Red Dots: A temperate 1.5 Earth-mass planet candidate in a compact multi-terrestrial planet system around GJ 1061<SUP>★</SUP>

DOI: 
10.1093/mnras/staa248
Publication date: 
01/01/2020
Main author: 
Dreizler, S.
IAA authors: 
Rodríguez, E.;López-González, M. J.;Morales, N.;Rodríguez López, C.;Anglada-Escudé, G.
Authors: 
Dreizler, S.;Jeffers, S. V.;Rodríguez, E.;Zechmeister, M.;Barnes, J. R.;Haswell, C. A.;Coleman, G. A. L.;Lalitha, S.;Hidalgo Soto, D.;Strachan, J. B. P.;Hambsch, F. -J.;López-González, M. J.;Morales, N.;Rodríguez López, C.;Berdiñas, Z. M.;Ribas, I.;Pallé, E.;Reiners, A.;Anglada-Escudé, G.
Journal: 
Monthly Notices of the Royal Astronomical Society
Refereed: 
Yes
Publication type: 
Article
Pages: 
235
Abstract: 
Small low-mass stars are favourable targets for the detection of rocky habitable planets. In particular, planetary systems in the solar neighbourhood are interesting and suitable for precise characterisation. The Red Dots campaigns seek to discover rocky planets orbiting nearby low-mass stars. The 2018 campaign targeted GJ 1061, which is the 20<SUP>th</SUP> nearest star to the Sun. For three consecutive months we obtained nightly, high-precision radial velocity measurements with the HARPS spectrograph. We analysed these data together with archival HARPS data. We report the detection of three planet candidates with periods of 3.204 ± 0.001, 6.689 ± 0.005 and 13.03 ± 0.03 days, which are close to 1:2:4 period commensurability. After several considerations related to the properties of the noise and sampling, we conclude that a 4<SUP>th</SUP> signal is most likely explained by stellar rotation, although it may be due to a planet. The proposed three-planet system (and the potential four-planet solution) is long-term dynamically stable. Planet-planet gravitational interactions are below our current detection threshold. The minimum masses of the three planets range from 1.4±0.2 to 1.8±0.3 M<SUB>⊕</SUB>. Planet d, with msin i = 1.64 ± 0.24M<SUB>⊕</SUB>, receives a similar amount of energy as Earth receives from the Sun. Consequently it lies within the liquid-water habitable zone of the star and has a similar equilibrium temperature to Earth. GJ 1061 has very similar properties to Proxima Centauri but activity indices point to lower levels of stellar activity.
Database: 
ADS
URL: 
https://ui.adsabs.harvard.edu/#abs/2020MNRAS.493..536D/abstract
ADS Bibcode: 
2020MNRAS.493..536D
Keywords: 
methods: data analysis;planetary systems;stars: late-type;stars: individual: GJ 1061;techniques: radial velocities;Astrophysics - Earth and Planetary Astrophysics;Astrophysics - Solar and Stellar Astrophysics