A Radial Velocity Study of the Planetary System of π Mensae: Improved Planet Parameters for π Mensae c and a Third Planet on a 125 Day Orbit
dc.contributor.author | Hatzes, Artie P. | |
dc.contributor.author | Gandolfi, Davide | |
dc.contributor.author | Korth, Judith | |
dc.contributor.author | Rodler, Florian | |
dc.contributor.author | Sabotta, Silvia | |
dc.contributor.author | Esposito, Massimiliano | |
dc.contributor.author | Barragán, Oscar | |
dc.contributor.author | Van Eylen, Vincent | |
dc.contributor.author | Livingston, John H. | |
dc.contributor.author | Serrano, Luisa Maria | |
dc.contributor.author | Luque, Rafael | |
dc.contributor.author | Smith, Alexis M. S. | |
dc.contributor.author | Redfield, Seth | |
dc.contributor.author | Persson, Carina M. | |
dc.contributor.author | Pätzold, Martin | |
dc.contributor.author | Palle, Enric | |
dc.contributor.author | Nowak, Grzegorz | |
dc.contributor.author | Osborne, Hannah L. M. | |
dc.contributor.author | Narita, Norio | |
dc.contributor.author | Mathur, Savita | |
dc.contributor.author | Lam, Kristine W. F. | |
dc.contributor.author | Kabáth, Petr | |
dc.contributor.author | Johnson, Marshall C. | |
dc.contributor.author | Guenther, Eike W. | |
dc.contributor.author | Grziwa, Sascha | |
dc.contributor.author | Goffo, Elisa | |
dc.contributor.author | Fridlund, Malcolm | |
dc.contributor.author | Endl, Michael | |
dc.contributor.author | Deeg, Hans J. | |
dc.contributor.author | Csizmadia, Szilard | |
dc.contributor.author | Cochran, William D. | |
dc.contributor.author | Cuesta, Lucía González | |
dc.contributor.author | Chaturvedi, Priyanka | |
dc.contributor.author | Carleo, Ilaria | |
dc.contributor.author | Cabrera, Juan | |
dc.contributor.author | Beck, Paul G. | |
dc.contributor.author | Albrecht, Simon | |
dc.date.accessioned | 2022-05-10T10:51:19Z | |
dc.date.available | 2022-05-10T10:51:19Z | |
dc.date.issued | 2022-04-20 | |
dc.date.updated | 2022-04-29T15:48:03Z | |
dc.description.abstract | π Men hosts a transiting planet detected by the Transiting Exoplanet Survey Satellite space mission and an outer planet in a 5.7 yr orbit discovered by radial velocity (RV) surveys. We studied this system using new RV measurements taken with the HARPS spectrograph on ESO’s 3.6 m telescope, as well as archival data. We constrain the stellar RV semiamplitude due to the transiting planet, π Men c, as Kc = 1.21 ± 0.12 m s−1, resulting in a planet mass of Mc = 3.63 ± 0.38 M⊕. A planet radius of Rc = 2.145 ± 0.015 R⊕ yields a bulk density of ρc = 2.03 ± 0.22 g cm−3. The precisely determined density of this planet and the brightness of the host star make π Men c an excellent laboratory for internal structure and atmospheric characterization studies. Our HARPS RV measurements also reveal compelling evidence for a third body, π Men d, with a minimum mass Md sin id = 13.38 ± 1.35 M⊕ orbiting with a period of Porb,d = 125 days on an eccentric orbit (ed = 0.22). A simple dynamical analysis indicates that the orbit of π Men d is stable on timescales of at least 20 Myr. Given the mutual inclination between the outer gaseous giant and the inner rocky planet and the presence of a third body at 125 days, π Men is an important planetary system for dynamical and formation studies. | en |
dc.description.sponsorship | DFG, 313698196, SPP 1992: Exploration der Diversität extrasolarer Planeten | en |
dc.identifier.eissn | 1538-3881 | |
dc.identifier.issn | 0004-6256 | |
dc.identifier.uri | https://depositonce.tu-berlin.de/handle/11303/16840 | |
dc.identifier.uri | http://dx.doi.org/10.14279/depositonce-15618 | |
dc.language.iso | en | en |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | en |
dc.subject.ddc | 520 Astronomie und zugeordnete Wissenschaften | de |
dc.subject.other | radial velocity | en |
dc.subject.other | planetary system | en |
dc.subject.other | π Mensae | en |
dc.subject.other | Transiting Exoplanet Survey Satellite | en |
dc.subject.other | telescope | en |
dc.title | A Radial Velocity Study of the Planetary System of π Mensae: Improved Planet Parameters for π Mensae c and a Third Planet on a 125 Day Orbit | en |
dc.type | Article | en |
dc.type.version | publishedVersion | en |
dcterms.bibliographicCitation.articlenumber | 223 | en |
dcterms.bibliographicCitation.doi | 10.3847/1538-3881/ac5dcb | en |
dcterms.bibliographicCitation.issue | 5 | en |
dcterms.bibliographicCitation.journaltitle | The Astronomical Journal | en |
dcterms.bibliographicCitation.originalpublishername | IOP | en |
dcterms.bibliographicCitation.originalpublisherplace | Bristol | en |
dcterms.bibliographicCitation.volume | 163 | en |
tub.accessrights.dnb | free | en |
tub.affiliation | Fak. 2 Mathematik und Naturwissenschaften::Zentrum für Astronomie und Astrophysik | de |
tub.affiliation.faculty | Fak. 2 Mathematik und Naturwissenschaften | de |
tub.affiliation.institute | Zentrum für Astronomie und Astrophysik | de |
tub.publisher.universityorinstitution | Technische Universität Berlin | en |