Andromeda Thick Disk Galactic Center Sagittarius A* Star Formation Satellite Galaxies Large Magellanic Cloud Galactic Collisions Galactic Structure Cosmic Phenomena Halo Stars eROSITA bubbles Extreme Outer Galaxy Infrared Observations Structure Black Holes Galactic Mapping Evolution Dark Matter Galactic Evolution Radcliffe Wave Gaia Space Telescope Galactic Mergers Binary Star Systems Galactic Structures Star Behavior Galactic Collision Central Molecular Zone Star Observations Andromeda Galaxy Star Populations Interstellar Objects Thick Disk Stars Visibility Nebulae Galaxy Mapping Southern Galactic Plane Local Hot Bubble Neutrinos Halo Dynamics Supermassive Black Hole Reticulum II Dwarf Galaxy Star Jets Collision History Distance to Stars Binary Stars Dwarf Galaxies Galactic Discoveries Gaia Mission Galactic Birth Radii Distant Worlds Star Systems Comparative Studies Space Tornadoes Data Analysis Astronomical Discoveries Cosmic Events Formation Small Magellanic Cloud Local Void KBC Void SPHEREx Telescope Galactic Bulge Spiral Galaxy Euclid Sagittarius C Stellar Streams Extragalactic Origin Center NGC 2264 Collision and merger with Magellanic Clouds Mapping Nuclear Disk Rotation Curve Center of Milky Way Hubble Space Telescope Gaia spacecraft Radcliffe Wave motion Radcliffe Wave properties Radcliffe Wave research Galactic Potential Radcliffe Wave Effect Galaxy Dynamics Star-Forming Regions Gaia Observatory Data Star Streams Ancient Structures Stellar Composition Gaia Telescope Ancient Star Streams Building Blocks Schildwolke Ancient Stars Thin Disk LSST Camera Black Holes in Milky Way BH3 Galaxy Merging Gaia BH3 Orion Constellation
Researchers compared zircon oxygen data with galactic hydrogen maps to suggest impact surges during spiral-arm crossings.