دورية أكاديمية

A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067

التفاصيل البيبلوغرافية
العنوان: A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067
المؤلفون: Luque, R., Osborn, H. P., Leleu, A., Pallé, E., Bonfanti, A., Barragán, O., Wilson, T. G., Broeg, C., Cameron, A. Collier, Lendl, M., Maxted, P. F. L., Alibert, Y., Gandolfi, D., Delisle, J. -B., Hooton, M. J., Egger, J. A., Nowak, G., Lafarga, M., Rapetti, D., Twicken, J. D., Morales, J. C., Carleo, I., Orell-Miquel, J., Adibekyan, V., Alonso, R., Alqasim, A., Amado, P. J., Anderson, D. R., Anglada-Escudé, G., Bandy, T., Bárczy, T., Barrado Navascues, D., Barros, S. C. C., Baumjohann, W., Bayliss, D., Bean, J. L., Beck, M., Beck, T., Benz, W., Billot, N., Bonfils, X., Borsato, L., Boyle, A. W., Brandeker, A., Bryant, E. M., Cabrera, J., Carrazco-Gaxiola, S., Charbonneau, D., Charnoz, S., Ciardi, D. R., Cochran, W. D., Collins, K. A., Crossfield, I. J. M., Csizmadia, Sz., Cubillos, P. E., Dai, F., Davies, M. B., Deeg, H. J., Deleuil, M., Deline, A., Delrez, L., Demangeon, O. D. S., Demory, B. -O., Ehrenreich, D., Erikson, A., Esparza-Borges, E., Falk, B., Fortier, A., Fossati, L., Fridlund, M., Fukui, A., Garcia-Mejia, J., Gill, S., Gillon, M., Goffo, E., Gómez Maqueo Chew, Y., Güdel, M., Guenther, E. W., Günther, M. N., Hatzes, A. P., Helling, Ch., Hesse, K. M., Howell, S. B., Hoyer, S., Ikuta, K., Isaak, K. G., Jenkins, J. M., Kagetani, T., Kiss, L. L., Kodama, T., Korth, J., Lam, K. W. F., Laskar, J., Latham, D. W., Lecavelier des Etangs, A., Leon, J. P. D., Livingston, J. H., Magrin, D., Matson, R. A., Matthews, E. C., Mordasini, C., Mori, M., Moyano, M., Munari, M., Murgas, F., Narita, N., Nascimbeni, V., Olofsson, G., Osborne, H. L. M., Ottensamer, R., Pagano, I., Parviainen, H., Peter, G., Piotto, G., Pollacco, D., Queloz, D., Quinn, S. N., Quirrenbach, A., Ragazzoni, R., Rando, N., Ratti, F., Rauer, H., Redfield, S., Ribas, I., Ricker, G. R., Rudat, A., Sabin, L., Salmon, S., Santos, N. C., Scandariato, G., Schanche, N., Schlieder, J. E., Seager, S., Ségransan, D., Shporer, A., Simon, A. E., Smith, A. M. S., Sousa, S. G., Stalport, M., Szabó, Gy. M., Thomas, N., Tuson, A., Udry, S., Vanderburg, A. M., van Eylen, V., van Grootel, V., Venturini, J., Walter, I., Walton, N. A., Watanabe, N., Winn, J. N., Zingales, T.
المساهمون: Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, Institut de Physique du Globe de Paris (IPGP (UMR_7154)), Institut national des sciences de l'Univers (INSU - CNRS)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
المصدر: ISSN: 0028-0836.
بيانات النشر: HAL CCSD
Nature Publishing Group
سنة النشر: 2023
المجموعة: Archive de l'Observatoire de Paris (HAL)
مصطلحات موضوعية: Astrophysics - Earth and Planetary Astrophysics, [SDU]Sciences of the Universe [physics]
الوصف: International audience ; Planets with radii between that of the Earth and Neptune (hereafter referred to as `sub-Neptunes') are found in close-in orbits around more than half of all Sun-like stars 1,2 . However, their composition, formation and evolution remain poorly understood 3 . The study of multiplanetary systems offers an opportunity to investigate the outcomes of planet formation and evolution while controlling for initial conditions and environment. Those in resonance (with their orbital periods related by a ratio of small integers) are particularly valuable because they imply a system architecture practically unchanged since its birth. Here we present the observations of six transiting planets around the bright nearby star HD 110067. We find that the planets follow a chain of resonant orbits. A dynamical study of the innermost planet triplet allowed the prediction and later confirmation of the orbits of the rest of the planets in the system. The six planets are found to be sub-Neptunes with radii ranging from 1.94R ⊕ to 2.85R ⊕ . Three of the planets have measured masses, yielding low bulk densities that suggest the presence of large hydrogen-dominated atmospheres.
نوع الوثيقة: article in journal/newspaper
اللغة: English
العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/2311.17775; insu-04462244; https://insu.hal.science/insu-04462244Test; ARXIV: 2311.17775; BIBCODE: 2023Natur.623.932L
DOI: 10.1038/s41586-023-06692-3
الإتاحة: https://doi.org/10.1038/s41586-023-06692-3Test
https://insu.hal.science/insu-04462244Test
رقم الانضمام: edsbas.172A46D2
قاعدة البيانات: BASE