Astronomers at the University of Hawaiʻi Institute for Astronomy (IfA) are part of a team that recently discovered three planets orbiting dangerously close to stars nearing the ends of their lives.
Out of the thousands of extrasolar planets found so far, these three gas giant planets, first detected by the NASA TESS (Transiting Exoplanet Survey Satellite) Mission, have some of the shortest-period orbits around subgiant or giant stars. One of the planets, TOI-2337b, will be consumed by its host star in less than 1 million years, sooner than any other planet currently known.
“These discoveries are crucial to understanding a new frontier in exoplanet studies: how planetary systems evolve over time,” explained lead author Samuel Grunblatt, a postdoctoral fellow at the American Museum of Natural History and the Flatiron Institute in New York City. Grunblatt, who earned his PhD from the IfA, added that “these observations offer new windows into planets nearing the end of their lives, before their host stars swallow them up.”
The discovery and confirmation of the planets has been accepted for publication in the Astronomical Journal, and was announced on January 13 at an American Astronomical Society press conference. The researchers estimate that the planets have masses between 0.5–1.7 times Jupiter’s mass, and sizes that range from slightly smaller to more than 1.6 times the size of Jupiter. They also span a wide range of densities, from the density of cork to three times denser than water, implying a wide variety of origins.
These three planets are believed to be just the tip of the iceberg. “We expect to find tens to hundreds of these evolved transiting planet systems with TESS, providing new details on how planets interact with each other, inflate, and migrate around stars, including those like our Sun,” said Nick Saunders, a graduate student at IfA and co-author of the study.
The team hopes that this ‘planetary archeology’ will help us to understand the past, present and future of planetary systems, moving us one step closer to answering the question: “Are we alone?”
In-depth confirmation on Maunakea
The planets were first found in NASA TESS Mission full-frame image data taken in 2018 and 2019. Grunblatt and his collaborators identified the candidate planets in TESS data, and then used the W. M. Keck Observatory on Maunakea to confirm the existence of the three planets.
“The Keck observations of these planetary systems are critical to understanding their origins, helping reveal the fate of solar systems like our own,” said IfA Astronomer Daniel Huber, who co-authored the study.
Current models of planet dynamics suggest that planets should spiral in toward their host stars as the stars evolve over time, particularly in the last 10% of the star’s lifetime. This process also heats the planets, potentially causing their atmospheres to inflate. However, this stellar evolution will also cause the planets around a star to come closer to each other, increasing the likelihood that some of them will collide, or even destabilize the entire planetary system.
The wide variety of planet densities found in the study suggests that these planetary systems have been shaped through chaotic planet-planet interactions. This could also have resulted in unpredictable heating rates and timescales for these planets, giving them the wide range of densities we observe today.
Future observations of one of the systems, TOI-4329, with the recently-launched James Webb Space Telescope, could reveal evidence for water or carbon dioxide in the planet’s atmosphere. If these molecules are seen, the data would provide constraints on where these planets formed, and what sort of interactions had to occur to produce the planetary orbits we see today.
Continued monitoring of these systems with the NASA TESS telescope will constrain the rate at which these planets are spiraling into their host stars. So far, no clear signal of orbital decay has been observed in any of the systems, but a longer baseline of observations with the TESS Extended Missions will provide much tighter constraints on planet in-spiral than are currently possible, revealing how strongly planetary systems are affected by stellar evolution.
Reference: “TESS Giants Transiting Giants II: The hottest Jupiters orbiting evolved stars” by Samuel K. Grunblatt, Nicholas Saunders, Meng Sun, Ashley Chontos, Melinda Soares-Furtado, Nora Eisner, Filipe Pereira, Thaddeus Komacek, Daniel Huber, Karen Collins, Gavin Wang, Chris Stockdale, Samuel N. Quinn, Rene Tronsgaard, George Zhou, Grzegorz Nowak, Hans J. Deeg, David R. Ciardi, Andrew Boyle, Malena Rice, Fei Dai, Sarah Blunt, Judah Van Zandt, Corey Beard, Joseph M. Akana Murphy, Paul A. Dalba, Jack Lubin, Alex Polanski, Casey Lynn Brinkman, Andrew W. Howard, Lars A. Buchhave, Ruth Angus, George R. Ricker, Jon M. Jenkins, Bill Wohler, Robert F. Goeke, Alan M. Levine, Knicole D. Colon, Chelsea X. Huang, Michelle Kunimoto, Avi Shporer, David W. Latham, Sara Seager, Roland K. Vanderspek and Joshua N. Winn, Accepted, Astronomical Journal.
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