(Image credit: Karen Teramura/University of Hawai`i Institute for Astronomy)
Astronomers have spotted three new exoplanets orbiting dangerously close to their parent stars, on the brink of extinction.
The three exoplanets, named TOI-2337b, TOI-4329b and TOI-2669b, were discovered using NASA’s Transiting Exoplanet Survey Satellite (TESS) and the W. M. Keck Observatory’s High-Resolution Echelle Spectrometer (HIRES) in Hawai`i.
“These planets are in such extreme places that actually less than 10 years ago, no one thought that they actually existed,” Samuel Grunblatt, lead author of the study and a postdoctoral fellow at the American Museum of Natural History, said during a news conference held by the American Astronomical Society on Thursday (Jan. 13). The new research was meant to be presented at a conference that the organization canceled due to high rates of COVID-19.
The newfound alien worlds are classified as gas giants, with masses between 0.5 and 1.7 times that of Jupiter. The planets also differ greatly in size and density, suggesting they have varying origins, according to a statement from the W. M. Keck Observatory.
“These discoveries are crucial to understanding a new frontier in exoplanet studies: how planetary systems evolve over time,” Grunblatt said in the Keck statement. These observations provide new insights into planets that are nearing the end their lives before their host stars swallow them. “
As a star evolves and enters the last 10% of its life, it may reel in nearby planets. Altering the orbits of the planets around their parent stars could lead to a destabilizing effect on the entire system, or even causing them to collide. Additionally, the planets’ spirals in towards their host stars can cause them to be heated, which can lead to atmospheric changes such as swelling. According to the statement, this type of interplanetary interaction could explain the differences in densities among the alien worlds.
Observations of TOI-2337b, TOI-4329b and TOI-2669b also revealed that the three exoplanets have some of the shortest orbits yet discovered around subgiant or giant dying stars. For example, the orbital period of TOI-2337b suggests the exoplanet will be consumed by its host star in less than 1 million years, which is sooner than any other known planet, according to the study.
“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,” Nick Saunders, co-author of the study and graduate student at the University of Hawaii Institute for Astronomy said in the statement.
Therefore, studying planetary systems like TOI-2337b, TOI-4329b and TOI-2669b may provide a better understanding of our own solar system’s evolution, the researchers said.
Further TESS observations are needed to determine the rate at which the newfound exoplanets are spiraling into their host stars. NASA’s recently-launched James Webb Space Telescope could also help identify the composition of the planets’ atmospheres and, in turn, where the planets formed and how they ended up in such a close-knit orbit around their parent star.
“The rapid changes of the star combined with the short orbital periods of these planets imply these planets should be consumed by their host stars faster than almost any other known planets,” Grunblatt said during the news conference. The study of these systems will reveal how the giant planets behave throughout their lives and how it affects smaller ones, before exploding into their host stars. “
Their findings have been accepted for publication in the Astronomical Journal.
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