass- and radius-distributions of exoplanet populations from basic physical principles and avoids the usual parametrisation of a multitude of processes.

Publisher

Cambridge University Press (CUP)

Subject

Astronomy and Astrophysics,Space and Planetary Science

Reference15 articles.

1. Pečnik B. 2005, Ph.D. thesis, Ludwig-Maximillians-Universität München, Germany. http://edoc.ub.uni-muenchen.de/archive/00005023/01/Pecnik_Bojan.pdf, http://www.znanost.org/~bonnie/work/Thesis.pdf

2. Broeg C. 2007a, Mass spectra corot mark 2a. Http://www.space.unibe.ch/~broeg, http://www.space.unibe.ch/~broeg

3. Lammer H. , Penz T. , Wuchterl G. , 2007, ArXiv Astrophysics e-prints. arXiv:astro-ph/0701565

4. Hydrostatic, isothermal planetary models from the point of view of dynamical systems: “Determination of explicit formulas for the point of critical mass”

5. Wuchterl G. , Guillot T. , & Lissauer J. J. 2000, Protostars and Planets IV, 1081

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