Astronomers identify a celestial '3-body problem' lurking in the outer solar system

New research suggests that a binary pair of Kuiper Belt objects, known as the Altjira system, is actually made up of three separate bodies orbiting one another in a complex triad. This rare orbital configuration is often referred to as the "three-body problem."

An artist's interpretation of two asteroids bein gorbited by a third space rock in the 3-body system
New research has suggested that the "Altjira system" of Kuiper Belt objects is made up from three distinct bodies orbiting one another, making it a stable example of the three-body problem.
(Image credit: NASA, ESA, Joseph Olmsted (STScI))

Astronomers may have just identified a rare example of a "three-body problem" hiding in plain sight beyond the solar system's most distant planet. If the observation can be confirmed, it suggests that many more cosmic triplets could be hiding in the outer reaches of our cosmic neighborhood, researchers say.

Back in 2001, astronomers discovered what they thought was a binary system made up of two large bodies orbiting each other approximately 3.7 billion miles (6 billion kilometers) from Earth in the Kuiper Belt — a ring of asteroids, comets and dwarf planets, including Pluto, that lies beyond the orbit of Neptune.

Harry Baker
Senior Staff Writer

Harry is a U.K.-based senior staff writer at Live Science. He studied marine biology at the University of Exeter before training to become a journalist. He covers a wide range of topics including space exploration, planetary science, space weather, climate change, animal behavior and paleontology. His recent work on the solar maximum won "best space submission" at the 2024 Aerospace Media Awards and was shortlisted in the "top scoop" category at the NCTJ Awards for Excellence in 2023. He also writes Live Science's weekly Earth from space series.

You must confirm your public display name before commenting

Please logout and then login again, you will then be prompted to enter your display name.