Artemis Program Perseverance Rover Europa Clipper Dragonfly Mission Mars Missions OSIRIS-REx Artemis II Apollo Program Spacecraft Technology Astronauts Curiosity Rover Sample Return Missions Parker Solar Probe InSight Mission SpaceX Launches Mars Sample Return Mission James Webb Space Telescope Apollo Missions Mars Exploration Psyche Mission DART Mission Voyager 2 Budget Cuts Endurance Mission DART Future Missions Cassini Lunar Reconnaissance Orbiter International Space Station Lucy Mission Europa Clipper Mission Mars Sample Return Dawn Mission Curiosity Mission Boeing Starliner DAVINCI Mission Habitable Worlds Observatory Spacecraft Issues Voyager Program Mars Rovers Artemis II Mission Astronaut Training OSIRIS-APEX Voyager Probes InSIGHT TESS Juno Mars 2020 Galileo Spacecraft MAVEN SPHEREx Mission Curiosity Rover Discoveries Voyager 1 Astronomical Discoveries InSight Curiosity Rover Mission Mars Reconnaissance Orbiter GRAIL Mission OSIRIS-REx Mission Spacecraft Development Astronaut Activities Juno Mission Voyager Missions Venus Exploration InSight Lander AWE Mission Climate Science Mars Insight Lander Asteroid Research Commercial Space Industry Venus Missions Cassini-Huygens IXPE Mars Sample Return Program Legacy Flag Boeing's Starliner Spacecraft Osiris-Rex Data Collection Lunar Prospector Kepler Space Telescope DART Findings Space Shuttles DaVINCI Mission DAVINCI Perseverance Mission DaVinci Mission New Horizon's Mission Mars Sample Return Project ICON Mission Voyager Mission Commercial Space Travel Dawn Spacecraft Solar Eclipse Missions STS-66 Ceres Missions Sounding Rockets SPHEREx Titan Moon Spacecraft Communication Lunar Exploration
Triple-oxygen isotope fingerprints in Apollo regolith isolate impactor material to set limits that Artemis-era samples can refine.