Article (Scientific journals)
Spitzer Secondary Eclipses of WASP-18b
Nymeyer, Sarah; Harrington, Joseph; Hardy, Ryan A et al.
2011In Astrophysical Journal, 742 (1), p. 35
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Keywords :
Astrophysics - Earth and Planetary Astrophysics
Abstract :
[en] The transiting exoplanet WASP-18b was discovered in 2008 by the Wide Angle Search for Planets (WASP) project. The Spitzer Exoplanet Target of Opportunity Program observed secondary eclipses of WASP-18b using Spitzer's Infrared Array Camera (IRAC) in the 3.6-micron and 5.8-micron bands on 2008 December 20, and in the 4.5-micron and 8.0-micron bands on 2008 December 24. We report eclipse depths of 0.31+-0.02, 0.38+-0.03, 0.41+-0.02, 0.43+-0.03 %, and brightness temperatures of 2920 +- 90, 3150 +- 130, 3040 +- 130 and 2960 +- 130 K, respectively. WASP-18b is one of the hottest planets yet discovered - as hot as an M-class star. The planet's pressure-temperature profile features a thermal inversion. The observations also require WASP-18b to have near-zero albedo and almost no redistribution of energy from the day-side to the night side of the planet.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Nymeyer, Sarah
Harrington, Joseph
Hardy, Ryan A
Stevenson, Kevin B
Campo, Christopher J
Madhusudhan, Nikku
Collier-Cameron, Andrew
Blecic, Jasmina
Bowman, William C
Britt, Christopher B T
Cubillos, Patricio
Hellier, Coel
Gillon, Michaël  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique et traitement de l'image
Maxted, Pierre F L
Hebb, Leslie
Wheatley, Peter J
Pollacco, Don
Anderson, David
More authors (8 more) Less
Language :
English
Title :
Spitzer Secondary Eclipses of WASP-18b
Publication date :
01 November 2011
Journal title :
Astrophysical Journal
ISSN :
0004-637X
eISSN :
1538-4357
Publisher :
University of Chicago Press, Chicago, United States - Illinois
Volume :
742
Issue :
1
Pages :
35
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
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