An Earth-like Density for the Temperate Earth-sized Planet GJ 12b
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arXiv
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| Main Authors: | , , , , , , , , , , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866909660030697472 |
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| author | Brady, Madison Bean, Jacob Basant, Ritvik Brown, Nina Das, Tanya Nixon, Matthew Luque, Rafael Piaulet-Ghorayeb, Caroline Radica, Michael Seifahrt, Andreas Stürmer, Julian Zhao, Lily |
| author_facet | Brady, Madison Bean, Jacob Basant, Ritvik Brown, Nina Das, Tanya Nixon, Matthew Luque, Rafael Piaulet-Ghorayeb, Caroline Radica, Michael Seifahrt, Andreas Stürmer, Julian Zhao, Lily |
| contents | While JWST has provided us with the opportunity to probe the atmospheres of potentially-habitable planets, observations of the TRAPPIST-1 system have shown us that active stars severely complicate efforts at studying their planets. GJ 12b is a newly-discovered temperate (Teq ~ 300 K), Earth-sized (Rp = 0.96 +/- 0.05 Earth radii) planet orbiting an inactive M dwarf that might be a good alternate to the TRAPPIST-1 planets for atmospheric characterization. In this paper, we use MAROON-X radial velocities to measure a mass of 0.71 +/- 0.12 Earth masses for GJ 12b. We also find moderate evidence that the planet has an eccentric (e ~ 0.16) orbit. GJ 12b's mass results in a planetary density comparable to or less dense than Earth, possibly indicating the presence of water or a low bulk iron mass fraction. With its low mass, GJ 12b is likely within reach of JWST transmission spectroscopy observations, making it an excellent target for determining the location of the cosmic shoreline. Its low mass may mean that the planet could have trouble retaining its primary atmosphere during the star's active pre-main-sequence phase. However, if it has a heightened eccentricity, it may be able to sustain a secondary atmosphere through tidally-induced volcanism. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2506_20561 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | An Earth-like Density for the Temperate Earth-sized Planet GJ 12b Brady, Madison Bean, Jacob Basant, Ritvik Brown, Nina Das, Tanya Nixon, Matthew Luque, Rafael Piaulet-Ghorayeb, Caroline Radica, Michael Seifahrt, Andreas Stürmer, Julian Zhao, Lily Earth and Planetary Astrophysics While JWST has provided us with the opportunity to probe the atmospheres of potentially-habitable planets, observations of the TRAPPIST-1 system have shown us that active stars severely complicate efforts at studying their planets. GJ 12b is a newly-discovered temperate (Teq ~ 300 K), Earth-sized (Rp = 0.96 +/- 0.05 Earth radii) planet orbiting an inactive M dwarf that might be a good alternate to the TRAPPIST-1 planets for atmospheric characterization. In this paper, we use MAROON-X radial velocities to measure a mass of 0.71 +/- 0.12 Earth masses for GJ 12b. We also find moderate evidence that the planet has an eccentric (e ~ 0.16) orbit. GJ 12b's mass results in a planetary density comparable to or less dense than Earth, possibly indicating the presence of water or a low bulk iron mass fraction. With its low mass, GJ 12b is likely within reach of JWST transmission spectroscopy observations, making it an excellent target for determining the location of the cosmic shoreline. Its low mass may mean that the planet could have trouble retaining its primary atmosphere during the star's active pre-main-sequence phase. However, if it has a heightened eccentricity, it may be able to sustain a secondary atmosphere through tidally-induced volcanism. |
| title | An Earth-like Density for the Temperate Earth-sized Planet GJ 12b |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2506.20561 |