Hostname: page-component-8448b6f56d-cfpbc Total loading time: 0 Render date: 2024-04-16T06:16:44.701Z Has data issue: false hasContentIssue false
  • English
  • Français

Planet masses and radii from physical principles

Published online by Cambridge University Press:  10 November 2011

Guenther Wuchterl
Guenther Wuchterl*
Affiliation:
Thüringer Landessternwarte, D-07778 Tautenburg, Germany email: gwuchterl@tls-tautenburg.de
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Masses 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.

Keywords

planetary systems: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S276: The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution , October 2010 , pp. 76 - 81
Copyright
Copyright © International Astronomical Union 2011

References

Broeg, C. 2006, Ph.D. thesis, Friedrich-Schiller-Universität Jena, Germany. http://www.db-thueringen.de/servlets/DocumentServlet?id=6619Google Scholar
Broeg, C. 2007a, Mass spectra corot mark 2a. Http://www.space.unibe.ch/~broeg, http://www.space.unibe.ch/~broegGoogle Scholar
Broeg, C. 2007b, MNRAS, 377, L44CrossRefGoogle Scholar
Broeg, C. H. 2009, Icarus, 204, 15CrossRefGoogle Scholar
Cabrera, J., Bruntt, H., Ollivier, M., et al. 2010, A&A, 522, A110+Google Scholar
Lammer, H., Penz, T., Wuchterl, G., et al. 2007, ArXiv Astrophysics e-prints. arXiv:astro-ph/0701565Google Scholar
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.pdfGoogle Scholar
Pečnik, B. & Wuchterl, G. 2005, A&A, 440, 1183Google Scholar
Pečnik, B. 2003, Master's thesis, University of Zagreb, CroatiaGoogle Scholar
Schönke, J. 2005, Diploma Thesis, AIU-JenaGoogle Scholar
Schönke, J. 2007, Plan. & Sp. Sci., 55, 1299CrossRefGoogle Scholar
Wuchterl, G. 1993, Icarus, 106, 323CrossRefGoogle Scholar
Wuchterl, G. 1995, Earth, Moon and Planets, 67, 51CrossRefGoogle Scholar
Wuchterl, G., Broeg, C., Krause, S., et al. 2007, arXiv:astro-ph/0701003Google Scholar
Wuchterl, G., Guillot, T., & Lissauer, J. J. 2000, Protostars and Planets IV, 1081Google Scholar