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Metals in the Exosphere of the Highly Irradiated Planet WASP-12b

Fossati, L.; Haswell, C. A.; Froning, C. S.; Hebb, L.; Holmes, S.; Kolb, U.; Helling, Ch.; Carter, A.; Wheatley, P.; Cameron, A. C.; Loeillet, B.; Pollacco, D.; Street, R.; Stempels, H. C.; Simpson, E.; Udry, S.; Joshi, Y. C.; West, R. G.; Skillen, I. and Wilson, D. (2010). Metals in the Exosphere of the Highly Irradiated Planet WASP-12b. Astrophysical Journal Letters, 714(2) L222.

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DOI (Digital Object Identifier) Link: http://dx.doi.org/10.1088/2041-8205/714/2/L222
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Abstract

We present near-UV transmission spectroscopy of the highly irradiated transiting exoplanet WASP-12b, obtained with the Cosmic Origins Spectrograph on the Hubble Space Telescope. The spectra cover three distinct wavelength ranges: NUVA (2539-2580 Å), NUVB (2655-2696 Å), and NUVC (2770-2811 Å). Three independent methods all reveal enhanced transit depths attributable to absorption by resonance lines of metals in the exosphere of WASP-12b. Light curves of total counts in the NUVA and NUVC wavelength ranges show a detection at a 2.5? level. We detect extra absorption in the Mg II ??2800 resonance line cores at the 2.8? level. The NUVA, NUVB, and NUVC light curves imply effective radii of 2.69 ± 0.24 R J , 2.18 ± 0.18 R J , and 2.66 ± 0.22 R J respectively, suggesting the planet is surrounded by an absorbing cloud which overfills the Roche lobe. We detect enhanced transit depths at the wavelengths of resonance lines of neutral sodium, tin, and manganese, and at singly ionized ytterbium, scandium, manganese, aluminum, vanadium, and magnesium. We also find the statistically expected number of anomalous transit depths at wavelengths not associated with any known resonance line. Our data are limited by photon noise, but taken as a whole the results are strong evidence for an extended absorbing exosphere surrounding the planet. The NUVA data exhibit an early ingress, contrary to model expectations; we speculate this could be due to the presence of a disk of previously stripped material.

Item Type: Journal Article
Copyright Holders: 2010 IOP Publishing
ISSN: 2041-8213
Academic Unit/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
eSTEeM
Item ID: 21403
Depositing User: Users 9 not found.
Date Deposited: 25 May 2010 09:24
Last Modified: 11 Mar 2014 18:44
URI: http://oro.open.ac.uk/id/eprint/21403
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