8 Ursae Minoris b, an enormous planet, surprisingly survives regardless of its host star’s enlargement that ought to have engulfed it. Scientists counsel both a binary star system that checked the star’s development or a second-generation planet formation from a stellar merger as attainable explanations, shedding new mild on stellar and planetary evolution.
A large planet has escaped engulfment by its host star, to the shock of scientists world wide.
The very uncommon planet, 8 Ursae Minoris b, survives in its present location, 520 mild years from Earth, within the Milky Way, for reasons very hard to explain. In normal circumstances, it should have been engulfed by its host star – which expands significantly as it decays. But 8 Ursae Minoris b remains in existence.
The discovery was made by a collaboration of more than 40 academics around the world – including Marc Hon at the University of Hawai’i and Dr. Dimitri Veras at the University of Warwick, which hosts leading research into white dwarf stars.
Dr. Veras said: “The distance between the Earth and its star, the sun, is 1 astronomical unit, or 1 au. 8 Ursae Minoris b is orbiting its star at 0.5 au. While the distance is not unusual in itself, what is strange is that the star is in the process of dying, having already spent some of its fuel.
“When a star spends fuel, it expands in size significantly. This star would have already expanded its size to 0.7 au, which should have engulfed and destroyed the planet. So it’s very unusual that the planet still exists.”
The scientists then further investigated reasons as to why the planet remains unscathed.
“We came up with two possible explanations,” added Dr. Veras. “The first, more plausible argument, is that the star once had a companion star (a “binary star”), that quenched its increase in size, allowing the planet to survive. This binary companion eventually merged with the main star, and now just appears as a single star.
“The second theory, which is less widely explored, again invokes a binary companion. This time the merger of the two stars produced a disc from which this planet was generated – known as a second-generation planet.
“The wider impact is a better understanding of the evolution of stars like our Sun and the evolution of planets like those we see in the solar system, and the need to look out for additional unusual cases like the observed system. Sometimes the rarest cases can reveal the most about stellar and planetary physics.
“Understanding these rare planetary systems enables us to learn new ways in which planets and stars evolve, and motivates us to discover even more rare examples.”
Marc Hon, University of Hawai’i, said: “Most stars are in binary systems, but we don’t yet fully grasp how planets may form around them. It is plausible that many more peculiar planetary systems may exist due to the influence of binary companions.”
Professor Bill Chaplin from the University of Birmingham added: “This is a great example of the detailed, forensic studies we can now perform thanks to the latest data, including using the natural oscillations of the host star (asteroseismology) observed by the TESS space telescope to confirm beyond any doubt that the star is a core-helium-burning red giant.”
For more on this discovery, see Astronomers Discover a Mysterious Planet That Shouldn’t Exist.
Reference: “A close-in giant planet escapes engulfment by its star” by Marc Hon, Daniel Huber, Nicholas Z. Rui, Jim Fuller, Dimitri Veras, James S. Kuszlewicz, Oleg Kochukhov, Amalie Stokholm, Jakob Lysgaard Rørsted, Mutlu Yıldız, Zeynep Çelik Orhan, Sibel Örtel, Chen Jiang, Daniel R. Hey, Howard Isaacson, Jingwen Zhang, Mathieu Vrard, Keivan G. Stassun, Benjamin J. Shappee, Jamie Tayar, Zachary R. Claytor, Corey Beard, Timothy R. Bedding, Casey Brinkman, Tiago L. Campante, William J. Chaplin, Ashley Chontos, Steven Giacalone, Rae Holcomb, Andrew W. Howard, Jack Lubin, Mason MacDougall, Benjamin T. Montet, Joseph M. A. Murphy, Joel Ong, Daria Pidhorodetska, Alex S. Polanski, Malena Rice, Dennis Stello, Dakotah Tyler, Judah Van Zandt and Lauren M. Weiss, 28 June 2023, Nature.