A study revealed that a distant planet is dangerously close to its aging star.
According to the study, which was published on Monday, this may give an idea of the possible end of the planet.
Located 2,600 light-years from Earth, Kepler-1658b is an exoplanet roughly the size of Jupiter.
But unlike this gas giant farther from the sun, Kepler-1658b orbits its star only an eighth of the distance separating our sun from its closest planet, Mercury.
The study, published in The Astrophysical Journal Letters, indicated that this “hot Jupiter” orbits its star in less than three days, and this rotation period is shrinking by about 131 miles per second per year.
“At this rate, the planet will collide with its star in less than three million years,” said lead author Shreyas Visapragada of the Harvard-Smithsonian Center for Astrophysics.
The astrophysicist explained, “This is the first time that we have observed direct evidence of the existence of a planet moving in a spiral path around its aging star.”
The star in question is in an advanced phase of its cycle, when it begins to swell and become brighter.
Kepler-1658b’s orbit is shrinking inexorably under the influence of gravity exerted by the star, similar to the gravity exerted by the Moon on various points on Earth.
This effect called tidal force can attract two bodies just as it can move them away from each other, for example the moon is moving very slowly away from the earth in a spiral path.
“The death of a planet due to a star is a fate that awaits many worlds, and could spell Earth’s final farewell after billions of years as it continues to orbit the sun,” the Center for Astrophysics wrote in a statement.
In five billion years, the sun will become a “red giant” that will grow exponentially, similar to the host star of Kepler-1658b.
Like this exoplanet, Earth can inexorably draw closer to the sun under the influence of tidal forces. But this effect can also be offset by the loss of mass from the Sun, says Shreyas Visapragadhan, who stresses that “the ultimate fate of the Earth is still not clear.”
Kepler-1658b was the first exoplanet to be detected using the Kepler space telescope, in 2009. For 13 years, scientists have been observing the slow but steady change in the planet’s orbit as it passes in front of its host star.
Finding it surprisingly bright compared to other exoplanets, they had long assumed that it particularly reflected starlight. But they now believe Kepler-1658b is hotter than expected due to the star’s gravity.