Concept d’artiste d’une planète extrasolaire “Jupiter chaud”. Crédit : NASA/JPL-Caltech
Les astronomes découvrent une nouvelle méthode pour déterminer l’âge relatif des exoplanètes et prouvent que ces planètes se forment de plusieurs façons.
Dans notre système solaire, les planètes ont un large éventail de propriétés. Par exemple, Jupiter is about 318 times the mass of Earth, while the average surface temperatures on Venus are 847 degrees F, which is hot enough to melt lead. Exoplanets, planets that orbit a star outside our solar system, also have a vast range of properties. Two basic properties are very useful for distinguishing planets: their size and their orbit.
Often, the shorthand names given to types of exoplanets are based on planets in the solar system they are similar to. For example, a Super-Earth is a potentially rocky world that is from double to 10x the mass of Earth. Likewise, a Hot Jupiter is a planet that is about the size of Jupiter, but orbits much closer to its star.
“The question of how these exoplanets form and get to their present orbits is literally the oldest question in our subfield and it is something that thousands of astronomers have been struggling to answer for more than 25 years.” — Kevin Schlaufman, Assistant professor, Department of Physics and Astronomy
Since the first hot Jupiter was discovered in 1995, astronomers have been trying to figure out how the searing-hot exoplanets formed and arrived in their extreme orbits. Johns Hopkins University astronomers have found a way to determine the relative age of hot Jupiters using new measurements from the Gaia spacecraft, which is tracking over a billion stars.
Lead author Jacob Hamer, a PhD student in Physics and Astronomy, will present the findings yesterday (June 13, 2022) at the American Astronomical Society conference. The work is set to be published in the Astronomical Journal.
Called hot Jupiters because the first one discovered was about the same size and shape as our solar system’s Jupiter, these planets are about 20 times closer to their stars than Earth is to the sun, causing these planets to reach temperatures of thousands of degrees Celsius. Existing theories of planet formation could not explain these planets, so scientists came up with several ideas for how hot Jupiters might form.
Initially, scientists proposed that hot Jupiters could form further out, like Jupiter, and then migrate to their present locations due to interactions with their host star’s disk of gas and dust. Or it could be that they form further out and then migrate in much later—after the disk is gone—through a more violent and extreme process called high-eccentricity migration.
An arrow at the bottom of the image indicates the age of the system increasing toward the right of the image from 1-10 Million years, to 10-100 Million years, to greater than 100 Million years. In the middle of the image, at left (1-10 Million years) there is a star surrounded by a disk of gas and dust. A planet is forming in it and migrating closer to the star. At 10-100 Million years the disk is gone and hot Jupiter has already arrived, and is on an aligned orbit. At the top of the figure, there is a planet forming in the disk at 1-10 Million years, but it forms further out than in the bottom panel. There is an arrow spanning the entire 10-100 Million years section. At more than 100 Million years, the planet is on an eccentric, misaligned orbit. A small amount of time later, the planet’s orbit is circular and misaligned. Credit: Jacob Hamer
“The question of how these exoplanets form and get to their present orbits is literally the oldest question in our subfield and it is something that thousands of astronomers have been struggling to answer for more than 25 years,” said co-author Kevin Schlaufman, an assistant professor who works at the intersection of Galactic astronomy and exoplanets.
Some hot Jupiters have orbits that are well-aligned to their star’s rotation, like the planets in our solar system. Others have orbits misaligned from the equators of their stars. Scientists weren’t able to prove whether the different configurations were a product of different formation process, or a single formation process followed by tidal interactions between the planets and the stars. “Without this really precise method of measuring ages there was always missing information,” said Hamer.
Hamer is one of the first astronomers to use the new data from the Gaia satellite to study the ages of exoplanet systems to figure out how they form and evolve. Being able to determine the velocities – the directional speed – of the stars was key in determining their age. When stars are born, they move similarly to one another within the Galaxy. As those stars age, their velocities become more and more different, Hamer said. With this new method, Hamer proved that there are multiple ways that hot Jupiters form.
“One [formation process] se produit rapidement et produit des systèmes alignés, et [the other] se produit sur des échelles de temps plus longues et produit des systèmes mal alignés “, a déclaré Hamer. “Mes résultats suggèrent également que dans certains systèmes avec des étoiles hôtes moins massives, les interactions de marée permettent aux Jupiters chauds de réaligner l’axe de rotation de leur étoile hôte pour être alignés avec leur orbite.”
De nouvelles données provenant de télescopes terrestres et spatiaux aident les scientifiques à en savoir plus sur les exoplanètes. En avril, des équipes d’astronomes, dont certaines de Johns Hopkins, ont fait part de découvertes sur les atmosphères de Jupiters ultra chaudes rendues possibles grâce aux observations du Hubble Space Telescope.
