Evolution and Observable Properties of Rocky Planet Atmospheres
arXiv:2607.11531 · doi:10.1007/s11214-026-01308-4
Abstract
The atmospheric composition of rocky exoplanets offers an important tool for constraining the properties of the interior of this type of planet, beyond what is possible from measurements of their mass and radius alone. However, the interpretation of these observations requires an understanding of the complex interplay of a larger number of coupled planetary and atmospheric processes. This review provides an overview of the current state of knowledge regarding rocky exoplanet atmospheres, beginning with their formation and escape mechanisms. We specifically highlight the importance of long-term interaction between the atmosphere, the surface, and the interior on rocky planets. Furthermore, this review addresses the influence of biological activity and photochemical reactions on the atmospheric compositions. Consequently, establishing how these different processes contribute to shaping the atmospheres of rocky exoplanets during their evolution is fundamental for the characterization of these planets with future space missions and ground-based surveys.
88 pages, 11 figures. Published in Space Science Reviews
References in corpus (226)
- Habitable Zones Around Main-Sequence Stars: New Estimates
- The California-Kepler Survey. III. A Gap in the Radius Distribution of Small Planets
- Detection of an Extrasolar Planet Atmosphere
- The origins and concentrations of water, carbon, nitrogen and noble gases on Earth
- A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion
- Images of a fourth planet orbiting HR 8799
- Clouds in the atmosphere of the super-Earth exoplanet GJ 1214b
- Evolution of the Solar Activity over Time and Effects on Planetary Atmospheres: I. High-energy Irradiances (1-1700 A)
- A map of the day-night contrast of the extrasolar planet HD 189733b
- Kepler planets: a tale of evaporation
- Most 1.6 Earth-Radius Planets are not Rocky
- The evaporation valley in the Kepler planets
- Atmospheric Circulation and Tides of "51Peg b-like" Planets
- Probabilistic Forecasting of the Masses and Radii of Other Worlds
- Infrared radiation from an extrasolar planet
- Extreme Water Loss and Abiotic O Buildup On Planets Throughout the Habitable Zones of M Dwarfs
- Rosseland and Planck Mean Opacities for Protoplanetary Discs
- Exoplanet Biosignatures: A Review of Remotely Detectable Signs of Life
- The California Kepler Survey VII. Precise Planet Radii Leveraging Gaia DR2 Reveal the Stellar Mass Dependence of the Planet Radius Gap
- An asteroseismic view of the radius valley: stripped cores, not born rocky
- Dynamics of Protoplanetary Disks
- Core-powered mass loss and the radius distribution of small exoplanets
- Detection of atmospheric haze on an extrasolar planet: The 0.55 - 1.05 micron transmission spectrum of HD189733b with the Hubble Space Telescope
- Roche lobe effects on the atmospheric loss of "Hot Jupiters"
- Separating gas-giant and ice-giant planets by halting pebble accretion
- Planetary evaporation by UV & X-ray radiation: basic hydrodynamics
- Sculpting the Valley in the Radius Distribution of Small Exoplanets as a by-product of Planet Formation: The Core-Powered Mass-Loss Mechanism
- The MUSCLES Treasury Survey I: Motivation and Overview
- How Thermal Evolution and Mass Loss Sculpt Populations of Super-Earths and Sub-Neptunes: Application to the Kepler-11 System and Beyond
- The Climate of Early Mars
- Increased insolation threshold for runaway greenhouse processes on Earth like planets
- The faint young Sun problem
- Observations of Mass Loss from the Transiting Exoplanet HD 209458b
- Exoplanet Biosignatures: Understanding Oxygen as a Biosignature in the Context of Its Environment
- Was Venus the First Habitable World of our Solar System?
- Density, not radius, separates rocky and water-rich small planets orbiting M dwarf stars
- Super-Earth Atmospheres: Self-Consistent Gas Accretion and Retention
- Inference of Inhomogeneous Clouds in an Exoplanet Atmosphere
- Breeding Super-Earths and Birthing Super-Puffs in Transitional Disks
- Compositional imprints in density-distance-time: a rocky composition for close-in low-mass exoplanets from the location of the valley of evaporation
- Photochemistry in Terrestrial Exoplanet Atmospheres I: Photochemistry Model and Benchmark Cases
- Make Super-Earths, Not Jupiters: Accreting Nebular Gas onto Solid Cores at 0.1 AU and Beyond
- Transient reducing greenhouse warming on early Mars
- The great dichotomy of the Solar System: small terrestrial embryos and massive giant planet cores
- Strong Dependence of the Inner Edge of the Habitable Zone on Planetary Rotation Rate
- The active lives of stars: a complete description of rotation and XUV evolution of F, G, K, and M dwarfs
- Absence of a thick atmosphere on the terrestrial exoplanet LHS 3844b
- Spectrally resolved helium absorption from the extended atmosphere of a warm Neptune-mass exoplanet
- The coronal X-ray - age relation and its implications for the evaporation of exoplanets
- To Cool is to Accrete: Analytic Scalings for Nebular Accretion of Planetary Atmospheres
- Thermal emission from the Earth-sized exoplanet TRAPPIST-1 b using JWST
- Constraints on the mass of a habitable planet with water of nebular origin
- The MUSCLES Treasury Survey III: X-ray to Infrared Spectra of 11 M and K Stars Hosting Planets
- Atmospheres of low-mass planets: the "boil-off"
- Abiotic oxygen-dominated atmospheres on terrestrial habitable zone planets
- Possible Disintegrating Short-Period Super-Mercury Orbiting KIC 12557548
- In-situ Accretion of Hydrogen-Rich Atmospheres on Short-Period Super-Earths: Implications for the Kepler-11 Planets
- Nitrogen Isotopic Composition and Density of the Archean Atmosphere
- Exoplanetary Atmospheres - Chemistry, Formation Conditions, and Habitability
- On the Minimum Core Mass for Giant Planet Formation at Wide Separations
- No thick carbon dioxide atmosphere on the rocky exoplanet TRAPPIST-1 c
- Exoplanet Biosignatures: A Framework for Their Assessment
- Atmospheric Mass Loss During Planet Formation: The Importance of Planetesimal Impacts
- Hydrodynamics of Embedded Planets' First Atmospheres. II. A Rapid Recycling of Atmospheric Gas
- Large Interferometer For Exoplanets (LIFE): I. Improved exoplanet detection yield estimates for a large mid-infrared space-interferometer mission
- Asynchronous rotation of Earth-mass planets in the habitable zone of lower-mass stars
- Abiotic O Levels on Planets around F, G, K, and M Stars: Possible False Positives for Life?
- High Stellar FUV/NUV Ratio and Oxygen Contents in the Atmospheres of Potentially Habitable Planets
- Chemistry of atmospheres formed during accretion of the Earth and other terrestrial planets
- The Gaia-Kepler Stellar Properties Catalog. II. Planet Radius Demographics as a Function of Stellar Mass and Age
- The Deep Blue Color of HD189733b: Albedo Measurements with Hubble Space Telescope/Space Telescope Imaging Spectrograph at Visible Wavelengths
- Strange messenger: A new history of hydrogen on Earth, as told by Xenon
- The Complete transmission spectrum of WASP-39b with a precise water constraint
- Venusian Habitable Climate Scenarios: Modeling Venus through time and applications to slowly rotating Venus-Like Exoplanets
- HAZMAT I: The Evolution of Far-UV and Near-UV Emission from Early M Stars
- Origin and Loss of nebula-captured hydrogen envelopes from "sub"- to "super-Earths" in the habitable zone of Sun-like stars
- The K2-ESPRINT Project. I. Discovery of the Disintegrating Rocky Planet K2-22b with a Cometary Head and Leading Tail
- Planet formation with envelope enrichment: new insights on planetary diversity
- Day-night cloud asymmetry prevents early oceans on Venus but not on Earth
- KOI-2700b - A Planet Candidate With Dusty Effluents on a 22-Hour Orbit
- Outgassing of Ordinary Chondritic Material and Some of its Implications for the Chemistry of Asteroids, Planets, and Satellites
- Energy-limited escape revised
- Atmosphere-interior exchange on hot rocky exoplanets
- A grid of upper atmosphere models for 1--40 MEARTH planets: application to CoRoT-7 b and HD219134 b,c
- New observations of the extended hydrogen exosphere of the extrasolar planet HD209458b
- Gas Giant Formation with Small Cores Triggered by Envelope Pollution by Icy Planetesimals
- Oxygen fugacities of extrasolar rocks: Evidence for an Earth-like geochemistry of exoplanets
- An Atmospheric Structure Equation for Grain Growth
- Catastrophic Evaporation of Rocky Planets
- The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age
- Impact of Clouds and Hazes on the Simulated JWST Transmission Spectra of Habitable Zone Planets in the TRAPPIST-1 System
- Heating efficiency in hydrogen-dominated upper atmospheres
- Planetary evolution with atmospheric photoevaporation I. Analytical derivation and numerical study of the evaporation valley and transition from super-Earths to sub-Neptunes
- Habitable Climate Scenarios for Proxima Centauri b With a Dynamic Ocean
- Aerosols in Exoplanet Atmospheres
- Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities. No excess of cold Jupiters in small planet systems
- Earth shaped by primordial H atmospheres
- Photoevaporation vs. core-powered mass-loss: model comparison with the 3D radius gap
- A secondary atmosphere on the rocky exoplanet 55 Cancri e
- Habitability of Terrestrial-Mass Planets in the HZ of M Dwarfs. I. H/He-Dominated Atmospheres
- Aeronomical constraints to the minimum mass and maximum radius of hot low-mass planets
- Grain opacity and the bulk composition of extrasolar planets. II. An analytical model for the grain opacity in protoplanetary atmospheres
- Carbon cycling and habitability of Earth-size stagnant lid planets
- Warm terrestrial planet with half the mass of Venus transiting a nearby star
- Retention of water in terrestrial magma oceans and carbon-rich early atmospheres
- Linking the evolution of terrestrial interiors and an early outgassed atmosphere to astrophysical observations
- Critical core mass for enriched envelopes: the role of H2O condensation
- Primary and secondary eclipse spectroscopy with JWST: exploring the exoplanet parameter space
- Redox evolution via gravitational differentiation on low mass planets: implications for abiotic oxygen, water loss and habitability
- The Case and Context for Atmospheric Methane as an Exoplanet Biosignature
- How cores grow by pebble accretion I. Direct core growth
- The Upper Atmospheres of Terrestrial Planets: Carbon Dioxide Cooling and the Earth's Thermospheric Evolution
- Sulphur dioxide in the mid-infrared transmission spectrum of WASP-39b
- Polarized reflected light from the exoplanet HD189733b: First multicolor observations and confirmation of detection
- First detection of polarized scattered light from an exoplanetary atmosphere
- Atmospheric effects of stellar cosmic rays on Earth-like exoplanets orbiting M-dwarfs
- Primordial Radius Gap and Potentially Broad Core Mass Distributions of Super-Earths and Sub-Neptunes
- Organic Haze as a Biosignature in Anoxic Earth-like Atmospheres
- Water Trapping on Tidally Locked Terrestrial Planets Requires Special Conditions
- Thermal mass loss of protoplanetary cores with hydrogen-dominated atmospheres: The influences of ionization and orbital distance
- Photochemistry of Anoxic Abiotic Habitable Planet Atmospheres: Impact of New HO Cross-Sections
- Testing exoplanet evaporation with multi-transiting systems
- Faint young Sun paradox remains
- What factors affect the duration and outgassing of the terrestrial magma ocean?
- Modeling pN2 through Geological Time: Implications for Planetary Climates and Atmospheric Biosignatures
- Climates of Warm Earth-like Planets I: 3-D Model Simulations
- The long-term evolution of the atmosphere of Venus: processes and feedback mechanisms
- The sub-Neptune desert and its dependence on stellar type: Controlled by lifetime X-ray irradiation
- A deep radius valley revealed by Kepler short cadence observations
- The habitable zone of Earth-like planets with different levels of atmospheric pressure
- Planet Formation Theory in the Era of ALMA and Kepler: from Pebbles to Exoplanets
- A warm or a cold early Earth? New insights from a 3-D climate-carbon model
- A Lower Limit of Atmospheric Pressure on Early Mars Inferred from Nitrogen and Argon Isotopic Compositions
- Detection of Ongoing Mass Loss from HD 63433c, a Young Mini Neptune
- From super-Earths to sub-Neptunes: Observational constraints and connections to theoretical models
- Escape and fractionation of volatiles and noble gases from Mars-sized planetary embryos and growing protoplanets
- Hydrodynamic simulations of captured protoatmospheres around Earth-like planets
- Exo-Planetary Transits of Limb Brightened Lines; Tentative Si IV Absorption by HD209458b
- Creating the Radius Gap without Mass Loss
- Water Partitioning in Planetary Embryos and Protoplanets with Magma Oceans
- Hydrodynamic escape of water vapor atmospheres near very active stars
- A fading radius valley towards M-dwarfs, a persistent density valley across stellar types
- Constraints on Metastable Helium in the Atmospheres of WASP-69b and WASP-52b with Ultra-Narrowband Photometry
- Measurements and semi-empirical calculations of CO2+CH4 and CO2+H2 collision-induced absorption across a wide range of wavelengths and temperatures. Application for the prediction of early Mars surface temperature
- Evidence for the volatile-rich composition of a 1.5- planet
- Survival of Terrestrial N2-O2 Atmospheres in Violent XUV Environments through Efficient Atomic Line Radiative Cooling
- Observability of Evaporating Lava Worlds
- Clouds and the Faint Young Sun Paradox
- Convective outgassing efficiency in planetary magma oceans: insights from computational fluid dynamics
- Solubility of water in peridotite liquids and the prevalence of steam atmospheres on rocky planets
- A Limited Habitable Zone for Complex Life
- Combined analysis of the 12.8 and 15 JWST/MIRI eclipse observations of TRAPPIST-1 b
- Loss and fractionation of noble gas isotopes and moderately volatile elements from planetary embryos and early Venus, Earth and Mars
- Carbonate-Silicate Cycle Predictions of Earth-like Planetary Climates and Testing the Habitable Zone Concept
- Was Venus Ever Habitable? Constraints from a Coupled Interior-Atmosphere-Redox Evolution Model
- Keck/NIRSPEC studies of He I in the atmospheres of two inflated hot gas giants orbiting K dwarfs: WASP-52b and WASP-177b
- The maximum mass of planetary embryos formed in core-accretion models
- The young Sun's XUV-activity as a constraint for lower CO-limits in the Earth's Archean atmosphere
- Habitability of Earth-like stagnant lid planets: Climate evolution and recovery from snowball states
- Growth and evolution of secondary volcanic atmospheres: I. Identifying the geological character of hot rocky planets
- The erosion of large primary atmospheres typically leaves behind substantial secondary atmospheres on temperate rocky planets
- Coupled Thermal and Compositional Evolution of Photo Evaporating Planet Envelopes
- The End of Runaway: How Gap Opening Limits the Final Masses of Gas Giants
- Cloud formation in metal-rich atmospheres of hot super-Earths like 55 Cnc e and CoRot7b
- Formation of Venus, Earth and Mars: Constrained by isotopes
- Carbon cycling and interior evolution of water-covered plate tectonics and stagnant lid planets
- Could Cirrus Clouds Have Warmed Early Mars?
- Atmospheric Erosion by Giant Impacts onto Terrestrial Planets
- Airy worlds or barren rocks? On the survivability of secondary atmospheres around the TRAPPIST-1 planets
- Effect of mantle oxidation state and escape upon the evolution of Earth's magma ocean atmosphere
- Circumpolar ocean stability on Mars 3 Gy ago
- Understanding planetary context to enable life detection on exoplanets and test the Copernican principle
- The Ice Cap Zone: A Unique Habitable Zone for Ocean Worlds
- Inner Super-Earths, Outer Gas Giants: How Pebble Isolation and Migration Feedback Keep Jupiters Cold
- A nitrogen-rich atmosphere on ancient Mars consistent with isotopic evolution models
- Waterworlds Probably Do Not Experience Magmatic Outgassing
- Less effective hydrodynamic escape of H-HO atmospheres on terrestrial planets orbiting pre-main sequence M dwarfs
- Life as the Only Reason for the Existence of N2-O2-Dominated Atmospheres
- Hot Rocks Survey I : A possible shallow eclipse for LHS 1478 b
- Impact degassing and atmospheric erosion on Venus, Earth, and Mars during the late accretion
- Synergies between Venus & Exoplanetary Observations
- Magma ocean evolution at arbitrary redox state
- Albedos, Equilibrium Temperatures, and Surface Temperatures of Habitable Planets
- Early habitability and crustal decarbonation of a stagnant-lid Venus
- Recycling of the first atmospheres of embedded planets: Dependence on core mass and optical depth
- Titania may produce abiotic oxygen atmospheres on habitable exoplanets
- Did Mars possess a dense atmosphere during the first ~400 million years?
- Coexistence of CH4, CO2 and H2O in exoplanet atmospheres
- Possible Atmospheric Diversity of Low Mass Exoplanets, some Central Aspects
- Unveiling the internal structure and formation history of the three planets transiting HIP 29442 (TOI-469) with CHEOPS
- Bioverse: The Habitable Zone Inner Edge Discontinuity as an Imprint of Runaway Greenhouse Climates on Exoplanet Demographics
- Hot Rocks Survey II: The thermal emission of TOI-1468 b reveals a hot bare rock
- Climate sensitivity to ozone and its relevance on the habitability of Earth-like planets
- Losing Oceans: The Effects of Composition on the Thermal Component of Impact-driven Atmospheric Loss
- Stability of Nitrogen in Planetary Atmospheres in Contact with Liquid Water
- Redox evolution of the crystallizing terrestrial magma ocean and its influence on atmosphere outgassing
- Volatile atmospheres of lava worlds
- Escape and evolution of Titan's N atmosphere constrained by N/N isotope ratios
- Redox state and interior structure control on the long-term habitability of stagnant-lid planets
- Sublimation of refractory minerals in the gas envelopes of accreting rocky planets
- Eta-Earth Revisited II: Deriving a Maximum Number of Earth-like Habitats in the Galactic Disk
- Modification of the radioactive heat budget of Earth-like exoplanets by the loss of primordial atmospheres
- Non-thermal escape of the Martian CO atmosphere over time: constrained by Ar isotopes
- Nitrogen Atmospheres of the Icy Bodies in the Solar System
- Evolution of HO Production in Comet C/2012 S1 (ISON) as Inferred from Forbidden Oxygen and OH Emission
- 3D simulations of the Archean Earth including photochemical haze profiles
- How planets form by pebble accretion V. Silicate rainout delays contraction of sub-Neptunes
- The evolution of catastrophically evaporating rocky planets
- Habitable Zone and Atmosphere Retention Distance (HaZARD) Stellar-evolution-dependent loss models of secondary atmospheres
- 3D simulations of TRAPPIST-1e with varying CO2, CH4 and haze profiles
- The Oxygen Bottleneck for Technospheres
- Characterisation of TOI-406 as showcase of the THIRSTEE program: A 2-planet system straddling the M-dwarf density gap
- Water versus land on temperate rocky planets
- A missing link in the nitrogen-rich organic chain on Titan
- A primordial radius valley as a consequence of planet formation
- Blowin' in the non-isothermal wind: core-powered mass loss with hydrodynamic radiative transfer
- Volatile-rich evolution of molten super-Earth L 98-59 d
- Implications of Abiotic Oxygen Buildup for Earth-like Complex Life
- Tracing the Snowball bifurcation of aquaplanets through time reveals a fundamental shift in critical-state dynamics
- The Roman coronagraph community participation program: observation planning
- Unraveling the non-equilibrium chemistry of the temperate sub-Neptune K2-18 b
- Variations in climate habitability parameters and their effect on Earth's biosphere during the Phanerozoic Eon
- From CO- to HO-dominated atmospheres and back -- How mixed outgassing changes the volatile distribution in magma oceans around M dwarf stars
- The atmospheres of rocky exoplanets III. Using atmospheric spectra to constrain surface rock composition
- Exoplanet Atmospheric Escape Observations with the Habitable Worlds Observatory
- Exoplanets synchronization in the habitable zone: Learning from Venus' retrograde rotation