[en] We present the first high-precision photometry of the transiting extrasolar planetary system WASP-7, obtained using telescope defocussing techniques and reaching a scatter of 0.68 mmag per point. We find that the transit depth is greater and that the host star is more evolved than previously thought. The planet has a significantly larger radius (1.330 +/- 0.093 Rjup versus 0.915 +0.046 -0.040 Rjup) and much lower density (0.41 +/- 0.10 rhojup versus 1.26 +0.25 -0.21 rhojup) and surface gravity (13.4 +/- 2.6 m/s2 versus 26.4 +4.4 -4.0 m/s2) than previous measurements showed. Based on the revised properties it is no longer an outlier in planetary mass--radius and period--gravity diagrams. We also obtain a more precise transit ephemeris for the WASP-7 system.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Southworth, J.
Dominik, M.
Jorgensen, U~G
Rahvar, S.
Snodgrass, C.
Alsubai, K.
Bozza, V.
Browne, P.
Burgdorf, M.
Calchi Novati, S.
Dodds, P.
Dreizler, S.
Finet, François ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)
Gerner, T.
Hardis, S.
Harpsoe, K.
Hellier, C.
Hinse, T~C
Hundertmark, M.
Kains, N.
Kerins, E.
Liebig, C.
Mancini, L.
Mathiasen, M.
Penny, M~T
Proft, S.
Ricci, Davide ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)
Sahu, K.
Scarpetta, G.
Schafer, S.
Schonebeck, F.
Surdej, Jean ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)
scite shows how a scientific paper has been cited by providing the context of the citation, a classification describing whether it supports, mentions, or contrasts the cited claim, and a label indicating in which section the citation was made.
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