CaltechAUTHORS
  A Caltech Library Service

A map of the day–night contrast of the extrasolar planet HD 189733b

Knutson, Heather A. and Charbonneau, David and Allen, Lori E. and Fortney, Jonathan J. and Agol, Eric and Cowan, Nicolas B. and Showman, Adam P. and Cooper, Curtis S. and Megeath, S. Thomas (2007) A map of the day–night contrast of the extrasolar planet HD 189733b. Nature, 447 (7141). pp. 183-186. ISSN 0028-0836. https://resolver.caltech.edu/CaltechAUTHORS:20130128-154306263

[img] PDF - Accepted Version
See Usage Policy.

229Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20130128-154306263

Abstract

'Hot Jupiter' extrasolar planets are expected to be tidally locked because they are close (<0.05 astronomical units, where 1 au is the average Sun–Earth distance) to their parent stars, resulting in permanent daysides and nightsides. By observing systems where the planet and star periodically eclipse each other, several groups have been able to estimate the temperatures of the daysides of these planets. A key question is whether the atmosphere is able to transport the energy incident upon the dayside to the nightside, which will determine the temperature at different points on the planet's surface. Here we report observations of HD 189733, the closest of these eclipsing planetary systems, over half an orbital period, from which we can construct a 'map' of the distribution of temperatures. We detected the increase in brightness as the dayside of the planet rotated into view. We estimate a minimum brightness temperature of 973 ± 33 K and a maximum brightness temperature of 1,212 ± 11 K at a wavelength of 8 mum, indicating that energy from the irradiated dayside is efficiently redistributed throughout the atmosphere, in contrast to a recent claim for another hot Jupiter. Our data indicate that the peak hemisphere-integrated brightness occurs 16 ± 6° before opposition, corresponding to a hotspot shifted east of the substellar point. The secondary eclipse (when the planet moves behind the star) occurs 120 ± 24 s later than predicted, which may indicate a slightly eccentric orbit.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1038/nature05782DOIArticle
https://rdcu.be/bDxg5PublisherFree ReadCube access
https://arxiv.org/abs/0705.0993arXivDiscussion Paper
ORCID:
AuthorORCID
Knutson, Heather A.0000-0002-0822-3095
Charbonneau, David0000-0002-9003-484X
Fortney, Jonathan J.0000-0002-9843-4354
Agol, Eric0000-0002-0802-9145
Cowan, Nicolas B.0000-0001-6129-5699
Megeath, S. Thomas0000-0001-7629-3573
Additional Information:© 2007 Nature Publishing Group, a division of Macmillan Publishers Limited. Received 8 February; accepted 23 March 2007. We thank J. Winn for sharing data from a recent paper describing the behaviour of the spots on the star, and D. Sasselov and E. Miller-Ricci for discussions on the properties of these spots. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract to NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech. We are grateful to the entire Spitzer team for their assistance throughout this process. H.A.K. was supported by a National Science Foundation Graduate Research Fellowship.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASA/JPL/CaltechUNSPECIFIED
NSF Graduate Research FellowshipUNSPECIFIED
Issue or Number:7141
Record Number:CaltechAUTHORS:20130128-154306263
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130128-154306263
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:36636
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:29 Jan 2013 00:13
Last Modified:03 Oct 2019 04:39

Repository Staff Only: item control page