The impossible planet
When red giants expand, they engulf the planets in their vicinity. Researchers have now found a planet that defies this notion – and a surprising explanation.
The constellation Ursa Minor is home to a planet that cannot exist. At far too close a distance, Halla orbits the red giant star Baekdu. When Baekdu inflated in its previous expansion phase, it should have "swallowed" such a close companion. No other planets orbiting similarly near a red giant star are known. In today's issue of the journal Nature, an international team of 42 researchers led by the University of Hawaii describes the unusual pair and presents extensive calculations of its possible evolution. The computer simulations, to which a researcher from the Max Planck Institute for Solar System Research (MPS) in Göttingen contributed, provide an intriguing explanation. Most likely Baekdu was once a binary star – and Halla never in any danger.
When stars similar in mass to the Sun reach the end of their lifetimes, a spectacular transformation takes place. The fusion of hydrogen atoms in their core comes to a halt, and the star initially collapses in on itself. The tremendous pressure and heat thus generated in the core causes helium fusion to begin. The star, now called a red giant, inflates to up to a hundred times its original size before shrinking again a little. Planets that are in the way of their star's enormous growth don't stand a chance. They are devoured. In the distant future, this fate is also likely to befall Earth. The red giant Baekdu, also referred to as 8 Ursae Minoris, and its planet Halla, however, seem to defy this conception.
Upon its discovery eight years ago by a South Korean research team, exoplanet Halla was by no means deemed remarkable. Since the measurements at the Bohyunsan Optical Astronomy Observatory at that time could not firmly identify the evolutionary state of the star, Halla's close orbit did not surprise. After all, Baekdu could have been a mid-life star – and thus of a much more modest size. It wasn't until NASA's space telescope TESS (Transiting Survey Satellite) took a closer look between 2019 and 2022 that it became possible to determine other properties of the star and its companion. TESS routinely records observational data such as characteristic brightness variations caused by stellar oscillations from thousands of stars. With the help of methods of asteroseismology, scientists can then infer the stars’ age, mass and evolutionary state. In addition, the W. M. Keck Observatory and the Canada-France-Hawaii Telescope on the Hawaiian volcano Mauna Kea also inspected Baekdu and Halla closely.
An unusual pair
Analyses of these data, reported today by the 42-member team in the journal Nature, prove Baekdu and Halla to be something of an oddity. Baekdu is one of the fainter objects in the constellation of Ursa Minor and, unlike its "neighbor" Polaris, cannot be seen with the naked eye. It is approximately 1.5 times heavier than the Sun and has reached the red giant stage. From these and other properties it follows that at the peak of Baedu’s expansion the star reached a radius of a little more than one hundred million kilometers. Afterwards, it subsided again somewhat. Its planetary companion Halla is about one and a half times heavier than Jupiter and orbits its star on a nearly circular path at a distance of about 75 million kilometers – which seams entirely impossible.
"Naturally, we wanted to understand how this strange planetary system came to be," said Dr. Chen Jiang of the MPS, who was involved in the study. How could the planet survive in such close proximity to a red giant? With the help of extensive computer simulations the researchers weighed various possibilities. As it turned out, the most likely explanation is a turn of events that never placed Halla in direct danger of being devoured by its host star.
From binary star to red giant
"We believe that Baekdu was once a binary star," Jiang said. "When one partner of a binary star expands toward the end of its lifetime, both stars can merge. This stops further expansion," he adds. In this case, the red giant might not have inflated to the orbit of its planet at all. To test this hypothesis, the team simulated this scenario on the computer. The scientists modelled not only the stellar merger itself, but also how this process would affect orbiting planets. Their calculations show that the newly formed star Baekdu would have expanded to a much smaller size – and Halla in turn would have been completely unaffected by the transformation of its star; it would continue to orbit unchanged.
It is also conceivable that Halla did not witness the merger of the double star, but was formed after this process. When two stars merge, rotating disks of dust can form around the new star. As in the early Solar System, this dust can gradually cluster together to form planets.
Neither impossible nor rare
Binary stars are far from rare. On the contrary, most stars are part of such stellar partnerships. And numerous exoplanets orbiting binary stars are also already known. "It is likely that planets orbiting in the close proximity to red giants are not as extraordinary as thought," Jiang concludes. Future space missions and observation campaigns may discover many more.