sub-Neptune Archives - Astrobiology

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Evidence For Sulfur Chemistry In The Atmosphere Of The Warm Sub-Neptune TOI-270 d

Atmospheres & Climate

Evidence For Sulfur Chemistry In The Atmosphere Of The Warm Sub-Neptune TOI-270 d

Planetary Albedo Is Limited By The Above-cloud Atmosphere: Implications For sub-Neptune Climate (K2-18b)

Exoplanetology: Exoplanets & Exomoons

Planetary Albedo Is Limited By The Above-cloud Atmosphere: Implications For sub-Neptune Climate (K2-18b)

Deciphering The Mysterious Atmosphere Of ‘Rosetta Stone’ Exoplanet TOI-270 d

Habitable Zones & Global Climate

Deciphering The Mysterious Atmosphere Of ‘Rosetta Stone’ Exoplanet TOI-270 d

Characterizing Planetary Systems With SPIRou: Detection Of A Sub-Neptune In A 6 day Period Orbit Around The M Dwarf Gl 410

Exoplanetology: Exoplanets & Exomoons

Characterizing Planetary Systems With SPIRou: Detection Of A Sub-Neptune In A 6 day Period Orbit Around The M Dwarf Gl 410

The Radiative Effects of Photochemical Hazes on the Atmospheric Circulation and Phase Curves of Sub-Neptunes

Atmospheres & Climate

The Radiative Effects of Photochemical Hazes on the Atmospheric Circulation and Phase Curves of Sub-Neptunes

Distinguishing Between Gas Dwarfs And Water Worlds With Young Transiting Exoplanets

Exoplanetology: Exoplanets & Exomoons

Distinguishing Between Gas Dwarfs And Water Worlds With Young Transiting Exoplanets

Combination Of Cosmic Processes Shapes The Size And Location Of sub-Neptunes

Exoplanetology: Exoplanets & Exomoons

Combination Of Cosmic Processes Shapes The Size And Location Of sub-Neptunes

An Oxidation Gradient Straddling the Small Planet Radius Valley

Astrogeology

An Oxidation Gradient Straddling the Small Planet Radius Valley

TESS and HARPS-N Unveil Two Planets Transiting TOI-1453. A Super-Earth and One of the Lowest Mass sub-Neptunes

News Summary Archives

TESS and HARPS-N Unveil Two Planets Transiting TOI-1453. A Super-Earth and One of the Lowest Mass sub-Neptunes

Utilizing Machine Learning to Predict Host Stars and the Key Elemental Abundances of Small Planets

Exoplanetology: Exoplanets & Exomoons

Utilizing Machine Learning to Predict Host Stars and the Key Elemental Abundances of Small Planets

Examining the Potential for Methyl Halide Accumulation and Detectability in Possible Hycean-Type Atmospheres

Water/Hycean Worlds & Oceanography

Examining the Potential for Methyl Halide Accumulation and Detectability in Possible Hycean-Type Atmospheres

A Long Spin Period For A Sub-Neptune-mass Exoplanet

Exoplanetology: Exoplanets & Exomoons

A Long Spin Period For A Sub-Neptune-mass Exoplanet

Architecture Classification For Extrasolar Planetary Systems

Exoplanetology: Exoplanets & Exomoons

Architecture Classification For Extrasolar Planetary Systems

A New Convection Scheme For GCMs Of Temperate Sub-Neptunes

Exoplanetology: Exoplanets & Exomoons

A New Convection Scheme For GCMs Of Temperate Sub-Neptunes

On The Robustness Of Exoplanet Atmospheric Detections: Insights From Extensive Simulations

Exoplanetology: Exoplanets & Exomoons

On The Robustness Of Exoplanet Atmospheric Detections: Insights From Extensive Simulations

Planetary Edge Trends (PET). I. The Inner Edge-Stellar Mass Correlation

Exoplanetology: Exoplanets & Exomoons

Planetary Edge Trends (PET). I. The Inner Edge-Stellar Mass Correlation

TOI-421 b: A Hot Sub-Neptune with a Haze-Free, Low Mean Molecular Weight Atmosphere

Exoplanetology: Exoplanets & Exomoons

TOI-421 b: A Hot Sub-Neptune with a Haze-Free, Low Mean Molecular Weight Atmosphere

Evolution Of Steam Worlds: Energetic Aspects

Exoplanetology: Exoplanets & Exomoons

Evolution Of Steam Worlds: Energetic Aspects

OrCAS: Origins, Compositions, and Atmospheres of Sub-neptunes. I. Survey Definition

Astrogeology

OrCAS: Origins, Compositions, and Atmospheres of Sub-neptunes. I. Survey Definition

Water-rich sub-Neptunes and Rocky Super Earths Around Different Stars: Radii Shaped by Volatile Partitioning, Formation, and Evolution

Exoplanetology: Exoplanets & Exomoons

Water-rich sub-Neptunes and Rocky Super Earths Around Different Stars: Radii Shaped by Volatile Partitioning, Formation, and Evolution