Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-26T07:46:47.753Z Has data issue: false hasContentIssue false

Testing planet formation models with Gaia μas astrometry

Published online by Cambridge University Press:  01 October 2007

A. Sozzetti
Affiliation:
INAF- Astronomical Observatory of Torino, via Osservatorio 20, I-10025, Pino Torinese (TO), Italy email: [email protected] Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
S. Casertano
Affiliation:
Space Telescope Science Institute, San Martin Drive, Baltimore, MD 21218, USA
M. G. Lattanzi
Affiliation:
INAF- Astronomical Observatory of Torino, via Osservatorio 20, I-10025, Pino Torinese (TO), Italy email: [email protected]
A. Spagna
Affiliation:
INAF- Astronomical Observatory of Torino, via Osservatorio 20, I-10025, Pino Torinese (TO), Italy email: [email protected]
R. Morbidelli
Affiliation:
INAF- Astronomical Observatory of Torino, via Osservatorio 20, I-10025, Pino Torinese (TO), Italy email: [email protected]
R. Pannunzio
Affiliation:
INAF- Astronomical Observatory of Torino, via Osservatorio 20, I-10025, Pino Torinese (TO), Italy email: [email protected]
D. Pourbaix
Affiliation:
Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, CP. 226, Boulevard du Triomphe, 1050 Bruxelles, Belgium
D. Queloz
Affiliation:
Observatoire de Genève, 51 Ch. de Maillettes, 1290 Sauveny, Switzerland
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.

In this paper, we first summarize the results of a large-scale double-blind tests campaign carried out for the realistic estimation of the Gaia potential in detecting and measuring planetary systems. Then, we put the identified capabilities in context by highlighting the unique contribution that the Gaia exoplanet discoveries will be able to bring to the science of extrasolar planets during the next decade.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Bean, J. L., et al. 2007, AJ, 134, 749CrossRefGoogle Scholar
Bienaymé, O., Robin, A. C., & Crézé, M. 1987, A&A, 180, 94Google Scholar
Casertano, S., Lattanzi, M. G., Perryman, M. A. C., & Spagna, A. 1996, AP&SS, 241, 89Google Scholar
Lattanzi, M. G., Spagna, A., Sozzetti, A., & Casertano, S. 2000, MNRAS, 317, 211CrossRefGoogle Scholar
Lattanzi, M. G., Casertano, S., Jancart, S., Morbidelli, R., Pannunzio, R., Pourbaix, D., Sozzetti, A., & Spagna, A. 2005, ESA SP-576, 251Google Scholar
Perryman, M. A. C., et al. 2001, A&A, 369, 339Google Scholar
Sozzetti, A., Casertano, S., Lattanzi, M. G., & Spagna, A. 2001, A&A (Letters), 373, L21Google Scholar
Sozzetti, A., Casertano, S., Lattanzi, M. G., & Spagna, A. 2003, ESA SP-539, 605Google Scholar
Sozzetti, A. 2005, PASP, 117, 1021CrossRefGoogle Scholar
Tabachnik, S., & Tremaine, S. 2002, MNRAS, 335, 151CrossRefGoogle Scholar