Atmospheric carbon depletion as a tracer of water oceans and biomass on temperate terrestrial exoplanets
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arXiv
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| Main Authors: | , , , , , , , , , , , |
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| Format: | Preprint |
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2023
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| _version_ | 1866914630496944128 |
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| author | Triaud, Amaury H. M. J. de Wit, Julien Klein, Frieder Turbet, Martin Rackham, Benjamin V. Niraula, Prajwal Glidden, Ana Jagoutz, Oliver E. Pec, Matej Petkowski, Janusz J. Seager, Sara Selsis, Franck |
| author_facet | Triaud, Amaury H. M. J. de Wit, Julien Klein, Frieder Turbet, Martin Rackham, Benjamin V. Niraula, Prajwal Glidden, Ana Jagoutz, Oliver E. Pec, Matej Petkowski, Janusz J. Seager, Sara Selsis, Franck |
| contents | The conventional observables to identify a habitable or inhabited environment in exoplanets, such as an ocean glint or abundant atmospheric O$_2$, will be challenging to detect with present or upcoming observatories. Here we suggest a new signature. A low carbon abundance in the atmosphere of a temperate rocky planet, relative to other planets of the same system, traces the presence of substantial amount of liquid water, plate tectonic and/or biomass. We show that JWST can already perform such a search in some selected systems like TRAPPIST-1 via the CO$_2$ band at $4.3\,\rm μm$, which falls in a spectral sweet spot where the overall noise budget and the effect of cloud/hazes are optimal. We propose a 3-step strategy for transiting exoplanets: 1) detection of an atmosphere around temperate terrestrial planets in $\sim 10$ transits for the most favorable systems, (2) assessment of atmospheric carbon depletion in $\sim 40$ transits, (3) measurements of O$_3$ abundance to disentangle between a water- vs biomass-supported carbon depletion in $\sim100$ transits. The concept of carbon depletion as a signature for habitability is also applicable for next-generation direct imaging telescopes. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2310_14987 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | Atmospheric carbon depletion as a tracer of water oceans and biomass on temperate terrestrial exoplanets Triaud, Amaury H. M. J. de Wit, Julien Klein, Frieder Turbet, Martin Rackham, Benjamin V. Niraula, Prajwal Glidden, Ana Jagoutz, Oliver E. Pec, Matej Petkowski, Janusz J. Seager, Sara Selsis, Franck Earth and Planetary Astrophysics The conventional observables to identify a habitable or inhabited environment in exoplanets, such as an ocean glint or abundant atmospheric O$_2$, will be challenging to detect with present or upcoming observatories. Here we suggest a new signature. A low carbon abundance in the atmosphere of a temperate rocky planet, relative to other planets of the same system, traces the presence of substantial amount of liquid water, plate tectonic and/or biomass. We show that JWST can already perform such a search in some selected systems like TRAPPIST-1 via the CO$_2$ band at $4.3\,\rm μm$, which falls in a spectral sweet spot where the overall noise budget and the effect of cloud/hazes are optimal. We propose a 3-step strategy for transiting exoplanets: 1) detection of an atmosphere around temperate terrestrial planets in $\sim 10$ transits for the most favorable systems, (2) assessment of atmospheric carbon depletion in $\sim 40$ transits, (3) measurements of O$_3$ abundance to disentangle between a water- vs biomass-supported carbon depletion in $\sim100$ transits. The concept of carbon depletion as a signature for habitability is also applicable for next-generation direct imaging telescopes. |
| title | Atmospheric carbon depletion as a tracer of water oceans and biomass on temperate terrestrial exoplanets |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2310.14987 |