Hostname: page-component-7c8c6479df-94d59 Total loading time: 0 Render date: 2024-03-28T10:21:47.012Z Has data issue: false hasContentIssue false

Towards the Albedo of an Exoplanet: MOST Satellite Observations of Bright Transiting Exoplanetary Systems

Published online by Cambridge University Press:  01 May 2008

Jason F. Rowe
Affiliation:
NASA-Ames Research ParkMS-244-30Moffett Field, CA 94035-1000 email: jasonfrowe@gmail.com
Jaymie M. Matthews
Affiliation:
NASA-Ames Research ParkMS-244-30Moffett Field, CA 94035-1000 email: jasonfrowe@gmail.com
Sara Seager
Affiliation:
NASA-Ames Research ParkMS-244-30Moffett Field, CA 94035-1000 email: jasonfrowe@gmail.com
Dimitar Sasselov
Affiliation:
NASA-Ames Research ParkMS-244-30Moffett Field, CA 94035-1000 email: jasonfrowe@gmail.com
Rainer Kuschnig
Affiliation:
NASA-Ames Research ParkMS-244-30Moffett Field, CA 94035-1000 email: jasonfrowe@gmail.com
David B. Guenther
Affiliation:
NASA-Ames Research ParkMS-244-30Moffett Field, CA 94035-1000 email: jasonfrowe@gmail.com
Anthony F. J. Moffat
Affiliation:
NASA-Ames Research ParkMS-244-30Moffett Field, CA 94035-1000 email: jasonfrowe@gmail.com
Slavek M. Rucinski
Affiliation:
NASA-Ames Research ParkMS-244-30Moffett Field, CA 94035-1000 email: jasonfrowe@gmail.com
Gordon A. H. Walker
Affiliation:
NASA-Ames Research ParkMS-244-30Moffett Field, CA 94035-1000 email: jasonfrowe@gmail.com
Werner W. Weiss
Affiliation:
NASA-Ames Research ParkMS-244-30Moffett Field, CA 94035-1000 email: jasonfrowe@gmail.com
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.

The Canadian MOST satellite is a unique platform for observations of bright transiting exoplanetary systems. Providing nearly continuous photometric observations for up to 4 weeks, MOST can produce important observational data to help us learn about the properties of exosolar planets. We review our current observations of HD 209458 and HD 189733 with implications for the albedo and our progress towards detecting reflected light from an exoplanet.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

Ackerman, A. S. & Marley, M. S. 2001, ApJ, 556, 872Google Scholar
Burrows, A., Hubeny, I., Budaj, J., Knutson, H., & Charbonneau, D. 2007, astro-ph/07093980Google Scholar
Cooper, C. S., Sudarsky, D., Milsom, J. A., Lunine, J. I., & Burrows, A. 2003, ApJ, 586, 1320CrossRefGoogle Scholar
Knutson, H. A., Charbonneau, D., Allen, L. E., Burrows, A., & Megeath, S. T. 2008, ApJ, 673, 526CrossRefGoogle Scholar
Marley, M. S., Gelino, C., Stephens, D., Lunine, J. I., & Freedman, R. 1999, ApJ, 513, 879CrossRefGoogle Scholar
Marley, M. S., Fortney, J., Seager, S., & Barman, T. 2006 astro-ph/0602468Google Scholar
Matthews, J. M., Kuschnig, R., Guenther, D. B., Walker, G. A. H., Moffat, A. F. J., Rucinski, S. M., Sasselov, D., & Weiss, W. W. 2004, Nature, 430, 51CrossRefGoogle Scholar
Rowe, J. F., Matthews, J. M., Seager, S., Kuschnig, R., Guenther, D. B., Moffat, A. F. J., Rucinski, S. M., Sasselov, D., Walker, G. A. H., & Weiss, W. W. 2006a, ApJ, 646, 1241Google Scholar
Rowe, J. F., Matthews, J. M., Seager, S., Kuschnig, R., Guenther, D. B., Moffat, A. F. J., Rucinski, S. M., Sasselov, D., Walker, G. A. H., & Weiss, W. W. 2007, ApJ, submittedGoogle Scholar
Russell, H. N. 1916, ApJ, 43, 173CrossRefGoogle Scholar
Walker, G., Matthews, J. M., Kuschnig, R., Johnson, R., Rucinski, S.Pazder, J., Burley, G., Walker, A., Skaret, K., Zee, R., Grocott, S.Carroll, K., Sinclair, P., Sturgeon, D., & Harron, J. 2003, PASP, 115, 1023CrossRefGoogle Scholar