A much lower density for the transiting extrasolar planet WASP-7

March 2011 • 2011A&A...527A...8S

Authors • Southworth, J. • Dominik, M. • Jørgensen, U. G. • Rahvar, S. • Snodgrass, C. • Alsubai, K. • Bozza, V. • Browne, P. • Burgdorf, M. • Calchi Novati, S. • Dodds, P. • Dreizler, S. • Finet, F. • Gerner, T. • Hardis, S. • Harpsøe, K. • Hellier, C. • Hinse, T. C. • Hundertmark, M. • Kains, N. • Kerins, E. • Liebig, C. • Mancini, L. • Mathiasen, M. • Penny, M. T. • Proft, S. • Ricci, D. • Sahu, K. • Scarpetta, G. • Schäfer, S. • Schönebeck, F. • Surdej, J.

Abstract • 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 R_Jup versus ; R_Jup) and much lower density (0.41 ± 0.10 ρ_Jup versus ; ρ_Jup) and surface gravity (13.4 ± 2.6 m s^-2 versus ; m s^-2) 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.

Based on data collected by MiNDSTEp with the Danish 1.54 m telescope at the ESO La Silla Observatory.Lightcurves data is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/527/A8

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Sebastiano Calchi Novati

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