Exoplanets come in many different types and sizes, and to understand how planets form and develop, it’s helpful to see them at a variety of different points throughout their life cycle. NASA’s exoplanet-hunting satellite TESS has recently discovered four “teenage” exoplanets, including one dramatic lava world that orbits ultra-close to its star.
TESS investigated two young stars that are close to each other and thought to be related, TOI 2076 and TOI 1807. It found four exoplanets in orbit around them that are in a rarely-spotted middle phase between recent birth and maturity.
“The planets in both systems are in a transitional, or teenage, phase of their life cycle,” said Christina Hedges, an astronomer at the Bay Area Environmental Research Institute in Moffett Field and NASA’s Ames Research Center in Silicon Valley. “They’re not newborns, but they’re also not settled down. Learning more about planets in this teen stage will ultimately help us understand older planets in other systems.”
Three of the exoplanets orbit TOI 2076, each of which is called a mini-Neptune, as they are between Earth and Neptune in size.
But the really dramatic planet is the one seen orbiting TOI 1807. The planet, TOI 1807 b, is so close to its star that a year there lasts just 13 hours. This planet is the youngest version of such a planet, called an ultra-short period planet, yet discovered. If the planet is mostly rock and doesn’t have a thick atmosphere, researchers predict that it could be covered in lakes or even oceans of lava.
This planet is also bombarded with UV radiation because its star is so young and active. It is estimated that the planet is hit with 22,000 times the amount of UV radiation from its star than Earth gets from the sun. And the other star is similarly active as well.
“The stars produce perhaps 10 times more UV light than they will when they reach the sun’s age,” said co-author George Zhou, an astrophysicist at the University of Southern Queensland in Australia. “Since the sun may have been equally as active at one time, these two systems could provide us with a window into the early conditions of the solar system.”
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