Habitable Zones Around Main-Sequence Stars: New Estimates

Abstract

Identifying terrestrial planets in the habitable zones (HZs) of other stars is one of the primary goals of ongoing radial velocity and transit exoplanet surveys and proposed future space missions. Most current estimates of the boundaries of the HZ are based on 1-D, cloud-free, climate model calculations by Kasting et al.(1993). The inner edge of the HZ in Kasting et al.(1993) model was determined by loss of water, and the outer edge was determined by the maximum greenhouse provided by a CO2 atmosphere. A conservative estimate for the width of the HZ from this model in our Solar system is 0.95-1.67 AU. Here, an updated 1-D radiative-convective, cloud-free climate model is used to obtain new estimates for HZ widths around F, G, K and M stars. New H2O and CO2 absorption coefficients, derived from the HITRAN 2008 and HITEMP 2010 line-by-line databases, are important improvements to the climate model. According to the new model, the water loss (inner HZ) and maximum greenhouse (outer HZ) limits for our Solar System are at 0.99 AU and 1.70 AU, respectively, suggesting that the present Earth lies near the inner edge. Additional calculations are performed for stars with effective temperatures between 2600 K and 7200 K, and the results are presented in parametric form, making them easy to apply to actual stars. The new model indicates that, near the inner edge of the HZ, there is no clear distinction between runaway greenhouse and water loss limits for stars with T_{eff} ~< 5000 K which has implications for ongoing planet searches around K and M stars. To assess the potential habitability of extrasolar terrestrial planets, we propose using stellar flux incident on a planet rather than equilibrium temperature. Our model does not include the radiative effects of clouds; thus, the actual HZ boundaries may extend further in both directions than the estimates just given.

(updated version) Accepted to Astrophysical Journal. Additional references added. Typo in Water Rayleigh scattering expression corrected. An online habitable zone calculator (and a FORTRAN code) is available at the first author's website or at http://depts.washington.edu/naivpl/content/hz-calculator

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• Assessing the habitability of planets with Earth-like atmospheres with 1D and 3D climate modeling
• Effects of UV stellar spectral uncertainty on the chemistry of terrestrial atmospheres
• Hot Hydrogen Climates near the inner edge of the Habitable Zone
• Airy worlds or barren rocks? On the survivability of secondary atmospheres around the TRAPPIST-1 planets
• Dynamics of atmospheres with a non-dilute condensible component
• Constraining the Radiation and Plasma Environment of the Kepler Circumbinary Habitable Zone Planets
• Chasing rainbows and ocean glints: Inner working angle constraints for the Habitable Worlds Observatory
• Is the Pale Blue Dot unique? Optimized photometric bands for identifying Earth-like exoplanets
• Discovery of a Transiting Planet Near the Snow-Line
• The Impact of Stellar Distances on Habitable Zone Planets
• Exo-Milankovitch Cycles I: Orbits and Rotation States
• The CARMENES search for exoplanets around M dwarfs: The warm super-Earths in twin orbits around the mid-type M dwarfs Ross 1020 (GJ 3779) and LP 819-052 (GJ 1265)
• The SOPHIE search for northern extrasolar planets. X. Detection and characterization of giant planets by the dozen
• The habitability of stagnant-lid Earths around dwarf stars
• Enhanced Habitability on High Obliquity Bodies near the Outer Edge of the Habitable Zone of Sun-like Stars
• Circumpolar ocean stability on Mars 3 Gy ago
• Water Condensation Zones around Main Sequence Stars
• The impact of stripped cores on the frequency of Earth-size planets in the habitable zone
• Erosion of an exoplanetary atmosphere caused by stellar winds
• Formation and evolution of the two 4/3 resonant giants planets in HD 200946
• Discriminating Between Cloudy, Hazy and Clearsky Exoplanets Using Refraction
• The Demographics of Kepler's Earths and super-Earths into the Habitable Zone
• Effect of mantle oxidation state and escape upon the evolution of Earth's magma ocean atmosphere
• The contribution of the ARIEL space mission to the study of planetary formation
• Exoplanet Characterization by Proxy: a Transiting 2.15 R_Earth Planet Near the Habitable Zone of the Late K dwarf Kepler-61
• Planet Detectability in the Alpha Centauri System
• The Ice Cap Zone: A Unique Habitable Zone for Ocean Worlds
• HAZMAT. V. The Ultraviolet and X-ray Evolution of K Stars
• Conditions for water ice lines and Mars-mass exomoons around accreting super-Jovian planets at 1 - 20 AU from Sun-like stars
• The First Habitable Zone Earth-sized Planet from TESS. III: Climate States and Characterization Prospects for TOI-700 d
• The Fundamental Connections Between the Solar System and Exoplanetary Science
• The Pseudo-zodi Problem for Edge-on Planetary Systems
• The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc
• Absolute densities, masses, and radii of the WASP-47 system determined dynamically
• On the Detection of Exomoons Transiting Isolated Planetary-Mass Objects
• A Second Earth-Sized Planet in the Habitable Zone of the M Dwarf, TOI-700
• Lightning climatology of exoplanets and brown dwarfs guided by Solar System data
• Quantifying the Observational Effort Required for the Radial Velocity Characterization of TESS Planets
• Sulfate Aerosol Hazes and SO2 Gas as Constraints on Rocky Exoplanets' Surface Liquid Water
• Predicting the Yield of Potential Venus Analogs from TESS and their Potential for Atmospheric Characterization
• Transits of Known Planets Orbiting a Naked-Eye Star
• Surface Flux Patterns on Planets in Circumbinary Systems, and Potential for Photosynthesis
• Identifiable Acetylene Features Predicted for Young Earth-like Exoplanets with Reducing Atmospheres undergoing Heavy Bombardment
• Climate Modeling of a Potential ExoVenus
• Simulated Phase-dependent Spectra of Terrestrial Aquaplanets in M Dwarf Systems
• Gliese 49: Activity evolution and detection of a super-Earth
• The SOPHIE search for northern extrasolar planets XIII. Two planets around M-dwarfs Gl617A and Gl96
• Exomoon Habitability and Tidal Evolution in Low-Mass Star Systems
• Implications of atmospheric nondetections for Trappist-1 inner planets on atmospheric retention prospects for outer planets
• Evidence for at least three planet candidates orbiting HD20794
• Evaluating the Plausible Range of N2O Biosignatures on Exo-Earths: An Integrated Biogeochemical, Photochemical, and Spectral Modeling Approach
• Know the Planet, Know the Star: Precise Stellar Densities from Kepler Transit Light Curves
• Less effective hydrodynamic escape of H${}_2$-H${}_2$O atmospheres on terrestrial planets orbiting pre-main sequence M dwarfs
• A 1.55 R${}_{\oplus }$ habitable-zone planet hosted by TOI-715, an M4 star near the ecliptic South Pole
• Life as the Only Reason for the Existence of N2-O2-Dominated Atmospheres
• The CARMENES search for exoplanets around M dwarfs, Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star
• Milankovitch Cycles of Terrestrial Planets in Binary Star Systems
• Habitability and Water Loss Limits on Eccentric Planets Orbiting Main Sequence Stars
• GCM Simulations of Unstable Climates in the Habitable Zone
• Techniques for High-Contrast Imaging in Multi-Star Systems II: Multi-Star Wavefront Control
• Tracking Advanced Planetary Systems with HARPS-N (TAPAS). I. A multiple planetary system around the red giant star TYC 1422-614-1
• The MUSCLES Extension for Atmospheric and Transmission Spectroscopy: UV and X-ray Host-star Observations for JWST ERS & GTO Targets
• Hot Rocks Survey I : A possible shallow eclipse for LHS 1478 b
• Climates of Warm Earth-like Planets II: Rotational 'Goldilocks' Zones for Fractional Habitability and Silicate Weathering
• Synergies between Venus & Exoplanetary Observations
• Validation of small Kepler transiting planet candidates in or near the habitable zone
• The Demographics of Terrestrial Planets in the Venus Zone
• Evaporation of planetary atmospheres due to XUV illumination by quasars
• Beyond runaway: initiation of the post-runaway greenhouse state on rocky exoplanets
• The SOPHIE search for northern extrasolar planets. XI. Three new companions and an orbit update: Giant planets in the habitable zone
• Spin evolution of Earth-sized exoplanets, including atmospheric tides and core-mantle friction
• Terminator Habitability: the Case for Limited Water Availability on M-dwarf Planets
• Short duration high amplitude flares detected on the M dwarf star KIC 5474065
• Mineral dust increases the habitability of terrestrial planets but confounds biomarker detection
• The Abundance of Atmospheric CO2 in Ocean Exoplanets: A Novel CO2 Deposition Mechanism
• The test case of HD26965: difficulties disentangling weak Doppler signals from stellar activity
• Dependence of the onset of the runaway greenhouse effect on the latitudinal surface water distribution of Earth-like planets
• Why do we find ourselves around a yellow star instead of a red star?
• Magma ocean evolution at arbitrary redox state
• Two Small Temperate Planets Transiting Nearby M Dwarfs in K2 Campaigns 0 and 1
• Evryscope and K2 Constraints on TRAPPIST-1 Superflare Occurrence and Planetary Habitability
• Constraints on the structure of hot exozodiacal dust belts
• Early habitability and crustal decarbonation of a stagnant-lid Venus
• The quest for cradles of life: using the fundamental metallicity relation to hunt for the most habitable type of galaxy
• Linearized Flux Evolution (LiFE): A Technique for Rapidly Adapting Fluxes from Full-Physics Radiative Transfer Models
• The CARMENES search for exoplanets around M dwarfs. A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data
• Observational Signatures of Self-Destructive Civilisations
• Oxygenic photosynthetic responses of cyanobacteria exposed under an M-dwarf starlight simulator: Implications for exoplanet's habitability
• A search for technosignatures from TRAPPIST-1, LHS 1140, and 10 planetary systems in the Kepler field with the Green Bank Telescope at 1.15-1.73 GHz
• Long Term Planetary Habitability and the Carbonate-Silicate Cycle
• A New Method for Finding Nearby White Dwarf Exoplanets and Detecting Biosignatures
• Anatomy of rocky planets formed by rapid pebble accretion II. Differentiation by accretion energy and thermal blanketing
• Inefficient water degassing inhibits ocean formation on rocky planets: An insight from self-consistent mantle degassing models
• Detecting Proxima b's atmosphere with JWST targeting CO2 at 15 micron using a high-pass spectral filtering technique
• Realistic collisional water transport during terrestrial planet formation: Self-consistent modeling by an N-body--SPH hybrid code
• The K2-OjOS Project: New and revisited planets and candidates in K2 campaigns 5, 16, & 18
• Detectability of Chlorofluorocarbons in the Atmospheres of Habitable M-dwarf Planets
• Transit and Radial Velocity Survey Efficiency Comparison for a Habitable Zone Earth
• Red-edge position of habitable exoplanets around M-dwarfs
• Long-Term Stability of Tightly Packed Multi-Planet Systems in Prograde, Coplanar, Circumstellar Orbits within the $\alpha$ Centauri AB System
• Stellar & Planetary Parameters for K2's Late Type Dwarf Systems from C1 to C5
• Planetary formation and water delivery in the habitable zone around solar-type stars in different dynamical environments
• 3D convection-resolving model of temperate, tidally-locked exoplanets
• Finding the Needles in the Haystacks: High-Fidelity Models of the Modern and Archean Solar System for Simulating Exoplanet Observations
• Revised Exoplanet Radii and Habitability Using Gaia Data Release 2
• HAZMAT. VII. The Evolution of Ultraviolet Emission with Age and Rotation for Early M Dwarf Stars
• Clouds in the atmospheres of extrasolar planets. V. The impact of CO2 ice clouds on the outer boundary of the habitable zone
• Warming Early Mars with Climate Cycling: The Effect of CO2-H2 Collision-induced Absorption
• Abrupt climate transition of icy worlds from snowball to moist or runaway greenhouse
• Modeling Indications of Technology in Planetary Transit Light Curves -- Dark-side illumination
• Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions
• Recovering planet radial velocity signals in the presence of starspot activity in fully convective stars
• The role of planetary interior in the long-term evolution of atmospheric CO2 on Earth-like exoplanets
• Probing the capability of future direct imaging missions to spectrally constrain the frequency of Earth-like planets
• Obliquity Variations of Habitable Zone Planets Kepler-62f and Kepler-186f
• Kepler-539: a young extrasolar system with two giant planets on wide orbits and in gravitational interaction
• Possible Atmospheric Diversity of Low Mass Exoplanets, some Central Aspects
• ExoPlaSim: Extending the Planet Simulator for Exoplanets
• Asteroid flux towards circumprimary habitable zones in binary star systems: I. Statistical Overview
• Target Selection for the LBTI Exozodi Key Science Program
• In Search of Future Earths: Assessing the possibility of finding Earth analogues in the later stages of their habitable lifetimes
• Changing spatial distribution of water flow charts major change in Mars' greenhouse effect
• Stellar Flares versus Luminosity: XUV-induced Atmospheric Escape and Planetary Habitability
• An upper limit on the ratio between the Extreme Ultraviolet and the bolometric luminosities of stars hosting habitable planets
• Atmospheric Dynamics on Terrestrial Planets: The Seasonal Response to changes in Orbital, Rotational and Radiative Timescales
• Rotational Synchronization May Enhance Habitability for Circumbinary Planets: Kepler Binary Case Studies
• Runaway climate cooling of ocean planets in the habitable zone: a consequence of seafloor weathering enhanced by melting of high-pressure ice
• Transit least-squares survey -- II. Discovery and validation of 17 new sub- to super-Earth-sized planets in multi-planet systems from K2
• A Habitable-Zone Earth-Sized Planet Rescued from False Positive Status
• Wavefront sensing and control in space-based coronagraph instruments using Zernike's phase-contrast method
• The CARMENES search for exoplanets around M dwarfs. Two terrestrial planets orbiting G 264-012 and one terrestrial planet orbiting Gl 393
• The Need for Laboratory Work to Aid in The Understanding of Exoplanetary Atmospheres
• Dynamics and habitability in circumstellar planetary systems of known binary stars
• The ultraviolet habitable zone of exoplanets
• JWST-TST DREAMS: NIRSpec/PRISM Transmission Spectroscopy of the Habitable Zone Planet TRAPPIST-1 e
• Planetary system around LTT 1445A unveiled by ESPRESSO: Multiple planets in a triple M-dwarf system
• TESS observations of flares and quasi-periodic pulsations from low mass stars and potential impact on exoplanets
• Efficiency of the oxygenic photosynthesis on Earth-like planets in the habitable zone
• Evolution and Spectral Response of a Steam Atmosphere for Early Earth with a coupled climate-interior model
• The CARMENES search for exoplanets around M dwarfs. Dynamical characterization of the multiple planet system GJ 1148 and prospects of habitable exomoons around GJ 1148 b
• Super Earths and Dynamical Stability of Planetary Systems: First Parallel GPU Simulations Using GENGA
• Lithologic Controls on Silicate Weathering Regimes of Temperate Planets
• Bridging the Planet Radius Valley: Stellar Clustering as a Key Driver for Turning Sub-Neptunes into Super-Earths
• Panspermia in a Milky Way-like Galaxy
• HADES RV program with HARPS-N at TNG. IX. A super-Earth around the M dwarf Gl686
• Bioverse: The Habitable Zone Inner Edge Discontinuity as an Imprint of Runaway Greenhouse Climates on Exoplanet Demographics
• Reduced late bombardment on rocky exoplanets around M-dwarfs
• Worlds Without Moons: Exomoon Constraints for Compact Planetary Systems
• Simulating radio emission from Low Mass Stars
• Lightning-induced chemistry on tidally-locked Earth-like exoplanets
• The KOBE experiment: K-dwarfs Orbited By habitable Exoplanets. Project goals, target selection and stellar characterization
• Effect of the exoplanet magnetic field topology on its magnetospheric radio emission
• The CARMENES search for exoplanets around M dwarfs: Spectroscopic orbits of nine M-dwarf multiple systems, including two triples, two brown dwarf candidates, and one close M-dwarf-white dwarf binary
• The Effect of Planetary Illumination on Climate Modelling of Earthlike Exomoons
• The peak absorbance wavelength of photosynthetic pigments around other stars from spectral optimization
• TESS Habitable Zone Star Catalog
• Effects of Radius and Gravity on the Inner Edge of the Habitable Zone
• JWST-TST DREAMS: Secondary Atmosphere Constraints for the Habitable Zone Planet TRAPPIST-1 e
• SPECULOOS exoplanet search and its prototype on TRAPPIST
• Estimating precipitation on early Mars using a radiative-convective model of the atmosphere and comparison with inferred runoff from geomorphology
• Potential long-term habitable conditions on planets with primordial H-He atmospheres
• Role of gaseous giants in the dynamical evolution of terrestrial planets and water delivery in the habitable zone
• Sensitive Multi-beam Targeted SETI Observations towards 33 Exoplanet Systems with FAST
• Exomoon Climate Models with the Carbonate-Silicate Cycle and Viscoelastic Tidal Heating
• Internal Structure and CO${}_2$ Reservoirs of Habitable Water-Worlds
• Giant planets: good neighbors for habitable worlds?
• Circumbinary Habitability Niches
• The CARMENES search for exoplanets around M dwarfs - The enigmatic planetary system GJ 4276: One eccentric planet or two planets in a 2:1 resonance?
• Two super-Earths at the edge of the habitable zone of the nearby M dwarf TOI-2095
• Role of stellar physics in regulating the critical steps for life
• Brown Dwarf Atmospheres as the Potentially Most Detectable and Abundant Sites for Life
• Climate sensitivity to ozone and its relevance on the habitability of Earth-like planets
• Quantifying the Influence of Jupiter on the Earth's Orbital Cycles
• Large Interferometer For Exoplanets (LIFE): IV. Ideal kernel-nulling array architectures for a space-based mid-infrared nulling interferometer
• Bioverse: a simulation framework to assess the statistical power of future biosignature surveys
• Assessing $TESS$'s Yield of Rocky Planets Around Nearby M Dwarfs
• In the Presence of a Wrecking Ball: Orbital Stability in the HR 5183 System
• Evolution of galaxy habitability
• Quantitative estimates of the surface habitability of Kepler-452b
• From climate models to planetary habitability: temperature constraints for complex life
• Habitable planet formation around low-mass stars: Rapid accretion, rapid debris removal and the essential contribution of external giants
• Radio masers on WX UMa: hints of a Neptune-sized planet, or magnetospheric reconnection?
• An extremely low-density and temperate giant exoplanet
• Planetary Magnetism as a Parameter in Exoplanet Habitability
• On the Orbital Inclination of Proxima Centauri b
• Transit Visibility Zones of the Solar System Planets
• Geothermal heating enhances atmospheric asymmetries on synchronously rotating planets
• The Effect of Land Fraction and Host Star Spectral Energy Distribution on the Planetary Albedo of Terrestrial Worlds
• Large Interferometer For Exoplanets (LIFE): IX. Assessing the Impact of Clouds on Atmospheric Retrievals at Mid-Infrared Wavelengths with a Venus-Twin Exoplanet
• How surfaces shape the climate of habitable exoplanets
• Transit Detection of a "Starshade" at the Inner Lagrange Point of an Exoplanet
• Dynamical Packing in the Habitable Zone: The Case of Beta CVn
• Transits of extrasolar moons around luminous giant planets
• TOI-4010: A System of Three Large Short-Period Planets With a Massive Long-Period Companion
• Stellar Activity Effects on Moist Habitable Terrestrial Atmospheres Around M dwarfs
• SPECULOOS: a network of robotic telescopes to hunt for terrestrial planets around the nearest ultracool dwarfs
• HADES RV Programme with HARPS-N at TNG VI. GJ 3942 b behind dominant activity signals
• MHD study of extreme space weather conditions for exoplanets with Earth-like magnetospheres: On habitability conditions and radio-emission
• Planetary parameters, XUV environments and mass-loss rates for nearby gaseous planets with X-ray detected host-stars
• An Integrated Analysis with Predictions on the Architecture of the tau Ceti Planetary System, Including a Habitable Zone Planet
• A quarter century of spectroscopic monitoring of the nearby M dwarf Gl 514. A super-Earth on an eccentric orbit moving in and out of the habitable zone
• Impact of ηearth on the capabilities of affordable space missions to detect biosignatures on extrasolar planets
• How does the background atmosphere affect the onset of the runaway greenhouse ?
• Evolution of the habitable zone of low-mass stars. Detailed stellar models and analytical relationships for different masses and chemical compositions
• The CARMENES search for exoplanets around M dwarfs. A super-Earth planet orbiting HD 79211 (GJ 338 B)
• The SOPHIE search for northern extrasolar planets-XIX. A system including a cold sub-Neptune potentially transiting a V = 6.5 star HD88986
• HAZMAT. IX. An Analysis of the UV and X-Ray Evolution of Low-Mass Stars in the Era of Gaia
• On the Inclination and Habitability of the HD 10180 System
• A Catalog of Stellar Evolution Profiles and the Effects of Variable Composition on Habitable Systems
• Rapid Water Loss can Extend the Lifetime of the Planetary Habitability
• Impact of Tides on the Potential for Exoplanets to Host Exomoons
• Convective shutdown in the atmospheres of lava worlds
• Planet occurrence rate density models including stellar effective temperature
• Stellar atmospheric parameters of FGK-type stars from high-resolution optical and near-infrared CARMENES spectra
• Thermal-orbital coupled tidal heating and habitability of Martian-sized extrasolar planets around M stars
• Biofluorescent Worlds I: Global Biological Fluorescence as a Biosignature
• Modelling the Inner Debris Disc of HR 8799
• Optimal Measures for Characterizing Water-rich Super-Earths
• Statistical-likelihood Exo-Planetary Habitability Index (SEPHI)
• Comparative Climates of TRAPPIST-1 planetary system: results from a simple climate-vegetation model
• The CARMENES search for exoplanets around M dwarfs Detection of a mini-Neptune around LSPM J2116+0234 and refinement of orbital parameters of a super-Earth around GJ 686 (BD+18 3421)
• Predicting multiple planet stability and habitable zone companions in the TESS era
• TOI 122b and TOI 237b, two small warm planets orbiting inactive M dwarfs, found by \textit{TESS}
• Atmospheric Dynamics of a Near Tidally Locked Earth-Size Planet
• Predicting the Yield of Small Transiting Exoplanets around Mid-M and Ultra-Cool Dwarfs in the Nancy Grace Roman Space Telescope Galactic Bulge Time Domain Survey
• Multibeam Blind Search of Targeted SETI Observations toward 33 Exoplanet Systems with FAST
• Interior Controls on the Habitability of Rocky Planets
• GCM Constraints on the Detectability of the CO${}_2$-CH${}_4$ Biosignature Pair on TRAPPIST-1e with JWST
• Robust asteroseismic properties of the bright planet host HD 38529
• The best place and time to live in the Milky Way
• Planetary candidates transiting cool dwarf stars from Campaigns 12 to 15 of K2
• Climate Diversity in the Solar-Like Habitable Zone due to Varying Background Gas Pressure
• The HADES RV Programme with HARPS-N at TNG XI. GJ 685 b: a warm super-Earth around an active M dwarf
• Transiting planet candidate from K2 with the longest period
• Prospects of detecting the polarimetric signature of the Earth-mass planet alpha Centauri B b with SPHERE / ZIMPOL
• Testing Earth-like atmospheric evolution on exo-Earths through oxygen absorption: required sample sizes and the advantage of age-based target selection
• Direct Imaging of Exoplanets Beyond the Radial Velocity Limit: Application to the HD 134987 System
• A New Line-By-Line General Circulation Model for Simulations of Diverse Planetary Atmospheres: Initial Validation and Application to the Exoplanet GJ 1132b
• Obliquity Evolution of the Potentially Habitable Exoplanet Kepler-62f
• The Chaotic Nature of TRAPPIST-1 Planetary Spin States
• Atmospheric circulation, chemistry, and infrared spectra of Titan-like exoplanets around different stellar types
• Earth as an Exoplanet. II. Earth's Time-variable Thermal Emission and Its Atmospheric Seasonality of Bioindicators
• The SOPHIE search for northern extrasolar planets - XII. Three giant planets suitable for astrometric mass determination with Gaia
• The effect of high nitrogen pressures on the habitable zone and an appraisal of greenhouse states
• Hierarchical Bayesian Atmospheric Retrieval Modeling for Population Studies of Exoplanet Atmospheres: A Case Study on the Habitable Zone
• A population-based Habitable Zone perspective
• On the radial velocity detection of additional planets in transiting, slowly rotating M-dwarf systems: the case of GJ 1132
• Atmospheric Evolution on Low-gravity Waterworlds
• In Situ Models for Planet Assembly around Cool stars
• A Comprehensive Characterization of the 70 Virginis Planetary System
• Solar Contamination in Extreme Precision Radial Velocity Measurements: Deleterious Effects and Prospects for Mitigation
• Large closed-field corona of WX UMa evidenced from radio observations
• Interstellar communication network. I. Overview and assumptions
• Habitable Zone Boundaries for Circumbinary Planets
• Constraining the magnitude of climate extremes from time-varying instellation on a circumbinary terrestrial planet
• Using HARPS-N to characterise the long-period planets in the PH-2 and Kepler-103 systems
• Atmospheric stability and collapse on tidally locked rocky planets
• How to Directly Image a Habitable Planet Around Alpha Centauri with a ~30-45cm Space Telescope
• 3D orbital architecture of a dwarf binary system and its planetary companion
• Habitability properties of circumbinary planets
• Eta-Earth Revisited II: Deriving a Maximum Number of Earth-like Habitats in the Galactic Disk
• Predictions of planet detections with near infrared radial velocities in the up-coming SPIRou Legacy Survey-Planet Search
• Formation of Solar system analogues II: post-gas phase growth and water accretion in extended discs via N-body simulations
• Can Moons Have Moons?
• Photometric rotation periods for 107 M dwarfs from the APACHE survey
• Two Planets Straddling the Habitable Zone of The Nearby K Dwarf Gl 414A
• GJ 3929: High Precision Photometric and Doppler Characterization of an Exo-Venus and its Hot, Mini-Neptune-mass Companion
• In the crosshair: astrometric exoplanet detection with WFIRST's diffraction spikes
• Characterization of the Wolf 1061 Planetary System
• Atmospheric dynamics on terrestrial planets with eccentric orbits
• The Cosmic Shoreline Revisited: A Metric for Atmospheric Retention Informed by Hydrodynamic Escape
• Which type of planets do we expect to observe in the Habitable Zone?
• Thermal and orbital evolution of low-mass exoplanets
• Interior-atmosphere modelling to assess the observability of rocky planets with JWST
• A Flexible Bayesian Framework for Assessing Habitability with Joint Observational and Model Constraints
• H${}_2$O${}_2$-induced Greenhouse Warming on Oxidized Early Mars
• The Demographics of Exoplanets
• Colliding Winds in Low-Mass Binary Star Systems: wind interactions and implications for habitable planets
• EOS-ESTM: A flexible climate model for habitable exoplanets
• Relative abundances of CO2, CO, and CH4 in atmospheres of Earth-like lifeless planets
• Lyman-$\alpha$ Observations of High Radial Velocity Low-Mass Stars Ross 1044 and Ross 825
• Where to Find Habitable "Earths" in Circumbinary Systems
• Minimal conditions for survival of technological civilizations in the face of stellar evolution
• The GAPS Programme with HARPS-N@TNG XII: Characterization of the planetary system around HD108874
• Stellar Parameters for HD 69830, a Nearby Star with Three Neptune Mass Planets and an Asteroid Belt
• Atmospheres and UV Environments of Earth-like Planets Throughout Post-Main Sequence Evolution
• Migrating Jupiter up to the habitable zone: Earth-like planet formation and water delivery
• The GALAH Survey: Using Galactic Archaeology to Refine our Knowledge of TESS Target Stars
• Aquaplanet Models on Eccentric Orbits: Effects of Rotation Rate on Observables
• S-Type and P-Type Habitability in Stellar Binary Systems: A Comprehensive Approach III. Results for Mars, Earth, and super-Earth Planets
• Habitable zones around almost extremely spinning black holes (black sun revisited)
• Evolution of steam worlds: energetic aspects
• Confirmation of the Long-Period Planet Orbiting Gliese 411 and the Detection of a New Planet Candidate
• Constraining exoplanet interiors using observations of their atmospheres
• Photosynthetic Potential of Planets in 3:2 Spin Orbit Resonances
• Habitable Zone and Atmosphere Retention Distance (HaZARD) Stellar-evolution-dependent loss models of secondary atmospheres
• EDEN Survey: Small Transiting Planet Detection Limits and Constraints on the Occurrence Rates for Late M Dwarfs within 15 pc
• Radial velocity homogeneous analysis of M dwarfs observed with HARPS I. Exoplanet detection and candidates
• Habitability in the Omega Centauri Cluster
• The energetic particle environment of a GJ 436 b-like planet
• Prospects for water vapor detection in the atmospheres of temperate and arid rocky exoplanets around M-dwarf stars
• Observability of hydrogen-rich exospheres in Earth-like exoplanets
• Electric sails are potentially more effective than light sails near most stars
• The Terrestrial Planet Formation around M Dwarfs: In-situ, Inward Migration or Reversed Migration
• HADES RV Programme with HARPS-N at TNG XIII. A sub-Neptune around the M dwarf GJ 720 A
• How likely are Snowball episodes near the inner edge of the habitable zone?
• Does the evolution of complex life depend on the stellar spectral energy distribution?
• Multiverse Predictions for Habitability: Number of Potentially Habitable Planets
• First exploration of the runaway greenhouse transition with a GCM
• Self-limited tidal heating and prolonged magma oceans in the L 98-59 system
• Exploring exomoon atmospheres with an idealized general circulation model
• Role of Planetary Radius on Atmospheric Escape of Rocky Exoplanets
• Impact of M-dwarf Stellar Wind and Photoevaporation on the Atmospheric Evolution of Small Planets
• Can comets deliver prebiotic molecules to rocky exoplanets?
• The TESS Triple-9 Catalog II: a new set of 999 uniformly-vetted exoplanet candidates
• Habitability and sub glacial liquid water on planets of M-dwarf stars
• A Bayesian Analysis of Technological Intelligence in Land and Oceans
• Excitation Properties of Photopigments and Their Possible Dependence on the Host Star
• Sensitivity of the Roman Coronagraph Instrument to Exozodiacal Dust
• An Energy Balance Model for Rapidly and Synchronously Rotating Terrestrial Planets
• Climate Sensitivity to Carbon Dioxide and Moist Greenhouse threshold of Earth-like planets under an increasing solar forcing
• A Method to Identify the Boundary Between Rocky and Gaseous Exoplanets from Tidal Theory and Transit Durations
• The high-energy radiation environment of the habitable-zone super-Earth LHS 1140b
• The GAPS Programme at TNG -- XXIV. An eccentric Neptune-mass planet near the inner edge of the BD-11 4672 habitable zone
• A New Definition of Exoplanet Habitability: Introducing the Photosynthetic Habitable Zone
• A Framework for Relative Biosignature Yields from Future Direct Imaging Missions
• High pCO${}_2$ reduces sensitivity to CO${}_2$ perturbations on temperate, Earth-like planets throughout most of habitable zone
• Expanding the Catalog: Considering the Importance of Carbon, Magnesium, and Neon in the Evolution of Stars and Habitable Zones
• A review of planetary systems around HD 99492, HD 147379 and HD 190007 with HARPS-N
• Direct Imaging in the Habitable Zone and the Problem of Orbital Motion
• The CARMENES search for exoplanets around M dwarfs. Revisiting the GJ 581 multi-planetary system with new Doppler measurements from CARMENES, HARPS, and HIRES
• 3D simulations of TRAPPIST-1e with varying CO2, CH4 and haze profiles
• Direct imaging of exoplanets in the habitable zone with adaptive optics
• CO${}_2$ ocean bistability on terrestrial exoplanets
• A Multi-Year Search For Transits Of Proxima Centauri. I: Light Curves Corresponding To Published Ephemerides
• Simulations of starspot anomalies within TESS exoplanetary transit light curves -- I. The detection limits of starspot anomalies in TESS light curves
• Terrestrial-type planet formation: Comparing different types of initial conditions
• The influence of surface $C{O}_2$ condensation on the evolution of warm and cold rocky planets orbiting Sun-like stars
• HWO Yield Sensitivities in the NIR and NUV
• Earth as an Exoplanet. III. Using Empirical Thermal Emission Spectra as an Input for Atmospheric Retrieval of an Earth-twin Exoplanet
• Prospects for Life on Temperate Planets Around Brown Dwarfs
• Three small transiting planets around the M dwarf host star LP 358-499
• The Dark Planets of the WASP-47 Planetary System
• K2-HERMES II. Planet-candidate properties from K2 Campaigns 1-13
• A Geologically Robust Procedure For Observing Rocky Exoplanets to Ensure that Detection of Atmospheric Oxygen is an Earth-Like Biosignature
• Statistical properties of habitable zones in stellar binary systems
• Stellar X-ray activity and habitability revealed by ROSAT sky survey
• Tidal and general relativistic effects in rocky planet formation at the substellar mass limit using N-body simulations
• Prospects for detecting the Rossiter-McLaughlin effect of Earth-like planets: the test case of TRAPPIST-1b and c
• Milankovitch Cycles for a Circumstellar Earth-analog within $\alpha$ Centauri-like Binaries
• TOI-712: a system of adolescent mini-Neptunes extending to the habitable zone
• Physical properties of terrestrial planets and water delivery in the habitable zone using N-body simulations with fragmentation
• High-Resolution Spectral Discriminants of Ocean Loss for M Dwarf Terrestrial Exoplanets
• Gravitational Microlensing Events as a Target for SETI project
• EOS: Atmospheric Radiative Transfer in Habitable Worlds with HELIOS
• Intermittent Signals and Planetary Days in SETI
• Sensitivity to habitable planets in the \textit{Roman} microlensing survey
• HD 83443c: A highly eccentric giant planet on a 22-year orbit
• The Solar Neighborhood LI: A Variability Survey of Nearby M Dwarfs with Planets from Months to Decades with TESS and the CTIO/SMARTS 0.9 m Telescope
• An Integrative Analysis of the HD 219134 Planetary System and the Inner Solar System: Extending DYNAMITE with Enhanced Orbital Dynamical Stability Criteria
• Consequences of dynamically unstable moons in extrasolar systems
• Inner Habitable Zone Boundary for Eccentric Exoplanets
• An Integrative Analysis of the Rich Planetary System of the Nearby Star e Eridani: Ideal Targets For Exoplanet Imaging and Biosignature Searches
• The Role of Atmospheric Exchange in False-Positive Biosignature Detection
• A Unified Spectroscopic and Photometric Model to Infer Surface Inhomogeneity: Application to Luhman 16B
• The Abundance of Belatedly Habitable Planets and Ambiguities in Definitions of the Continuously Habitable Zone
• Mapping the Skies of Ultracool Worlds: Detecting Storms and Spots with Extremely Large Telescopes
• The Effect of Seafloor Weathering on Planetary Habitability
• Tidally driven tectonic activity as a parameter in exoplanet habitability
• Pursuing Truth: Improving Retrievals on Mid-Infrared Exo-Earth Spectra with Physically Motivated Water Abundance Profiles and Cloud Models
• CHEOPS observations of TESS primary mission monotransits
• TOI-4336 A b: A temperate sub-Neptune ripe for atmospheric characterization in a nearby triple M-dwarf system
• The independent discovery of planet candidates around low mass stars and astrophysical false positives from the first two TESS sectors
• Aliasing in the Radial Velocities of YZ Ceti: An Ultra-Short Period for YZ Ceti c?
• The Habitable Zones of Rapidly Rotating Main Sequence A/F Stars
• Exoplanetary Detection By Multifractal Spectral Analysis
• Climate of high obliquity exo-terrestrial planets with a three-dimensional cloud system resolving climate model
• Spin-driven tidal pumping: Tidally driven changes in planetary spin coupled with secular interactions between planets
• Exoplanet Exergy: Why useful work matters for planetary habitabilty
• Three direct imaging epochs could constrain the orbit of Earth 2.0 inside the habitable zone
• Effects of a Binary Companion Star on Habitability of Tidally Locked Planets around an M-type Host Star
• Estimating Planetary Mass with Deep Learning
• Improved Analysis of Clarke Exobelt Detectability
• Exploring Climate with Obliquity in a Variable-eccentricity Earth-like World
• Transit least-squares survey -- III. A $1.9R_{\oplus }$ transit candidate in the habitable zone of Kepler-160 and a nontransiting planet characterized by transit-timing variations
• Fiber mode scrambler for the Subaru infrared Doppler instrument (IRD)
• The influence of orbital resonances on the water transport to objects in the circumprimary habitable zone of binary star systems
• Earth: Atmospheric Evolution of a Habitable Planet
• The GAPS programme at TNG. XLVI. Deep search for low-mass planets in late-dwarf systems hosting cold Jupiters
• Tidal decay of circumbinary planetary systems
• Effects of Proxima Centauri on Planet Formation in Alpha Centauri
• Carbon cycle instability for high-$\mathrm{C}{\mathrm{O}}_2$ exoplanets: Implications for habitability
• Properties of a Previously Unidentified Instrumental Signature in $\text{Kepler/K2}$ that was Confused for AGN Variability
• Characteristics of aquatic biospheres on temperate planets around Sun-like stars and M-dwarfs
• Fourth-order Coronagraph for High-Contrast Imaging of Exoplanets with Off-axis Segmented Telescopes
• A limbus mundi elucidation of habitability: the Goldilocks Edge
• Potential Interior Structures and Habitability of Super-Earth Exoplanets LHS 1140 b, K2-18 b, TOI-1452 b and TOI-1468 c
• Tracing the Inner Edge of the Habitable Zone with Sulfur Chemistry
• Effect of vegetation on the temperatures of Trappist-1 planets
• The Habitable Zone of Kepler-16: Impact of Binarity and Climate Models
• A Statistical Comparative Planetology Approach to Maximize the Scientific Return of Future Exoplanet Characterization Efforts
• On the enlargement of habitable zones around binary stars in hostile environments
• Identifying Exo-Earth Candidates in Direct Imaging Data through Bayesian Classification
• Gas disk interactions, tides and relativistic effects in the rocky planet formation at the substellar mass limit
• HD 163296 and its Giant Planets: Creation of Exo-comets, Interstellar Objects and Transport of Volatile Material
• Climatological and UV-based Habitability of Possible Exomoons in F-star Systems
• The escape of hydrogen-rich atmosphere of exoplanet: Mass loss rates and the absorptions of stellar Lyman $\alpha$
• Potential for life to exist and be detected on Earth-like planets orbiting white dwarfs
• KOBE-1: The first planetary system from the KOBE survey. Two planets likely residing in the sub-Neptune mass regime around a late K-dwarf
• Tidal evolution of Earth-like planets in the habitable zone of low-mass stars
• Setting the Stage for Habitable Planets
• Asteroid flux towards circumprimary habitable zones in binary star systems: II. Dynamics
• The GALAH Survey: Improving our understanding of confirmed and candidate planetary systems with large stellar surveys
• Space telescope design to directly image the habitable zone of Alpha Centauri
• Effects of Flux Variation on the Surface Temperatures of Earth-like Circumbinary Planets
• Updated Studies on Exomoons in the HD 23079 System
• Close stellar encounters kicking planets out of habitable zone in various stellar environments
• Enlarging habitable zones around binary stars in hostile environments
• Fitting Formulae and Constraints for the Existence of S-type and P-type Habitable Zones
• The CARMENES search for exoplanets around M dwarfs. A sub-Neptunian mass planet in the habitable zone of HN Lib
• A transiting super-Earth close to the inner edge of the habitable zone of an M0 dwarf star
• The Direct Mid-Infrared Detectability of Habitable-zone Exoplanets Around Nearby Stars
• TRAPPIST-1h as an Exo-Titan. I. The Role of Assumptions about Atmospheric Parameters in Understanding an Exoplanet Atmosphere
• Orbital evolution of potentially habitable planets of tidally interacting binary stars
• X-ray variability of the triplet star system LTT1445 and evaporation history of the exoplanets around its A component
• Planet Earth in reflected and polarized light: II. Refining contrast estimates for rocky exoplanets with ELT and HWO
• Characterization of Low Mass K2 Planet Hosts Using Near-Infrared Spectroscopy
• Absence of a Runaway Greenhouse Limit on Lava Planets
• Development of the SPECULOOS exoplanet search project
• HADES RV programme with HARPS-N at TNG XIV. A candidate super-Earth orbiting the M-dwarf GJ 9689 with a period close to half the stellar rotation period
• Internal Structure and Magnetic Moment of Rocky Planets. Application to the first exoplanets discovered by TESS
• Around which stars can TESS detect Earth-like planets? The Revised TESS Habitable Zone Catalog
• A Transiting Giant on a 7.7-Year Orbit Revealed by TTVs in the TOI-201 System
• Delivery of icy planetesimals to inner planets in the Proxima Centauri planetary system
• An unusual reservoir of water emission in the VV CrA A protoplanetary disk
• Using Kepler Candidates to Examine the Properties of Habitable Zone Exoplanets
• The role of dynamics on the habitability of an Earth-like planet
• Impact of Planetary Parameters on Water Clouds Microphysics
• Exocomets in the 47 UMa System: Theoretical Simulations including Water Transport
• The Featureless HST/WFC3 Transmission Spectrum of the Rocky Exoplanet GJ 1132b: No Evidence For A Cloud-Free Primordial Atmosphere and Constraints on Starspot Contamination
• Controls of Atmospheric Methane on Early Earth and Inhabited Earth-like Terrestrial Exoplanets
• Can Planets Exist in the Habitable Zone of 55~Cancri?
• A New Planet in the Kepler-159 System From Transit Timing Variations
• The Importance of 3D General Circulation Models for Characterizing the Climate and Habitability of Terrestrial Extrasolar Planets
• Photobombing Earth 2.0: Diffraction Limit Related Contamination and Uncertainty in Habitable Planet Spectra
• New Dynamical State and Habitability of the HD 45364 Planetary System
• Convection and Clouds under Different Planetary Gravities Simulated by a Small-domain Cloud-resolving Model
• The time evolution of the ultraviolet habitable zone
• The Potential of Detecting Nearby Terrestrial Planets in the HZ with Different Methods
• Meta-modelling the climate of dry tide locked rocky planets
• Greenhouse warming potential of a suite of gas species on early Mars evaluated using a radiative-convective climate model
• A One-Dimensional Energy Balance Model Parameterization for the Formation of CO2 Ice on the Surfaces of Eccentric Extrasolar Planets
• Characterizing planetary systems with SPIRou: a temperate sub-Neptune exoplanet orbiting the nearby fully-convective star GJ 1289 and a candidate around GJ 3378
• 3D Global climate model of an exo-Venus: a modern Venus-like atmosphere for the nearby super-Earth LP 890-9 c
• Combining Photometry and Astrometry to Improve Orbit Retrieval of Directly Imaged Exoplanets
• Plausibility of Capture into High-Obliquity States for Exoplanets in the M Dwarf Habitable Zone
• Characterization of transiting exoplanets by way of differential photometry
• Relative Habitability of Exoplanet Systems with Two Giant Planets
• A rocky exoplanet classification method and its application to calculating surface pressure and surface temperature
• Effect of multiple scattering on the Transmission spectra and the Polarization phase curves for Earth-like Exoplanets
• Tides Tighten the Hycean Habitable Zone
• Planetary host stars: Evaluating uncertainties in ultra-cool model atmospheres
• A systematic study of \ce{CO2} planetary atmospheres and their link to the stellar environment
• Dead Zones of Classical Habitability in Stellar Binary Systems
• Three-dimensional Transport-induced Chemistry on Temperate sub-Neptune K2-18b, Part I: the Effects of Atmospheric Dynamics
• Empirical Predictions for the Period Distribution of Planets to be Discovered by the Transiting Exoplanet Survey Satellite
• Baseline Requirements For Detecting Biosignatures with the HabEx and LUVOIR Mission Concepts
• Exoplanets Around Red Giants: Distribution and Habitability
• Artificial Greenhouse Gases as Exoplanet Technosignatures
• A Readily Implemented Atmosphere Sustainability Constraint for Terrestrial Exoplanets Orbiting Magnetically Active Stars
• Probing the Limits of Habitability: A Catalog of Rocky Exoplanets in the Habitable Zone
• The GAPS Programme at TNG -- XXIII. HD 164922 d: a close-in super-Earth discovered with HARPS-N in a system with a long-period Saturn mass companion
• On the formation of terrestrial planets between two massive planets: The case of 55 Cancri
• Characterization of low-mass companions to $\text{Kepler}$ objects of interest observed with APOGEE-N
• Hot Earth or Young Venus? A nearby transiting rocky planet mystery
• L 363-38 b: a planet newly discovered with ESPRESSO orbiting a nearby M dwarf star
• SHAMPOO: A stochastic model for tracking dust particles under the influence of non-local disk processes
• The Most Common Habitable Planets II -- Salty Oceans in Low Mass Habitable Planets and Global Climate Evolution
• Constraints on Evolutionary Timescales for M Dwarf Planets from Dynamical Stability Arguments
• From CO${}_2$- to H${}_2$O-dominated atmospheres and back -- How mixed outgassing changes the volatile distribution in magma oceans around M dwarf stars
• Galactic settlement of low-mass stars as a resolution to the Fermi paradox
• Dynamical evolution and stability maps of the Proxima Centauri system
• Is the high-energy environment of K2-18b special?
• A Venus in the Making? Predictions for JWST Observations of the Ultracool M-Dwarf planet LP 890-9 c
• The Formation of Habitable Planets in the Four-Planet System HD 141399
• Water worlds in N-body simulations with fragmentation in systems without gaseous giants
• A Consistent Orbital Stability Analysis for the GJ 581 System
• Exoplanets: Possible Biosignatures
• The DRAKE mission: finding the frequency of life in the Cosmos
• The impact of stellar winds and tidal locking effects on the habitability of Earth-like exoplanets around M dwarf stars
• Formation of terrestrial planets in eccentric and inclined giant planet systems
• A revolution is brewing: observations of TRAPPIST-1 exoplanetary system fosters a new biomarker
• Predicting the Dominant Formation Mechanism of Multi-Planetary Systems
• Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
• The impact of water clouds on the prospective emission spectrum of Teegarden's Star b as observed by LIFE
• Dual-Backend Multibeam Position Switching Targeted SETI Observations toward Nearby Active Planet-Hosting Systems with FAST
• Characterizing Exoplanets for Assessing Their Potential Habitability
• Interpolation and synthesis of sparse samples in exoplanet atmospheric modeling
• A novel metric for assessing climatological surface habitability
• A transiting rocky super-Earth and a non-transiting sub-Neptune orbiting the M dwarf TOI-771
• The when and where of water in the history of the universe
• Exploring the habitability and interior composition of exoplanets lying within the extended habitable zone
• The Dustiest Galactic S Stars: Mid-Infrared Spectra from SOFIA/FORCAST
• On the Dynamics of Comets in Extrasolar Planetary Systems
• From Global Climate Models (GCMs) to Exoplanet Spectra with the Global Emission Spectra (GlobES)
• Rebuilding the Habitable Zone from the Bottom Up with Computational Zones
• Impact of vegetation albedo on the habitability of Earth-like exoplanets
• Forming Earth-like and Low-Mass Rocky Exoplanets Through Pebble and Planetesimal Accretion
• TOI-1634 b: an Ultra-Short Period Keystone Planet Sitting Inside the M Dwarf Radius Valley
• New models of reflection spectra for terrestrial exoplanets: Present and prebiotic Earth orbiting around stars of different spectral types
• Bioverse: Potentially Observable Exoplanet Biosignature Patterns Under the UV Threshold Hypothesis for the Origin of Life
• Atmospheric gravitational tides of Earth-like planets orbiting low-mass stars
• ARDENT: A Python package for fast dynamical detection limits with radial velocities
• Destruction of "Peas in a Pod?" A Candidate Multi-planet System Around the Nearby, Bright Star, HD208487
• Impacts of Atmospheric Carbon Species and Stellar Type on Climates of Terrestrial Planets
• A Cool Earth-sized Planet Candidate Transiting a Tenth Magnitude K-dwarf From K2
• Modelling the Milky Way's exoplanet population based on cosmological galaxy simulations
• Continuous Habitable Zones: Using Bayesian Methods to Prioritize Characterization of Potentially Habitable Worlds
• Carbon Cycle Imbalances on Arid Terrestrial Planets with Implications for Venus
• On the importance of laboratory experiments for interpreting exoplanet observations
• The Most Common Habitable Planets III -- Modeling Temperature Forcing and Surface Conditions on Rocky Exoplanets and Exomoons
• Confirmation of the hot super-Neptune TOI-672 b with NIRPS and HARPS and Insights into the Neptunian desert around M dwarfs
• Evolution and Observable Properties of Rocky Planet Atmospheres
• Main ways in which stars influence the climate and surface habitability of their planets
• Formation of Earth-sized planets within the Kepler-1647 System Habitable Zone
• Quantitative Nonequilibrium Pathway from Fundamental Physics to the Emergence and Persistence of Exoplanetary Biospheres
• A Validated Low-to-Intermediate Mass Planetary Interior Structure Model and New Mass-Radius Relations
• Not Earth-like Yet Temperate? More Generic Climate Feedback Configurations Still Allow Temperate Climates in Habitable Zone Exo-Earth Candidates
• Limit cycles and the climate history of Mars
• Beyond a pale blue dot : how to search for possible bio-signatures on earth-like planets
• Astrophysical Simulations and Data Analyses on the Formation, Detection, and Habitability of Moons Around Extrasolar Planets
• The GAPS programme at TNG LXXI. A sub-Neptune suitable for atmospheric characterization in a multiplanet and mutually inclined system orbiting the bright K dwarf TOI-5789 (HIP 99452)
• A dynamical test for terrestrial planets in the habitable zone of HD 204313
• Does Cosmological Evolution Select for Technology?
• Earth-Like: An education & outreach tool for exploring the diversity of planets like our own
• Ultra-Stable Environment Control for the NEID Spectrometer: Design and Performance Demonstration
• Why M-dwarf flares have limited impact on the atmospheric evaporation of sub-Neptunes and Earth-sized planets
• SPORES-HWO. II. Companion Mass Limits and Updated Planet Properties for 120 Future Exoplanet Imaging Targets from 35 yr of Precise Doppler Monitoring
• The Feasibility of Asynchronous Rotation via Thermal Tides for Diverse Atmospheric Compositions
• Habitability on local, Galactic and cosmological scales
• Hidden water in magma ocean exoplanets
• Twinkle Twinkle Little Star, Roman Sees Where You Are: Predicting Exoplanet Transit Yields in the Rosette Nebula with the Nancy Grace Roman Space Telescope
• The influence of stellar activity on detecting Earth-like planets via nulling interferometry
• The HOSTS Survey: Suspected variable dust emission and constraints on companions around θ Boo
• High-CO2 Climates and Observables in the Outer Habitable Zone
• The Onset of a Globally Ice-covered State for a Land Planet
• Simulated Effects of Radioactive Elements on Magnetic Evolution and Atmospheric Mass Loss of Earth-like Planets
• Multicolour Validation of Two Temperate Mini-Neptunes Around M-dwarf Habitable Zones
• Dynamical Interactions in the Planetary System GJ4276
• Circumbinary habitable zones in the presence of a giant planet
• Multi-Wavelength High-Resolution Spectroscopy for Exoplanet Detection: Motivation, Instrumentation and First Results
• The effect of a biosphere on the habitable timespan of stagnant-lid planets and implications for the atmospheric spectrum
• Rapid Formation of Super-Earths Around Low-Mass Stars
• K2-99 revisited: a non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant
• Setting the Stage: The Early History of the Solar System
• Assessing the Climate and Habitability of Tidally Locked Rocky Exoplanets
• Convection modeling of pure-steam atmospheres
• Super-Earths, M Dwarfs, and Photosynthetic Organisms: Habitability in the Lab
• Interaction between Winds from Weak-lined T Tauri Stars with Exoplanetary Magnetospheres
• A multispecies pseudoadiabat for simulating condensable-rich exoplanet atmospheres
• L 98-59: a Benchmark System of Small Planets for Future Atmospheric Characterization
• Mantle Degassing Lifetimes through Galactic Time and the Maximum Age Stagnant-lid Rocky Exoplanets can Support Temperate Climates
• Potential Habitability as a Stellar Property: Effects of Model Uncertainties and Measurement Precision
• TFAW survey II: 6 Newly Validated Planets and 13 Planet Candidates from K2
• HZ_evolution: A Package to Calculate Habitable Histories
• Chemistry, Climate, and Transmission Spectra of TRAPPIST-1 e Explored with a Multimodel Sparse Sampled Ensemble
• The Color of Habitability
• The extrasolar planet Gliese 581 d: a potentially habitable planet? (Corrigendum to arXiv:1009.5814)
• Habitable zone predictions and how to test them
• Geologic Constraints on Early Mars Climate