It’s not certain how HD 106906 b achieved this orbit, but the leading theory postulates that it formed close to its host stars, and drag within the gas disk pulled it inward. The gravitational effects of the two stars shot it outward, but a passing star stabilized the orbit and prevented the world from becoming a rogue planet.
The findings might also offer a rare peek at the early days of star systems, including ours. This star system is ‘just’ 15 million years old — you apparently don’t have to wait long for a Planet Nine-like orbit to form. Young stars frequently have active cosmic neighborhoods, and this is proof.
There are many unanswered questions, but some of them may be answered relatively soon. Teams hope to use the James Webb Space Telescope to not only confirm their data, but determine if the planet captures material on its way out and even has a mini-system of debris. As unusual as HD 106906 b is now, it might be stranger once astronomers have had a closer look.