Rapid contraction of giant planets orbiting the 20-million-year-old star V1298 Tau

Suárez Mascareño, A.; Damasso, M.; Lodieu, N.; Sozzetti, A.; Béjar, V. J. S.; Benatti, S.; Zapatero Osorio, M. R.; Micela, G.; Rebolo, R.; Desidera, S.; Murgas, F.; Claudi, R.; González Hernández, J. I.; Malavolta, L.; del Burgo, C.; D'Orazi, V.; Amado, P. J.; Locci, D.; Tabernero, H. M.; Marzari, F.; Aguado, D. S.; Turrini, D.; Cardona Guillén, C.; Toledo-Padrón, B.; Maggio, A.; Aceituno, J.; Bauer, F. F.; Caballero, J. A.; Chinchilla, P.; Esparza-Borges, E.; González-Álvarez, E.; Granzer, T.; Luque, R.; Martín, E. L.; Nowak, G.; Oshagh, M.; Pallé, E.; Parviainen, H.; Quirrenbach, A.; Reiners, A.; Ribas, I.; Strassmeier, K. G.; Weber, M.; Mallonn, M.
Bibliographical reference

Nature Astronomy

Advertised on:
12
2021
Description
Current theories of planetary evolution predict that infant giant planets have large radii and very low densities before they slowly contract to reach their final size after about several hundred million years1,2. These theoretical expectations remain untested so far as the detection and characterization of very young planets is extremely challenging due to the intense stellar activity of their host stars3,4. Only the recent discoveries of young planetary transiting systems allow initial constraints to be placed on evolutionary models5-7. With an estimated age of 20 million years, V1298 Tau is one of the youngest solar-type stars known to host transiting planets; it harbours a system composed of four planets, two Neptune-sized, one Saturn-sized and one Jupiter-sized8,9. Here we report a multi-instrument radial velocity campaign of V1298 Tau, which allowed us to determine the masses of two of the planets in the system. We find that the two outermost giant planets, V1298 Tau b and e (0.64 ± 0.19 and 1.16 ± 0.30 Jupiter masses, respectively), seem to contradict our knowledge of early-stages planetary evolution. According to models, they should reach their mass-radius combination only hundreds of millions of years after formation. This result suggests that giant planets can contract much more quickly than usually assumed.
Related projects
Discovery of a system of super-Earths orbiting the star HD 176986 with about 5.7 and 9.2 Earth masses.
Very Low Mass Stars, Brown Dwarfs and Planets

Our goal is to study the processes that lead to the formation of low mass stars, brown dwarfs and planets and to characterize the physical properties of these objects in various evolutionary stages. Low mass stars and brown dwarfs are likely the most numerous type of objects in our Galaxy but due to their low intrinsic luminosity they are not so

Rafael
Rebolo López
Projects' name image
Exoplanets and Astrobiology

The search for life in the universe has been driven by recent discoveries of planets around other stars (known as exoplanets), becoming one of the most active fields in modern astrophysics. The growing number of new exoplanets discovered in recent years and the recent advance on the study of their atmospheres are not only providing new valuable

Enric
Pallé Bago