Life After Death: Hawaiʻi Astronomers Find a Planet that Shouldn’t Exist

Maunakea, Hawaiʻi  – When our Sun reaches the end of its life, it will expand to 100 times its current size, enveloping the Earth. Many planets in other solar systems face a similar doom as their host stars grow old. But not all hope is lost, as astronomers from the University of Hawaiʻi Institute for Astronomy (UH IfA) have made the remarkable discovery of a planet’s survival after what should have been certain doom at the hands of its sun.

The Jupiter-like planet 8 UMi b, officially named Halla, orbits the red giant star Baekdu (8 UMi) at only half the distance separating the Earth and the Sun. Using two Maunakea Observatories on Hawaiʻi Island – W. M. Keck Observatory and Canada-France-Hawaiʻi Telescope (CFHT) – a team of astronomers led by Marc Hon, a NASA Hubble Fellow at UH IfA, has discovered that Halla persists despite the normally perilous evolution of Baekdu. Using observations of Baekdu’s stellar oscillations from NASA’s Transiting Exoplanet Survey Satellite (TESS), they found that the star is burning helium in its core, signaling that it had already expanded enormously into a red giant star once before. 

The star would have inflated up to 1.5 times the planet’s orbital distance – engulfing the planet in the process – before shrinking to its current size at only one tenth of that distance.

The study is published in today’s issue of the journal Nature

“Planetary engulfment has catastrophic consequences for either the planet or the star itself – or both. The fact that Halla has managed to persist in the immediate vicinity of a giant star that would have otherwise engulfed it highlights the planet as an extraordinary survivor,” said Hon, the lead author of the study.    


The planet Halla was discovered in 2015 by a team of astronomers from Korea using the radial velocity method, which measures the periodic movement of a star due to the gravitational tug of the orbiting planet. Following the discovery that the star must at one time have been larger than the planet’s orbit, the IfA team conducted additional observations from 2021-2022 using Keck Observatory’s High-Resolution Echelle Spectrometer (HIRES) and CFHT’s ESPaDOnS instrument. These new data confirmed the planet’s 93-day, nearly circular orbit had remained stable for over a decade and that the radial velocity changes must be due to a planet.

“Together, these observations confirmed the existence of the planet, leaving us with the compelling question of how the planet actually survived,” said IfA astronomer Daniel Huber, second author of the study. “The observations from multiple telescopes on Maunakea was critical in this process.”

Artist’s animation showing one of the possible explanations as to how planet Halla managed to avoid getting swallowed by its host star Baekdu. In this scenario, Baekdu may have originally been part of a binary system comprising a red giant star and a white dwarf star. The two stars then merged, which would have prevented the red giant from expanding large enough to engulf Halla. Credit: W. M. Keck Observatory/Adam Makarenko

Artist’s animation showing an alternative explanation for planet Halla’s existence. In this scenario. Baekdu was originally a binary system comprising a red giant star closely orbiting a white dwarf star. The two stars then merged, and the violent collision between the pair released debris from which the planet Halla formed. Credit: W. M. Keck Observatory/Adam Makarenko


At a distance of 0.46 astronomical units (AU, or the Earth-Sun distance) to its star, the planet Halla resembles ‘warm’ or ‘hot’ Jupiter-like planets that are thought to have started on larger orbits before migrating inward close to their stars. However, in the face of a rapidly evolving host star, such an origin becomes an extremely unlikely survival pathway for planet Halla. 

Another theory for the planet’s survival is that it never faced the danger of engulfment. Similar to the famous planet Tatooine from Star Wars, which orbits two suns, the team believes the host star Baekdu may have originally been two stars. A merger of these two stars may have prevented any one of them from expanding sufficiently large enough to engulf the planet. 

A third possibility is that Halla is a relative newborn — that the violent collision between the two stars produced a gas cloud from which the planet formed. In other words, the planet Halla may be a recently-born ‘second generation’ planet. 

“Most stars are in binary systems, but we don’t yet fully grasp how planets may form around them. Therefore, it’s plausible that more planets may actually exist around highly evolved stars thanks to binary interactions,” explained Hon. 

Evolutionary pathways for the 8 UMi system. (Top) Had the planet 8 UMi b orbited a single star closely, the star’s expansion would have destroyed the planet. (Middle and bottom) The merger of two stars provides two scenarios that may have led to the planet’s survival around a core-helium burning star as observed today.


As the first known close-in planet around a core-helium burning star, the planet Halla shows that exoplanet discoveries may still surprise us by appearing around stars where they are least expected. The ultimate fate of exoplanets is yet uncertain, but the union between stellar and planetary sciences will continue to shed light on whether death-by-star is a fate truly shared across all planets residing near their suns.

Co-authors on the study include Nicholas Rui and Jim Fuller from Caltech, Dimitri Veras from the University of Warwick, a multinational group of researchers hailing from Italy, Denmark, Turkey, and Australia, as well as astronomers affiliated with the California Planet Search group. Additional co-authors on the study include IfA graduate students Jingwen Zhang and Casey Brinkman, IfA postdoctoral fellows Daniel Hey and Joel Ong, and UH IfA alumni Ashley Chontos, Zachary Claytor, Jamie Tayar, and Lauren Weiss.


W. M. Keck Observatory’s High-Resolution Echelle Spectrometer (HIRES) produces spectra of single objects at very high spectral resolution, yet covering a wide wavelength range. It does this by separating the light into many “stripes” of spectra stacked across a mosaic of three large CCD detectors. HIRES is famous for finding exoplanets. Astronomers also use HIRES to study important astrophysical phenomena like distant galaxies and quasars, and find cosmological clues about the structure of the early universe, just after the Big Bang.


Founded in 1967, the Institute for Astronomy at the University of Hawaiʻi at Mānoa conducts research into galaxies, cosmology, stars, planets, and the sun. Its faculty and staff are also involved in astronomy education, deep space missions, and in the development and management of the observatories on Haleakalā and Maunakea. The Institute operates facilities on the islands of Oahu, Maui, and Hawaiʻi.


The Maunakea Observatories are a collaborative of independent institutions with telescopes located on Maunakea on the island of Hawaiʻi. Together, the Observatories make Maunakea the most scientifically productive site for astronomy world-wide. The Maunakea Observatories include: Canada-France-Hawaii Telescope, international Gemini Observatory, a Program of NSFʻs NOIRLab, James Clerk Maxwell Telescope (EAO), NASA Infrared Telescope Facility, Subaru Telescope, Submillimeter Array, UKIRT Observatory, University of Hawai’i Hilo Educational Telescope, University of Hawai‘i 2.2 Meter Telescope, Very Long Baseline Array, and W. M. Keck Observatory (Keck I and Keck II).