Detection of period variations in extrasolar transiting planet ogle-TR-111b
Two consecutive transits of planetary companion OGLE-TR-111b were observed in the I band. Combining these observations with data from the literature, we find that the timing of the transits cannot be explained by a constant period and that the observed variations cannot be originated by the presence...
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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v682_n1PART2_pL49_Diaz |
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todo:paper_0004637X_v682_n1PART2_pL49_Diaz2023-10-03T14:02:09Z Detection of period variations in extrasolar transiting planet ogle-TR-111b Diáz, R.F. Rojo, P. Melita, M. Hoyer, S. Minniti, D. Mauas, P.J.D. Ruíz, M.T. Planetary systems stars: individual (OGLE-TR-111) Two consecutive transits of planetary companion OGLE-TR-111b were observed in the I band. Combining these observations with data from the literature, we find that the timing of the transits cannot be explained by a constant period and that the observed variations cannot be originated by the presence of a satellite. However, a perturbing planet with the mass of the Earth in an exterior orbit could explain the observations if the orbit of OGLE-TR-111b is eccentric. We also show that the eccentricity needed to explain the observations is not ruled out by the radial velocity data found in the literature. © 2008. The American Astronomical Society. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0004637X_v682_n1PART2_pL49_Diaz |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Planetary systems stars: individual (OGLE-TR-111) |
spellingShingle |
Planetary systems stars: individual (OGLE-TR-111) Diáz, R.F. Rojo, P. Melita, M. Hoyer, S. Minniti, D. Mauas, P.J.D. Ruíz, M.T. Detection of period variations in extrasolar transiting planet ogle-TR-111b |
topic_facet |
Planetary systems stars: individual (OGLE-TR-111) |
description |
Two consecutive transits of planetary companion OGLE-TR-111b were observed in the I band. Combining these observations with data from the literature, we find that the timing of the transits cannot be explained by a constant period and that the observed variations cannot be originated by the presence of a satellite. However, a perturbing planet with the mass of the Earth in an exterior orbit could explain the observations if the orbit of OGLE-TR-111b is eccentric. We also show that the eccentricity needed to explain the observations is not ruled out by the radial velocity data found in the literature. © 2008. The American Astronomical Society. |
format |
JOUR |
author |
Diáz, R.F. Rojo, P. Melita, M. Hoyer, S. Minniti, D. Mauas, P.J.D. Ruíz, M.T. |
author_facet |
Diáz, R.F. Rojo, P. Melita, M. Hoyer, S. Minniti, D. Mauas, P.J.D. Ruíz, M.T. |
author_sort |
Diáz, R.F. |
title |
Detection of period variations in extrasolar transiting planet ogle-TR-111b |
title_short |
Detection of period variations in extrasolar transiting planet ogle-TR-111b |
title_full |
Detection of period variations in extrasolar transiting planet ogle-TR-111b |
title_fullStr |
Detection of period variations in extrasolar transiting planet ogle-TR-111b |
title_full_unstemmed |
Detection of period variations in extrasolar transiting planet ogle-TR-111b |
title_sort |
detection of period variations in extrasolar transiting planet ogle-tr-111b |
url |
http://hdl.handle.net/20.500.12110/paper_0004637X_v682_n1PART2_pL49_Diaz |
work_keys_str_mv |
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1807314519602495488 |