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

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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
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S253: Transiting Planets , May 2008 , pp. 121 - 127
Copyright
Copyright © International Astronomical Union 2009

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