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- W3102431859 abstract "LHS 1140 is an M dwarf known to host two known transiting planets at orbital periods of 3.77 and 24.7 days. The external planet (LHS 1140 b) is a rocky super-Earth that is located in the middle of the habitable zone of this low-mass star, placing this system at the forefront of the habitable exoplanet exploration. We further characterize this system by improving the physical and orbital properties and search for additional planetary-mass components in the system, also exploring the possibility of co-orbitals. We collected 113 new radial velocity observations with ESPRESSO over a 1.5-year time span with an average photon-noise precision of 1.07 m/s. We determine new masses with a precision of 6% for LHS 1140 b ($6.48 pm 0.46~M_{oplus}$) and 9% for LHS 1140 c ($m_c=1.78 pm 0.17~M_{oplus}$), reducing by half the previously published uncertainties. Although both planets have Earth-like bulk compositions, the internal structure analysis suggests that LHS 1140 b might be iron-enriched. In both cases, the water content is compatible to a maximum fraction of 10-12% in mass, which is equivalent to a deep ocean layer of $779 pm 650$ km for the habitable-zone planet LHS 1140 b. Our results also provide evidence for a new planet candidate in the system ($m_d= 4.8pm1.1~M_{oplus}$) on a ~78.9-day orbital period, which is detected through three independent methods. The analysis also allows us to discard other planets above 0.5 $M_{oplus}$ for periods shorter than 10 days and above 2 $M_{oplus}$ for periods up to one year. Finally, our analysis discards co-orbital planets of LHS 1140 b down to 1 $M_{oplus}$. Indications for a possible co-orbital signal in LHS 1140 c are detected in both radial velocity and photometric data, however. The new characterization of the system make it a key target for atmospheric studies of rocky worlds at different stellar irradiations" @default.
- W3102431859 created "2020-11-23" @default.
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- W3102431859 date "2020-10-01" @default.
- W3102431859 modified "2023-10-13" @default.
- W3102431859 title "Planetary system LHS 1140 revisited with ESPRESSO and TESS" @default.
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- W3102431859 cites W2020716381 @default.
- W3102431859 cites W2022113292 @default.
- W3102431859 cites W2025615742 @default.
- W3102431859 cites W2031887605 @default.
- W3102431859 cites W2035213284 @default.
- W3102431859 cites W2081815463 @default.
- W3102431859 cites W2084306225 @default.
- W3102431859 cites W2088072491 @default.
- W3102431859 cites W2089014417 @default.
- W3102431859 cites W2091460103 @default.
- W3102431859 cites W2096799072 @default.
- W3102431859 cites W2101167036 @default.
- W3102431859 cites W2101687185 @default.
- W3102431859 cites W2102515206 @default.
- W3102431859 cites W2126833612 @default.
- W3102431859 cites W2138385083 @default.
- W3102431859 cites W2151075722 @default.
- W3102431859 cites W2297162316 @default.
- W3102431859 cites W2343190161 @default.
- W3102431859 cites W2514404059 @default.
- W3102431859 cites W2605851178 @default.
- W3102431859 cites W2606686133 @default.
- W3102431859 cites W2729741217 @default.
- W3102431859 cites W2739265538 @default.
- W3102431859 cites W2766198534 @default.
- W3102431859 cites W2798336535 @default.
- W3102431859 cites W2809499035 @default.
- W3102431859 cites W2914436676 @default.
- W3102431859 cites W2942777410 @default.
- W3102431859 cites W2943428116 @default.
- W3102431859 cites W2951688286 @default.
- W3102431859 cites W2955141932 @default.
- W3102431859 cites W2963754333 @default.
- W3102431859 cites W2971688194 @default.
- W3102431859 cites W2975892868 @default.
- W3102431859 cites W3009681333 @default.
- W3102431859 cites W3032579245 @default.
- W3102431859 cites W3098865689 @default.
- W3102431859 cites W3099558145 @default.
- W3102431859 cites W3099682429 @default.
- W3102431859 cites W3099749551 @default.
- W3102431859 cites W3100484086 @default.
- W3102431859 cites W3100770095 @default.
- W3102431859 cites W3101015041 @default.
- W3102431859 cites W3102014803 @default.
- W3102431859 cites W3102286923 @default.
- W3102431859 cites W3103199344 @default.
- W3102431859 cites W3103224716 @default.
- W3102431859 cites W3104148413 @default.
- W3102431859 cites W3104335016 @default.
- W3102431859 cites W3104414789 @default.
- W3102431859 cites W3104455560 @default.
- W3102431859 cites W3104810115 @default.
- W3102431859 cites W3105493278 @default.
- W3102431859 cites W3105972254 @default.
- W3102431859 cites W3106126163 @default.
- W3102431859 cites W4288079914 @default.
- W3102431859 cites W4288360581 @default.
- W3102431859 cites W4289462170 @default.
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- W3102431859 doi "https://doi.org/10.1051/0004-6361/202038922" @default.
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