Protostars Star Clusters Nebulae Stellar Evolution Young Stars Star-Forming Regions Massive Stars Stellar Nurseries Molecular Clouds Magnetic Fields New Star Formation Protoplanetary Disks Supernovae New Stars Protostellar Outflows Gas Clouds Star-Forming Region Bipolar Jets Low-Mass Stars Planet Formation Interstellar Medium Tarantula Nebula Active Star Formation Starburst Nebulas Early Universe Gas Dynamics Galaxy Interactions Cosmic Evolution Quiescent Galaxies Accretion Processes Dark Nebulae Cosmic Dust Galactic Characteristics Cosmic Time Rho Opiuchi Cloud Complex Nearest Star-Forming Region Stellar Processes Hydrogen and Helium Stellar Clusters Ongoing Star Formation Starburst Galaxies Protostellar Jets Extreme Environments Galactic Center Massive Planets Cloud Collapse Theories Failed Stars Rho Ophiuchi Supernovas Galaxies Stellar Birth Nebula Starburst Patterns Large Magellanic Cloud Dusty Clouds Galaxy Formation Gas and Dust Cosmic Forces Acceleration Effects of Ram Pressure Radcliffe Wave Massive Young Stars Early Star Formation Water Vapor Observations Star-Forming Environments Formation Processes Early Stages Planetary Development Radiation Triangulum Galaxy (M33) Herbig-Haro Object First Stars Turbulence Rate Starburst Galaxy Newly Born Stars Protostellar Disk Protostellar Disks Population III Stars Environmental Conditions Galaxy Evolution Galaxy Characteristics Hydrogen Gas Molecular Cloud Lifecycle Star Families Stellar Families Molecular Hydrogen Binary Stars Orion Nebula Early Phase Nurseries Orphan Stars Star Nurseries Stellar Nursery Newly Formed Stars Euclid Mission Nursery of Star Formation
The immersive rendering of the Gum 31 region highlights star formation and nebular dynamics, debuting at the International Planetarium Society’s 100th anniversary in Munich.