A One-Dimensional Energy Balance Model Parameterization for the Formation of CO2 Ice on the Surfaces of Eccentric Extrasolar Planets
arXiv:2501.11667 · doi:10.1089/ast.2023.0103
Abstract
Eccentric planets may spend a significant portion of their orbits at large distances from their host stars, where low temperatures can cause atmospheric CO2 to condense out onto the surface, similar to the polar ice caps on Mars. The radiative effects on the climates of these planets throughout their orbits would depend on the wavelength-dependent albedo of surface CO2 ice that may accumulate at or near apoastron and vary according to the spectral energy distribution of the host star. To explore these possible effects, we incorporated a CO2 ice-albedo parameterization into a one-dimensional energy balance climate model. With the inclusion of this parameterization, our simulations demonstrated that F-dwarf planets require 29% more orbit-averaged flux to thaw out of global water ice cover compared with simulations that solely use a traditional pure water ice-albedo parameterization. When no eccentricity is assumed, and host stars are varied, F-dwarf planets with higher bond albedos relative to their M-dwarf planet counterparts require 30% more orbit-averaged flux to exit a water snowball state. Additionally, the intense heat experienced at periastron aids eccentric planets in exiting a snowball state with a smaller increase in instellation compared with planets on circular orbits; this enables eccentric planets to exhibit warmer conditions along a broad range of instellation. This study emphasizes the significance of incorporating an albedo parameterization for the formation of CO2 ice into climate models to accurately assess the habitability of eccentric planets, as we show that, even at moderate eccentricities, planets with Earth-like atmospheres can reach surface temperatures cold enough for the condensation of CO2 onto their surfaces, as can planets receiving low amounts of instellation on circular orbits.
18 pages, 14 figures
References in corpus (62)
- The James Webb Space Telescope
- Habitable Zones Around Main-Sequence Stars: New Estimates
- Habitable Zones Around Main-Sequence Stars: Dependence on Planetary Mass
- Biosignatures from Earth-Like Planets Around M Dwarfs
- The Pluto system: Initial results from its exploration by New Horizons
- Stabilizing Cloud Feedback Dramatically Expands the Habitable Zone of Tidally Locked Planets
- Global modelling of the early Martian climate under a denser CO2 atmosphere: Water cycle and ice evolution
- 3D modelling of the early Martian Climate under a denser CO2 atmosphere: Temperatures and CO2 ice clouds
- The Habitability of Planets Orbiting M-dwarf Stars
- Exoplanet Orbital Eccentricities Derived From LAMOST-Kepler Analysis
- Thermal emission from the Earth-sized exoplanet TRAPPIST-1 b using JWST
- Modelling climate diversity, tidal dynamics and the fate of volatiles on TRAPPIST-1 planets
- The Effect of Host Star Spectral Energy Distribution and Ice-Albedo Feedback on the Climate of Extrasolar Planets
- HD 80606 b, a planet on an extremely elongated orbit
- Cometary Chemistry and the Origin of Icy Solar System Bodies, the view after Rosetta
- Habitable Climates: The Influence of Obliquity
- Habitable Climates: The Influence of Eccentricity
- Scientific Discovery with the James Webb Space Telescope
- Is Gliese 581d habitable? Some constraints from radiative-convective climate modeling
- Resolving Orbital and Climate Keys of Earth and Extraterrestrial Environments with Dynamics 1.0: A General Circulation Model for Simulating the Climates of Rocky Planets
- Generalized Milankovitch Cycles and Longterm Climatic Habitability
- Tides and the Evolution of Planetary Habitability
- A Volcanic Hydrogen Habitable Zone
- High eccentricity planets from the Anglo-Australian Planet Search
- Suppression of the water ice and snow albedo feedback on planets orbiting red dwarf stars and the subsequent widening of the habitable zone
- The CORALIE survey for southern extra-solar planets XV. Discovery of two eccentric planets orbiting HD4113 and HD156846
- Constraints on Climate and Habitability for Earth-like Exoplanets Determined from a General Circulation Model
- Habitability of planets on eccentric orbits: the limits of the mean flux approximation
- Selection Functions in Doppler Planet Searches
- Limit cycles can reduce the width of the habitable zone
- A more comprehensive habitable zone for finding life on other planets
- Methane and Nitrogen Abundances On Pluto and Eris
- The Equilibrium Temperature of Planets in Elliptical Orbits
- Climate simulations of early Mars with estimated precipitation, runoff, and erosion rates
- Red Dots: A temperate 1.5 Earth-mass planet in a compact multi-terrestrial planet system around GJ1061
- Spectrum-driven Planetary Deglaciation Due to Increases in Stellar Luminosity
- Effects of variable eccentricity on the climate of an Earth-like world
- A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS
- The CARMENES search for exoplanets around M dwarfs. Three temperate to warm super-Earths
- A Second Planet Transiting LTT 1445A and a Determination of the Masses of Both Worlds
- CO2 condensation is a serious limit to the deglaciation of Earth-like planets
- Photometric Phase Variations of Long-Period Eccentric Planets
- Convection in Condensible-rich Atmospheres
- The Pan-Pacific Planet Search VII: The most eccentric planet orbiting a giant star
- Exo-Milankovitch Cycles II: Climates of G-dwarf Planets in Dynamically Hot Systems
- Space-based infrared interferometry to study exoplanetary atmospheres
- Habitability and Water Loss Limits on Eccentric Planets Orbiting Main Sequence Stars
- Evidence for Reflected Light from the Most Eccentric Exoplanet Known
- Terminator Habitability: the Case for Limited Water Availability on M-dwarf Planets
- TOI-1728b: The Habitable-zone Planet Finder confirms a warm super Neptune orbiting an M dwarf host
- The Effect of Land Albedo on the Climate of Land-Dominated Planets in the TRAPPIST-1 System
- Kepler-1656b: a Dense Sub-Saturn With an Extreme Eccentricity
- Superhabitability of High-Obliquity and High-Eccentricity Planets
- Hydrohalite Salt-albedo Feedback Could Cool M-dwarf Planets
- HAZMAT. VIII. A Spectroscopic Analysis of the Ultraviolet Evolution of K Stars: Additional Evidence for K Dwarf Rotational Stalling in the First Gigayear
- The Effect of Land Fraction and Host Star Spectral Energy Distribution on the Planetary Albedo of Terrestrial Worlds
- Kepler-1656b's Extreme Eccentricity: Signature of a Gentle Giant
- Global or Local Pure-Condensible Atmospheres: Importance of Horizontal Latent Heat Transport
- Aquaplanet Models on Eccentric Orbits: Effects of Rotation Rate on Observables
- The influence of surface condensation on the evolution of warm and cold rocky planets orbiting Sun-like stars
- Energy Budgets for Terrestrial Extrasolar Planets
- Purple is the new green: biopigments and spectra of Earth-like purple worlds