Spin-orbit misalignment in the HD 80606 planetary system

DSpace/Manakin Repository

Open Research Exeter (ORE)

Spin-orbit misalignment in the HD 80606 planetary system

Please use this identifier to cite or link to this item: http://hdl.handle.net/10036/87370

Share:                 



Title: Spin-orbit misalignment in the HD 80606 planetary system
Author: Pont, F.
Hébrard, G.
Irwin, J. M.
Bouchy, F.
Moutou, C.
Ehrenreich, D.
Guillot, T.
Aigrain, Suzanne
Bonfils, X.
Berta, Z.
Boisse, I.
Burke, C.
Charbonneau, D.
Delfosse, X.
Desort, M.
Eggenberger, A.
Forveille, T.
Lagrange, A.-M.
Lovis, C.
Nutzman, P.
Pepe, F.
Perrier, C.
Queloz, D.
Santos, N. C.
Ségransan, D.
Udry, S.
Vidal-Madjar, A.
Citation: 502 (2), pp. 695-703
Publisher: EDP Sciences
Journal: Astronomy and Astrophysics
Date Issued: 2009
URI: http://hdl.handle.net/10036/87370
DOI: 10.1051/0004-6361/200912463
Links: http://dx.doi.org/10.1051/0004-6361/200912463
Abstract: We recently reported the photometric and spectroscopic detection of the primary transit of the 111-day-period, eccentric extra-solar planet HD80606b, at Observatoire de Haute-Provence, France. The whole egress of the primary transit and a section of its central part were observed, allowing the measurement of the planetary radius, and evidence for a spin-orbit misalignment through the observation of the Rossiter-McLaughlin anomaly. The ingress not having been observed for this long-duration transit, uncertainties remained in the parameters of the system. We present here a refined, combined analysis of our photometric and spectroscopic data, together with further published radial velocities, ground-based photometry, and Spitzer photometry around the secondary eclipse, as well as new photometric measurements of HD80606 acquired at Mount Hopkins, Arizona, just before the beginning of the primary transit. Although the transit is not detected in those new data, they provide an upper limit for the transit duration, which narrows down the possible behaviour of the Rossiter-McLaughlin anomaly in the unobserved part of the transit. We analyse the whole data with a Bayesian approach using a Markov-chain Monte Carlo integration on all available information. We find Rp = 0.98 ± 0.03 RJup for the planetary radius, and a total primary transit duration of 11.9±1.3 h from first to fourth contact. Our analysis reinforces the hypothesis of spin-orbit misalignment in this system (alignment excluded at >95% level), with a positive projected angle between the planetary orbital axis and the stellar rotation (median solution λ ∼ 50◦). As HD80606 is a component of a binary system, the peculiar orbit of its planet could result from a Kozai mechanism.
Type: Article
Description: Copyright © The European Southern Observatory (ESO)
Keywords: planetary systems
ISSN: 0004-63611432-0746


Please note: Before reusing this item please check the rights under which it has been made available. Some items are restricted to non-commercial use. Please cite the published version where applicable.

Files in this item

Files Size Format View
Spin-orbit misalignment in the HD80606.pdf 1.246Mb PDF Thumbnail

This item appears in the following Collection(s)

Browse

My Account

Local Links