Solar System Planetary Atmospheres Protoplanetary Discs Accretion Processes Debris Disks Orbital Dynamics Exoplanetary Systems Chemical Composition Gravitational Interactions Kuiper Belt Planetary History Cosmic Dust Saturn Planetary Composition Water Evaporation Planetary Dynamics Planetary Disintegration Evolution of Exoplanets Nebulae Planetary Evolution Disk Dynamics Exoplanet Atmospheres Protoplanetary Disks Direct Imaging Planet-Star Interactions Cosmic Materials Planetesimals Gas Giants Habitability Planetary Systems Magnetic Fields Planetary Interiors Core Evolution Substellar Companions Exoplanets Extraterrestrial Materials Accretion Gas and Dust Disks Celestial Mechanics Disk Accretion Models Rocky Planets Composition of Celestial Bodies Meteorites Water in Space Galactic Evolution Interplanetary Dust Dust Clouds Neutron Stars Atmospheric Science Gas Giant Formation Star Remnants Ring Systems Disk Structure Planetary Characteristics Formation Theories Extreme Environments Inner Planets Interstellar Objects Moon Formation Theories Stellar Evolution Solar System Formation Low-Mass Planets Tidal Locking
NIRSpec integral-field measurements of H3+ across nearly a full rotation reveal structure set by Uranus’s tilted, offset magnetic field.
