Neptune Archives - Astrobiology

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“Neptune”

The Possibility of Hydrogen-Water Demixing in Uranus, Neptune, K2-18b and TOI-270d

Ice Giant

The Possibility of Hydrogen-Water Demixing in Uranus, Neptune, K2-18b and TOI-270d

Different Inhomogeneous Evolutionary Histories for Uranus and Neptune

Ice Giant

Different Inhomogeneous Evolutionary Histories for Uranus and Neptune

Improved H2-He and H2-H2 Collision-Induced Absorption Models and Application to Outer-Planet Atmospheres

Atmospheres, Climate, Weather

Improved H2-He and H2-H2 Collision-Induced Absorption Models and Application to Outer-Planet Atmospheres

Icy Worlds

TOI-6478 b: A Cold Under-dense Neptune Transiting A Fully Convective M Dwarf From The Thick Disc

Exoplanets, -moons, -comets

TOI-6478 b: A Cold Under-dense Neptune Transiting A Fully Convective M Dwarf From The Thick Disc

Webb Space Telescope Captures Neptune’s Auroras For First Time

Neptune

Webb Space Telescope Captures Neptune’s Auroras For First Time

Super-Earth vs. Sub-Neptune? The Winner is Super-Venus

Exoplanets, -moons, -comets

Super-Earth vs. Sub-Neptune? The Winner is Super-Venus

Hubble Celebrates A Decade Of Tracking Outer Planets

Astronomy & Telescopes

Hubble Celebrates A Decade Of Tracking Outer Planets

Detecting Planetary Oceans: Application To The Uranus System

Uranus

Detecting Planetary Oceans: Application To The Uranus System

A Clue To What Lies Beneath The Bland Surfaces Of Uranus And Neptune

Icy Worlds

A Clue To What Lies Beneath The Bland Surfaces Of Uranus And Neptune

H2-H2O Demixing In Uranus And Neptune: Adiabatic Structure Models

Exoplanets, -moons, -comets

H2-H2O Demixing In Uranus And Neptune: Adiabatic Structure Models

Sulfur in the Giant Planets, their Moons, and Extrasolar Gas Giant Planets

Astrochemistry

Sulfur in the Giant Planets, their Moons, and Extrasolar Gas Giant Planets

The Trans- And Post-Capture Orbital Evolution Of Triton

Triton

The Trans- And Post-Capture Orbital Evolution Of Triton

Triton’s Captured Youth: Tidal Heating Kept Triton Warm and Active for Billions of Years

Triton

Triton’s Captured Youth: Tidal Heating Kept Triton Warm and Active for Billions of Years

Mapping The Exo-Neptunian Landscape. A Ridge Between The Desert And Savanna

Exoplanets, -moons, -comets

Mapping The Exo-Neptunian Landscape. A Ridge Between The Desert And Savanna

Hidden Exoplanets Between The Neptunian Desert And Savanna

Exoplanets, -moons, -comets

Hidden Exoplanets Between The Neptunian Desert And Savanna

Classifications For Exoplanet and Exoplanetary Systems

Exoplanets, -moons, -comets

Classifications For Exoplanet and Exoplanetary Systems

Storms and Convection on Uranus and Neptune: Impact of Methane Abundance Revealed by a 3D Cloud-resolving Model

Atmospheres, Climate, Weather

Storms and Convection on Uranus and Neptune: Impact of Methane Abundance Revealed by a 3D Cloud-resolving Model

Volatile-rich Sub-Neptunes as Hydrothermal Worlds: The Case of K2-18 b

Exoplanets, -moons, -comets

Volatile-rich Sub-Neptunes as Hydrothermal Worlds: The Case of K2-18 b

Twin Worlds, Divergent Fates: How Obliquity has Differently Shaped Pluto’s and Triton’s Landscapes and Climates

Triton

Twin Worlds, Divergent Fates: How Obliquity has Differently Shaped Pluto’s and Triton’s Landscapes and Climates