Alien planet spiraling toward its doom could be Earth's future

The planet, Kepler-1658b, will soon be engulfed in the flames of its own sun.
Chris Young
An artist's impression of the Kepler-1658 system.
An artist's impression of the Kepler-1658 system.

Gabriel Perez Diaz / Instituto de Astrofísica de Canarias 

In a world first, astronomers observed an exoplanet — a planet outside our solar system — whose orbit is decaying to the point it will soon be engulfed by the flames of its host star.

The new discovery sheds light on the incredibly slow process of planetary orbital decay. It is the first glimpse at a planet so near its demise due to the decay of its orbit, a press statement reveals.

Kepler-1658b nears a fiery end

Scientists believe that the Earth could eventually be eaten up by the Sun billions of years from now. Until now, though, scientists hadn't observed another planet so close to meeting a fiery death by its own sun.

Thanks to the new observations, the scientific community can now analyze the exoplanet, called Kepler-1658b, to test theories about orbital decay and the very late stages of planetary evolution.

"We've previously detected evidence for exoplanets inspiraling toward their stars, but we have never before seen such a planet around an evolved star," explains Shreyas Vissapragada from the Center for Astrophysics | Harvard & Smithsonian and lead author of a new study detailing the observation. "Theory predicts that evolved stars are very effective at sapping energy from their planets' orbits, and now we can test those theories with observations." 

The scientists, who published their findings in a paper in The Astrophysical Journal Letters, discovered the exoplanet using the planet-hunting Kepler space telescope, which launched into space in 2009.

Kepler-1658b is a hot Jupiter planet, meaning it naturally has a close orbit to its host star. To be precise, Kepler-1658b is located about an eighth of the distance between the Sun and Mercury.

Scientists calculate infinitesimal orbital decay

Astonishingly, the new study shows how the scientists calculated that Kepler-1658b's orbital period is decreasing by an incredibly slow rate of roughly 131 milliseconds (thousandths of a second) per year.

Calculating that minuscule change required 13 years of observation using Kepler, the Palomar Observatory’s Hale Telescope in Southern California, and the Transiting Exoplanet Survey Telescope, or TESS.

All of these observatories captured transits, which is the term used for the amount of time it takes a planet to cross between its host star and Earth, leading to a very slight dimming in the light received from the star.

The scientists point out that the orbital decay of Kepler-1658b is caused by tidal forces between the planet and its host star, causing it to slowly travel inward.

"Now that we have evidence of inspiraling of a planet around an evolved star, we can really start to refine our models of tidal physics," Vissapragada says. "The Kepler-1658 system can serve as a celestial laboratory in this way for years to come, and with any luck, there will soon be many more of these labs."