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HST hot-Jupiter transmission spectral survey: Clear skies for cool Saturn WASP-39b

Abstract:
We present the Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS) optical transmission spectroscopy of the cool Saturn-mass exoplanet WASP-39b from 0.29-1.025 μm, along with complementary transit observations from Spitzer IRAC at 3.6 and 4.5 μm. The low density and large atmospheric pressure scale height of WASP-39b make it particularly amenable to atmospheric characterization using this technique. We detect a Rayleigh scattering slope as well as sodium and potassium absorption features; this is the first exoplanet in which both alkali features are clearly detected with the extended wings predicted by cloud-free atmosphere models. The full transmission spectrum is well matched by a clear H 2 -dominated atmosphere, or one containing a weak contribution from haze, in good agreement with the preliminary reduction of these data presented in Sing et al. WASP-39b is predicted to have a pressure-temperature profile comparable to that of HD 189733b and WASP-6b, making it one of the coolest transiting gas giants observed in our HST STIS survey. Despite this similarity, WASP-39b appears to be largely cloud-free, while the transmission spectra of HD 189733b and WASP-6b both indicate the presence of high altitude clouds or hazes. These observations further emphasize the surprising diversity of cloudy and cloud-free gas giant planets in short-period orbits and the corresponding challenges associated with developing predictive cloud models for these atmospheres.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/0004-637X/827/1/19

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Role:
Author
ORCID:
0000-0002-1321-2139
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Role:
Author
ORCID:
0000-0003-4155-8513


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Grant:
HST-GO-12473
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Grant:
FP7/2007-2013/ERC grant agreement no. 336792


Publisher:
IOP Publishing
Journal:
Astrophysical Journal More from this journal
Volume:
827
Issue:
1
Article number:
19
Publication date:
2016-08-03
Acceptance date:
2016-06-01
DOI:
EISSN:
1538-4357
ISSN:
0004-637X


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Pubs id:
pubs:598292
UUID:
uuid:92b2f6be-4c7a-4fba-846f-2772d63bd060
Local pid:
pubs:598292
Source identifiers:
598292
Deposit date:
2018-01-23

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