The discovery of planets outside our solar system has reshaped humanity’s understanding of the universe.
However, theories about the formation of hot Jupiters typically fall into two camps,
Published in The Astrophysical Journal Letters, scientists have discovered that TOI-1408c, a peculiar planet in a system featuring a hot Jupiter, sheds new light on planetary formation theories and the complex dynamics of such systems.
TOI-1408b, a grazing hot Jupiter, orbits its star every 4.42 days.
Its companion, TOI-1408c, is a smaller planet with a radius 2.2 times that of Earth and a mass approximately eight times that of Earth.
Transit timing variations are changes in a planet’s orbital timing caused by gravitational interactions with nearby planets.
For TOI-1408c, these variations amount to 15% of its orbital period—the largest relative TTV amplitude ever measured.
TOI-1408c’s peculiarities lie not only in its orbital dynamics but also in its proximity to a hot Jupiter.
Discoveries like TOI-1408c advance our understanding of how planets form and evolve.
As TESS and other instruments uncover more exoplanets, scientists hope to build a more comprehensive picture of the processes governing planetary systems.