Bibcode
Turner, Daisy A.; Eschen, Yoshi Nike Emilia; Murgas, Felipe; Mortier, Annelies; Wilson, Thomas G.; Fernández Fernández, Jorge; Gromek, Nicole; Morello, Giuseppe; Tabernero, Hugo M.; Egger, Jo Ann; Vissapragada, Shreyas; Caballero, José A.; Dreizler, Stefan; Freckelton, Alix Violet; Hatzes, Artie P.; Lakeland, Ben Scott; Nagel, Evangelos; Naponiello, Luca; Vanaverbeke, Siegfried; Venner, Alexander; Zapatero Osorio, María Rosa; Amado, Pedro J.; Béjar, Víctor J. S.; Bonomo, Aldo Stefano; Buchhave, Lars A.; Collier Cameron, Andrew; Carleo, Ilaria; Chaturvedi, Priyanka; Cloutier, Ryan; Damasso, Mario; Daspute, Mangesh; Dholakia, Shishir; Dufoer, Sjoerd; Dumusque, Xavier; Martinez Fiorenzano, Aldo Fabricio; Ghedina, Adriano; Harutyunyan, Avet; Herrero, Enrique; John, Ancy Anna; Lillo-Box, Jorge; Lodieu, Nicolas; López-Morales, Mercedes; Malavolta, Luca; Mancini, Luigi; Mantovan, Giacomo; Montes, David; Morales, Juan Carlos; Nicholson, Belinda; Orell-Miquel, Jaume; Palethorpe, Larissa; Palle, Enric; Quirrenbach, Andreas; Reffert, Sabine; Reiners, Ansgar; Ribas, Ignasi; Rice, Ken; Silva, André M.; Sozzetti, Alessandro; Stalport, Manu; Tal-Or, Lev; Trifonov, Trifon; Udry, Stéphane; Zechmeister, Mathias
Referencia bibliográfica
Monthly Notices of the Royal Astronomical Society
Fecha de publicación:
1
2026
Número de citas
2
Número de citas referidas
0
Descripción
Small temperate planets are prime targets for exoplanet studies due to their possible similarities with the rocky planets in the Solar system. M dwarfs are promising hosts since the planetary signals are within our current detection capabilities. Gliese 12 b is a Venus-sized temperate planet orbiting a quiet M dwarf. We present here the first precise mass measurement of this small exoplanet. We performed a detailed analysis using HARPS-N (High Accuracy Radial velocity Planet Searcher for the Northern Hemisphere), ESPRESSO (Echelle Spectrograph for Rocky Exoplanets and Stable Spectroscopic Observations), and CARMENES (Calar Alto high-Resolution search for M dwarfs with Exoearths with Near-infrared and optical Echelle Spectrographs) radial velocities, along with new and archival TESS (Transiting Exoplanet Survey Satellite), CHEOPS (CHaracterising ExOPlanet Satellite), and MuSCAT2/3 (Multicolor Simultaneous Camera for studying Atmospheres of Transiting exoplanets) photometry data. From fitting the available data, we find that the planet has a radius of $R_\mathrm{p} = 0.93\pm 0.06 \, \mathrm{R_{\rm{\oplus }}}$ and a mass of $M_\mathrm{p} = 0.95^{+0.29}_{-0.30} \, \mathrm{M_{\rm{\oplus }}}$ (a $3.2\sigma$ measurement of the semi-amplitude $K=0.67\pm 0.21\, \mathrm{m\, s^{-1}}$), and is on an orbit with a period of $12.761418^{+0.000060}_{-0.000055}\, \mathrm{d}$. A variety of techniques were utilized to attenuate stellar activity signals. Gliese 12 b has an equilibrium temperature of $T_\mathrm{eq}=317 \pm 8\, \mathrm{K}$, assuming an albedo of zero, and a density consistent with that of Earth and Venus ($\rho _\mathrm{p}=6.4\pm 2.4\, \mathrm{g\, cm^{-3}}$). We find that Gliese 12 b has a predominantly rocky interior and simulations indicate that it is unlikely to have retained any of its primordial gaseous envelope. The bulk properties of Gliese 12 b place it in an extremely sparsely populated region of both mass─radius and density─$T_\mathrm{eq}$ parameter space, making it a prime target for follow-up observations, including Lyman-$\alpha$ studies.