_version_ 1866910455294853120
author Dholakia, Shishir
Palethorpe, Larissa
Venner, Alexander
Mortier, Annelies
Wilson, Thomas G.
Huang, Chelsea X.
Rice, Ken
Van Eylen, Vincent
Nabbie, Emma
Cloutier, Ryan
Boschin, Walter
Ciardi, David
Delrez, Laetitia
Dransfield, Georgina
Ducrot, Elsa
Essack, Zahra
Everett, Mark E.
Gillon, Michaël
Hooton, Matthew J.
Kunimoto, Michelle
Latham, David W.
López-Morales, Mercedes
Li, Bin
Li, Fan
McDermott, Scott
Murphy, Simon
Murray, Catriona A.
Seager, Sara
Timmermans, Mathilde
Triaud, Amaury
Turner, Daisy A.
Twicken, Joseph D.
Vanderburg, Andrew
Wang, Su
Wittenmyer, Robert A.
Wright, Duncan
author_facet Dholakia, Shishir
Palethorpe, Larissa
Venner, Alexander
Mortier, Annelies
Wilson, Thomas G.
Huang, Chelsea X.
Rice, Ken
Van Eylen, Vincent
Nabbie, Emma
Cloutier, Ryan
Boschin, Walter
Ciardi, David
Delrez, Laetitia
Dransfield, Georgina
Ducrot, Elsa
Essack, Zahra
Everett, Mark E.
Gillon, Michaël
Hooton, Matthew J.
Kunimoto, Michelle
Latham, David W.
López-Morales, Mercedes
Li, Bin
Li, Fan
McDermott, Scott
Murphy, Simon
Murray, Catriona A.
Seager, Sara
Timmermans, Mathilde
Triaud, Amaury
Turner, Daisy A.
Twicken, Joseph D.
Vanderburg, Andrew
Wang, Su
Wittenmyer, Robert A.
Wright, Duncan
contents We report on the discovery of Gliese 12 b, the nearest transiting temperate, Earth-sized planet found to date. Gliese 12 is a bright ($V=12.6$ mag, $K=7.8$ mag) metal-poor M4V star only $12.162\pm0.005$ pc away from the Solar System with one of the lowest stellar activity levels known for an M-dwarf. A planet candidate was detected by TESS based on only 3 transits in sectors 42, 43, and 57, with an ambiguity in the orbital period due to observational gaps. We performed follow-up transit observations with CHEOPS and ground-based photometry with MINERVA-Australis, SPECULOOS, and Purple Mountain Observatory, as well as further TESS observations in sector 70. We statistically validate Gliese 12 b as a planet with an orbital period of $12.76144\pm0.00006$ days and a radius of $1.0\pm{0.1}$ R$_\oplus$, resulting in an equilibrium temperature of $\sim$315K. Gliese 12 b has excellent future prospects for precise mass measurement, which may inform how planetary internal structure is affected by the stellar compositional environment. Gliese 12 b also represents one of the best targets to study whether Earth-like planets orbiting cool stars can retain their atmospheres, a crucial step to advance our understanding of habitability on Earth and across the Galaxy.
format Preprint
id arxiv_https___arxiv_org_abs_2405_13118
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Gliese 12 b, A Temperate Earth-sized Planet at 12 Parsecs Discovered with TESS and CHEOPS
Dholakia, Shishir
Palethorpe, Larissa
Venner, Alexander
Mortier, Annelies
Wilson, Thomas G.
Huang, Chelsea X.
Rice, Ken
Van Eylen, Vincent
Nabbie, Emma
Cloutier, Ryan
Boschin, Walter
Ciardi, David
Delrez, Laetitia
Dransfield, Georgina
Ducrot, Elsa
Essack, Zahra
Everett, Mark E.
Gillon, Michaël
Hooton, Matthew J.
Kunimoto, Michelle
Latham, David W.
López-Morales, Mercedes
Li, Bin
Li, Fan
McDermott, Scott
Murphy, Simon
Murray, Catriona A.
Seager, Sara
Timmermans, Mathilde
Triaud, Amaury
Turner, Daisy A.
Twicken, Joseph D.
Vanderburg, Andrew
Wang, Su
Wittenmyer, Robert A.
Wright, Duncan
Earth and Planetary Astrophysics
We report on the discovery of Gliese 12 b, the nearest transiting temperate, Earth-sized planet found to date. Gliese 12 is a bright ($V=12.6$ mag, $K=7.8$ mag) metal-poor M4V star only $12.162\pm0.005$ pc away from the Solar System with one of the lowest stellar activity levels known for an M-dwarf. A planet candidate was detected by TESS based on only 3 transits in sectors 42, 43, and 57, with an ambiguity in the orbital period due to observational gaps. We performed follow-up transit observations with CHEOPS and ground-based photometry with MINERVA-Australis, SPECULOOS, and Purple Mountain Observatory, as well as further TESS observations in sector 70. We statistically validate Gliese 12 b as a planet with an orbital period of $12.76144\pm0.00006$ days and a radius of $1.0\pm{0.1}$ R$_\oplus$, resulting in an equilibrium temperature of $\sim$315K. Gliese 12 b has excellent future prospects for precise mass measurement, which may inform how planetary internal structure is affected by the stellar compositional environment. Gliese 12 b also represents one of the best targets to study whether Earth-like planets orbiting cool stars can retain their atmospheres, a crucial step to advance our understanding of habitability on Earth and across the Galaxy.
title Gliese 12 b, A Temperate Earth-sized Planet at 12 Parsecs Discovered with TESS and CHEOPS
topic Earth and Planetary Astrophysics
url https://arxiv.org/abs/2405.13118