Astrophysics, abstract
astro-ph/0603291

From: Gaspar Bakos A [view email]

Date: Sun, 12 Mar 2006 22:36:03 GMT (117kb)

Refined parameters of the planet orbiting HD 189733

Authors: G. A. Bakos (1,2), H. Knutson (1), F. Pont (5), C. Moutou (3), D. Charbonneau (1), A. Shporer (8), F. Bouchy (4,10), M. Everett (6), C. Hergenrother (7), D. W. Latham (1), M. Mayor (5), T. Mazeh (8), R. W. Noyes (1), D. Queloz (5), A. Pal (9,1), S. Udry (5) ((1) Harvard-Smithsonian Center for Astrophysics, (2) Hubble Fellow, (3) Laboratoire d'Astrophysique de Marseille, (4) Observatoire de Haute Provence, (5) Observatoire de Geneve, (6) Planetary Science Institute, (7) Dep. of Planetary Sciences and Lunar and Planetary Laboratory, UofA, (8) Wise Observatory, Tel Aviv University, (9) Eotvos Lorand University, Department of Astronomy, (10) Institut d'Astrophysique de Paris)

Comments: 10 pages, 4 figures, submitted to ApJ

We report on the BVRI multi-band follow-up photometry of the transiting extrasolar planet HD 189733b. We revise the transit parameters and find planetary radius RP = 1.154+/- 0.032RJ and inclination i_P = 85.79+/-0.24deg. The new density (~ 1g cm-3) is significantly higher than the former estimate (~ 0.75g cm-3); this shows that from the current sample of 9 transiting planets, only HD 209458 (and possibly OGLE-10b) have anomalously large radii and low densities. We note that due to the proximity of the parent star, HD 189733b currently has one of the most precise radius determinations among extrasolar planets. We calculate new ephemerides: P = 2.218573+/-0.000020 days, T0 = 2453629.39420+/-0.00024 (HJD), and estimate the timing offsets of the 11 distinct transits with respect to the predictions of a constant orbital period, which can be used to reveal the presence of additional planets in the system.

http://fr.arxiv.org/abs/astro-ph/0603291