Hostname: page-component-cc8bf7c57-77pjf Total loading time: 0 Render date: 2024-12-12T06:35:55.709Z Has data issue: false hasContentIssue false
  • English
  • Français

What Photometric Space Telescopes Can Tell Us About Extrasolar Giant Planets

Published online by Cambridge University Press:  26 May 2016

S. Seager  and
Lam Hui
S. Seager
Affiliation:
Institute for Advanced Study, Einstein Dr., Princeton, NJ 08540, USA
Lam Hui
Affiliation:
Department of Physics, Columbia University, 538 West 120th St., New York, NY 10027, USA

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.

Within the next few years three microsatellites with part-per-million photometric capability (MOST, MONS, COROT) will be launched. These space telescopes, which were designed for asteroseismology, as well as other proposed or planned space telescopes to detect Earth-like transiting planets (Kepler and Eddington), will be able to observe the reflected light curves of the close-in extrasolar giant planets (CEGPs). The CEGPs are 0.05 AU from their parent star and are potentially bright in reflected light. For a transiting planet (at any orbital distance) moons and planetary rings may be detected.

Type
Part V: Discovery and study of extrasolar planets - future
Information
Symposium - International Astronomical Union , Volume 202: Planetary Systems in the Universe – Observation, Formation and Evolution , 2004 , pp. 468 - 470
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Charbonneau, D., Brown, T. M., Gilliland, R. L., Noyes, R. W., & Burrows, A. 2000, in ASP Conf. Ser. xx, Planetary Systems in the Universe, ed. Penny, A.J., Artymowicz, P., Lagrange, A.-M., & Russell, S.S., (San Francisco: ASP), in press.Google Scholar
Sartoretti, P., & Schneider, J. 1998, A&AS, 134, 553.Google Scholar
Seager, S., Whitney, B. A., & Sasselov, D. D. 2000, ApJ, 540, 504.CrossRefGoogle Scholar