The Sun Migrated from the Galactic Center 5 Billion Years Ago

Published on March 15, 2026 | Translated from Spanish

New studies with data from the ESA's Gaia satellite indicate that our Sun did not form in its current location. The research, led by Japanese teams, suggests that it formed near the heart of the Milky Way and then migrated. By analyzing stars that are twins to the Sun in age and composition, a common pattern of radial displacement is observed. This journey of about 10,000 light-years may have been a determining factor for Earth to be a more stable and conducive environment for life.

The Sun, in its youth, shines near the galactic bulge, beginning its long migratory journey toward the suburbs of the Milky Way.

Gaia and the chemical analysis of solar twin stars 🔬

The key to the discovery lies in Gaia's astrometric and spectroscopic precision. The researchers identified thousands of stars with chemical compositions and ages very similar to those of the Sun, considered twins. By mapping the current distribution of these stars and applying dynamic models of the galaxy, it is inferred that their common point of origin is significantly closer to the galactic bulge. This technique allows reconstructing past movements without directly observing the event, validating theories of stellar radial migration.

Our Sun was a young star that left the bustling galactic center 🚀

It seems that our king star had a restless youth. Tired of the dense and violent environment of the galactic center, with its constant supernova explosions and intense radiation, it decided to pack its bags. It embarked on a journey of billions of years toward the quiet suburbs of the spiral arm. Without this cosmic move, seeking a calmer neighborhood, we might never have had the opportunity to discuss charts or performance on this forum. A lesson that changing neighborhoods sometimes has its advantages.