Stuart Talbott: "Rogue Planet" Breaks Astronomy
Thunderbolts Project
Oct 27, 2025
A milestone discovery of evidential data may prove it doesn’t take the million years or more thought necessary to form a planet or star.
Astronomers have observed what they call a young “rogue planet” growing at an impossibly rapid rate. Rather than the slow accretion process of Standard Model gravitational theory, the object is forming at a rate of up to billions of metric tons per second—astonishingly growth that blur the theoretical lines between planets, brown dwarfs, and stars.
Located 620 light years from Earth is Cha 1107-7626 at only 5-to-10 times the mass of Jupiter—well below the 80-Jupiter lower mass limit for stars and the 13-Jupiter lower mass limit for brown dwarfs.
Independent researcher Stuart Talbott deconstructs “the strongest accretion episode ever recorded for a planetary mass object” and shares his 2018 interview with Wall Thornhill who anticipated such discoveries decades ago.

