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Two temperate earth-mass planets orbiting the nearby star GJ 1002

Authors :
Ministerio de Ciencia e Innovación (España)
European Commission
Ministerio de Ciencia, Innovación y Universidades (España)
Agencia Estatal de Investigación (España)
Consejo Superior de Investigaciones Científicas (España)
Fundação para a Ciência e a Tecnologia (Portugal)
Junta de Andalucía
Swiss National Science Foundation
Gobierno de Canarias
Suárez Mascareño, A.
González-Álvarez, E.
Zapatero Osorio, María Rosa
Lillo-Box, Jorge
Faria, J. P.
Passegger, V.M.
González Hernández, Jonay I.
Figueira, Pedro
Sozzetti, Alessandro
Rebolo López, Rafael
Pepe, F.
Santos, Nuno C.
Cristiani, Stefano
Lovis, Christophe
Silva, André
Ribas, Ignasi
Amado, Pedro J.
Caballero, J. A.
Quirrenbach, Andreas
Reiners, Ansgar
Zechmeister, Mathias
Adibekyan, Vardan
Alibert, Y.
Béjar, Victor J. S.
Benatti, S.
D'Odorico, Valentina
Damasso, M.
Delisle, J. -B.
Di Marcantonio, P.
Dreizler, S.
Ehrenreich, David
Hatzes, Artie P.
Hara, N. C.
Henning, Thomas
Kaminski, Adriaan
López González, Maria J.
Martins, C.J.A.P.
Micela, Giusi
Montes, D.
Pallé, Enric
Pedraz, S.
Rodríguez Martínez, Eloy
Rodríguez-López, Cristina
Tal-Or, L.
Sousa, S. G.
Udry, Stephane
Ministerio de Ciencia e Innovación (España)
European Commission
Ministerio de Ciencia, Innovación y Universidades (España)
Agencia Estatal de Investigación (España)
Consejo Superior de Investigaciones Científicas (España)
Fundação para a Ciência e a Tecnologia (Portugal)
Junta de Andalucía
Swiss National Science Foundation
Gobierno de Canarias
Suárez Mascareño, A.
González-Álvarez, E.
Zapatero Osorio, María Rosa
Lillo-Box, Jorge
Faria, J. P.
Passegger, V.M.
González Hernández, Jonay I.
Figueira, Pedro
Sozzetti, Alessandro
Rebolo López, Rafael
Pepe, F.
Santos, Nuno C.
Cristiani, Stefano
Lovis, Christophe
Silva, André
Ribas, Ignasi
Amado, Pedro J.
Caballero, J. A.
Quirrenbach, Andreas
Reiners, Ansgar
Zechmeister, Mathias
Adibekyan, Vardan
Alibert, Y.
Béjar, Victor J. S.
Benatti, S.
D'Odorico, Valentina
Damasso, M.
Delisle, J. -B.
Di Marcantonio, P.
Dreizler, S.
Ehrenreich, David
Hatzes, Artie P.
Hara, N. C.
Henning, Thomas
Kaminski, Adriaan
López González, Maria J.
Martins, C.J.A.P.
Micela, Giusi
Montes, D.
Pallé, Enric
Pedraz, S.
Rodríguez Martínez, Eloy
Rodríguez-López, Cristina
Tal-Or, L.
Sousa, S. G.
Udry, Stephane
Publication Year :
2023

Abstract

We report the discovery and characterisation of two Earth-mass planets orbiting in the habitable zone of the nearby M-dwarf GJ 1002 based on the analysis of the radial-velocity (RV) time series from the ESPRESSO and CARMENES spectrographs. The host star is the quiet M5.5 V star GJ 1002 (relatively faint in the optical, V ~ 13.8 mag, but brighter in the infrared, J ~ 8.3 mag), located at 4.84 pc from the Sun. We analyse 139 spectroscopic observations taken between 2017 and 2021. We performed a joint analysis of the time series of the RV and full-width half maximum (FWHM) of the cross-correlation function (CCF) to model the planetary and stellar signals present in the data, applying Gaussian process regression to deal with the stellar activity. We detect the signal of two planets orbiting GJ 1002. GJ 1002 b is a planet with a minimum mass mp sin i of 1.08 ± 0.13 M⊕ with an orbital period of 10.3465 ± 0.0027 days at a distance of 0.0457 ± 0.0013 au from its parent star, receiving an estimated stellar flux of 0.67 F⊕. GJ 1002 c is a planet with a minimum mass mp sin i of 1.36 ± 0.17 M⊕ with an orbital period of 20.202 ± 0.013 days at a distance of 0.0738 ± 0.0021 au from its parent star, receiving an estimated stellar flux of 0.257 F⊕. We also detect the rotation signature of the star, with a period of 126 ± 15 days. We find that there is a correlation between the temperature of certain optical elements in the spectrographs and changes in the instrumental profile that can affect the scientific data, showing a seasonal behaviour that creates spurious signals at periods longer than ~200 days. GJ 1002 is one of the few known nearby systems with planets that could potentially host habitable environments. The closeness of the host star to the Sun makes the angular sizes of the orbits of both planets (~9.7 mas and ~15.7 mas, respectively) large enough for their atmosphere to be studied via high-contrast high-resolution spectroscopy with instruments such as the future spectrog

Details

Database :
OAIster
Notes :
English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1380455999
Document Type :
Electronic Resource