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LHS 1140 b is a potentially habitable water world

Published 20 Mar 2024 in astro-ph.EP | (2403.13265v2)

Abstract: LHS 1140 b is a small planet orbiting in the habitable zone of its M4.5V dwarf host. Recent mass and radius constraints have indicated that it has either a thick H2_2-rich atmosphere or substantial water by mass. Here we present a transmission spectrum of LHS 1140 b between 1.7 and 5.2 μ\mum, obtained using the NIRSpec instrument on JWST. By combining spectral retrievals and self-consistent atmospheric models, we show that the transmission spectrum is inconsistent with H2_2-rich atmospheres with varied size and metallicity, leaving a water world as the remaining scenario to explain the planet's low density. Specifically, a H2_2-rich atmosphere would result in prominent spectral features of CH4_4 or CO2_2 on this planet, but they are not seen in the transmission spectrum. Instead, the data favors a high-mean-molecular-weight atmosphere (possibly N2_2-dominated with H2_2O and CO2_2) with a modest confidence. Forming the planet by accreting C- and N-bearing ices could naturally give rise to a CO2_2- or N2_2-dominated atmosphere, and if the planet evolves to or has the climate-stabilizing mechanism to maintain a moderate-size CO2_2/N2_2-dominated atmosphere, the planet could have liquid-water oceans. Our models suggest CO2_2 absorption features with an expected signal of 20 ppm at 4.2 μ\mum. As the existence of an atmosphere on TRAPPIST-1 planets is uncertain, LHS 1140 b may well present the best current opportunity to detect and characterize a habitable world.

Citations (8)

Summary

  • The paper presents evidence from spectral and transit analyses indicating LHS 1140 b's potential to harbor liquid water.
  • It employs multi-wavelength observations and atmospheric modeling to assess the planet's habitability.
  • The results suggest that LHS 1140 b is a strong candidate for future exoplanet habitability studies.

An Examination of AAS and AMS Math Symbols in LaTeX

The paper under analysis provides a comprehensive inventory of mathematical symbols and accents available within the American Astronomical Society (AAS) and American Mathematical Society (AMS) document classes for LaTeX. This inventory is structured through a series of tables categorizing these symbols and accents according to their respective functionalities in document preparation.

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