Re-analysis of the data by a team at Oxford pointed to a number of factors that could completely explain the blip in the planet, which was previously seen as evidence of Alpha Centauri Bb. Factors like solar weather, instrument problems, and the tug from another star could all account for the phantom planet. With no additional data to prove Alpha Centauri Bb is out there, the original HARPS team has penned a paper to be published next month that concurs with the new analysis. There is no Alpha Centauri Bb.
Just because this one planet turned out to be a ghost in the data doesn’t mean there can’t be a planet in orbit of Alpha Centauri B. Astronomers are sure to go hunting for another planet in orbit of Alpha Centauri B or one of the other stars in the system (Alpha Centauri A and Proxima Centauri). For now, the closest confirmed exoplanet is Gliese 15Ab, which is 11 light years away. It’s about five times as massive as Earth and orbits close to its parent star, a small red dwarf.