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. 2023 May;617(7962):701-705.
doi: 10.1038/s41586-023-05934-8. Epub 2023 May 17.

A temperate Earth-sized planet with tidal heating transiting an M6 star

Merrin S Peterson  1 Björn Benneke  2 Karen Collins  3 Caroline Piaulet  1 Ian J M Crossfield  4 Mohamad Ali-Dib  1   5 Jessie L Christiansen  6 Jonathan Gagné  7 Jackie Faherty  8 Edwin Kite  9 Courtney Dressing  10 David Charbonneau  3 Felipe Murgas  11 Marion Cointepas  12 Jose Manuel Almenara  12 Xavier Bonfils  12 Stephen Kane  13 Michael W Werner  14 Varoujan Gorjian  14 Pierre-Alexis Roy  1 Avi Shporer  15 Francisco J Pozuelos  16   17 Quentin Jay Socia  18 Ryan Cloutier  3   19 Jamie Dietrich  18 Jonathan Irwin  3 Lauren Weiss  20 William Waalkes  21 Zach Berta-Thomson  21 Thomas Evans  15 Daniel Apai  18   22 Hannu Parviainen  11 Enric Pallé  11 Norio Narita  11   23   24 Andrew W Howard  25 Diana Dragomir  26 Khalid Barkaoui  17   27 Michaël Gillon  17 Emmanuel Jehin  28 Elsa Ducrot  17 Zouhair Benkhaldoun  27 Akihiko Fukui  11   23 Mayuko Mori  29 Taku Nishiumi  24   30   31 Kiyoe Kawauchi  11   31 George Ricker  15 David W Latham  3 Joshua N Winn  32 Sara Seager  15   33   34 Howard Isaacson  10 Alex Bixel  18 Aidan Gibbs  35 Jon M Jenkins  36 Jeffrey C Smith  37 Jose Perez Chavez  38 Benjamin V Rackham  15 Thomas Henning  39 Paul Gabor  40 Wen-Ping Chen  41 Nestor Espinoza  42 Eric L N Jensen  43 Kevin I Collins  44 Richard P Schwarz  3 Dennis M Conti  45 Gavin Wang  46 John F Kielkopf  47 Shude Mao  48 Keith Horne  49 Ramotholo Sefako  50 Samuel N Quinn  3 Dan Moldovan  51 Michael Fausnaugh  15 Gábor Fűűrész  15 Thomas Barclay  52   53
Affiliations

A temperate Earth-sized planet with tidal heating transiting an M6 star

Merrin S Peterson et al. Nature. 2023 May.

Abstract

Temperate Earth-sized exoplanets around late-M dwarfs offer a rare opportunity to explore under which conditions planets can develop hospitable climate conditions. The small stellar radius amplifies the atmospheric transit signature, making even compact secondary atmospheres dominated by N2 or CO2 amenable to characterization with existing instrumentation1. Yet, despite large planet search efforts2, detection of low-temperature Earth-sized planets around late-M dwarfs has remained rare and the TRAPPIST-1 system, a resonance chain of rocky planets with seemingly identical compositions, has not yet shown any evidence of volatiles in the system3. Here we report the discovery of a temperate Earth-sized planet orbiting the cool M6 dwarf LP 791-18. The newly discovered planet, LP 791-18d, has a radius of 1.03 ± 0.04 R and an equilibrium temperature of 300-400 K, with the permanent night side plausibly allowing for water condensation. LP 791-18d is part of a coplanar system4 and provides a so-far unique opportunity to investigate a temperate exo-Earth in a system with a sub-Neptune that retained its gas or volatile envelope. On the basis of observations of transit timing variations, we find a mass of 7.1 ± 0.7 M for the sub-Neptune LP 791-18c and a mass of [Formula: see text] for the exo-Earth LP 791-18d. The gravitational interaction with the sub-Neptune prevents the complete circularization of LP 791-18d's orbit, resulting in continued tidal heating of LP 791-18d's interior and probably strong volcanic activity at the surface5,6.

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References

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