Planetary Embryo Growth: From Dust to Planetesimals to Protoplanets
From micrometer grains to lunar-mass embryos: the physics governing planetary assembly across fifteen orders of magnitude
Ocean World Habitability: Energy Sources Below Ice Shells
Beneath ice shells, planetary chemistry and orbital physics conspire to create potential cradles for life in eternal darkness.
Tidally Locked Worlds: How Orbital Dynamics Shape Habitability
Where eternal day meets endless night, the terminator zones of tidally locked planets may offer refuge for life
Cryovolcanism: How Ice Worlds Erupt
Where water becomes magma and ice shells fracture under tidal forces, outer solar system moons reveal alien volcanism
Crustal Dichotomy: Mars' Most Fundamental Mystery
A five-kilometer elevation drop splits Mars in half—and planetary scientists still cannot explain why.
Exoplanet Atmospheres: Reading Alien Air Through Transit Spectroscopy
How filtering starlight through alien atmospheres reveals molecular fingerprints across interstellar distances
Magnetospheric Architecture: How Planetary Magnetic Fields Shape Space Environments
From liquid iron cores to superionic water shells, planetary dynamos create magnetic fortresses that determine which worlds can shelter life from the solar wind.
The Collision That Created Earth's Moon: Reconstructing Giant Impacts
Isotopic puzzles and competing hypotheses reveal that reconstructing the giant impact requires rethinking planetary collision dynamics entirely.
Atmospheric Escape: Why Some Worlds Lose Their Air
Thermal velocities, solar wind interactions, and magnetic fields combine to determine which worlds retain their atmospheres and which lose them to space over billions of years.
The Water Story of Mars: From Oceans to Desiccation
How isotopes, minerals, and ancient valleys reveal the fate of Martian water across four billion years of planetary evolution.
Core Formation: The Violent Process That Makes Planets Habitable
How the violent descent of iron to planetary centers releases energy that powers magnetic shields, drives volcanism, and determines whether worlds can sustain life for billions of years.
Volcanic Resurfacing: How Worlds Erase Their Cratering History
From Venus's catastrophic overturn to Io's hyperactive volcanism, planetary resurfacing rates reveal how worlds manage their internal heat and geological destiny.
Why Planets Migrate: The Solar System's Hidden Orbital History
Discover how ancient gravitational chaos among giant planets delivered Earth's oceans and shaped the conditions that made life possible.
Planetary Ring Formation: The Physics of Debris Disks Around Planets
Inside the Roche limit where moons cannot exist, tidal physics creates the solar system's most spectacular debris disks through catastrophic disruption and resonant sculpting.