
Caltech Study: Random Solar Mass Ejections Will Destroy Outer Planets in 1 Billion Years
A new study led by Konstantin Batygin at Caltech argues that the outer solar system will collapse within one billion years after the Sun becomes a white dwarf, a timeline a billion times shorter than previous estimates. The research suggests that random, violent mass ejections from the dying Sun, rather than smooth mass loss, will destabilize the orbits of Jupiter, Saturn, Uranus, and Neptune. While earlier models predicted stability for trillions of years, this new analysis indicates that stochastic 'kicks' from the Sun will trigger violent scattering, potentially ending the solar system's existence far sooner than anticipated.













