Direct Measure of Radiative and Dynamical Properties of an Exoplanet Atmosphere

Julien de Wit, Nikole K. Lewis, Jonathan Langton, Gregory Laughlin, Drake Deming, Konstantin Batygin, Jonathan J Fortney
(Submitted on 3 Jun 2016)

Two decades after the discovery of 51 Peg b, the formation processes and atmospheres of short-period gas giants remain poorly understood. Observations of eccentric systems provide key insights on those topics as they can illuminate how a planet’s atmosphere responds to changes in incident flux. We report here the analysis of multi-day multi-channel photometry of the eccentric (e~ 0.93) hot Jupiter HD 80606 b obtained with the Spitzer Space Telescope. The planet’s extreme eccentricity combined with the long coverage and exquisite precision of new periastron-passage observations allow us to break the degeneracy between the radiative and dynamical timescales of HD 80606 b’s atmosphere and constrain its global thermal response. Our analysis reveals that the atmospheric layers probed heat rapidly (~4 hr radiative timescale) from <500 to 1400 K as they absorb ~ 20% of the incoming stellar flux during the periastron passage, while the planet’s rotation period is 93±8535 hr, which exceeds the predicted pseudo-synchronous period (40 hr).

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Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Journal reference: ApJL, 820, 2, L33, (2016)
DOI: 10.3847/2041-8205/820/2/L33
Cite as: arXiv:1606.01105 [astro-ph.EP]
(or arXiv:1606.01105v1 [astro-ph.EP] for this version)
Submission history
From: Julien de Wit
[v1] Fri, 3 Jun 2016 14:33:51 GMT (2487kb)
http://arxiv.org/abs/1606.01105