Planet Formation Solar System Protoplanetary Disks Orbital Mechanics Gas Giants Exoplanets Red Dwarf Stars Planetary Formation Star Characteristics Formation Solar Systems Protoplanetary Discs Planetary Discovery Planetary Evolution Rocky Planets Solar System Formation Orbital Dynamics Stability Beta Pictoris Multi-Planetary Systems Planetary Characteristics Super-Earths Formation Theories Exoplanetary Atmospheres Planet Types Planet Consumption Formation Mechanisms Jupiter System Habitability Development Kepler-725 System Planetary Distances Red Giant Stars Satellite Dynamics HD 110067 Atmosphere L 98-59 System Orbiting Planets Kuiper Belt Objects Goldilocks Zone Planet-Planet Occultations Magnetosphere Ingestion Factors Binary Objects Star Systems Planetary Formation Theories Inner Planets Ring Systems Planets Uranus Formation of Comets G-type Stars Binary Stars Orbital Patterns Planetary Dynamics Super-Neptune Outer Planets Moon Formation Binary Star Systems Small Bodies Mutual Inclination Gas Dispersal Water Vapor Planetary Nebulae Exoplanetary Comparisons Young Stars Giant Planets Debris Discs Planetary Remnants Multiplanet system Consequences of Planetary Ingestion Formation of Planets Instability Circumbinary Planets Dynamics Metal Accretion Orbit LHS 1903 Extrasolar Planets Habitable Zone Diversity Red Dwarfs Ejection Processes Planetary Devouring Solar System Analogues Multi-Planet Systems Multiplanet Systems Epsilon Indi System 14 Herculis System Planet Population Synthesis Moons Epsilon Indi Diverse Compositions Resonance Formation Processes Life TRAPPIST-1 System TRAPPIST-1 40 Eridani A System Kepler Space Telescope
Validating TESS’s high-cadence archive as a microlensing tool, the discovery opens a new way to find wide-orbit planets.
