By Jacopo Prisco, CNN
(CNN) — An exoplanetary system about 116 light-years from Earth could flip the script on how planets form, according to researchers who discovered it using telescopes from NASA and the European Space Agency, or ESA.
Four planets orbit LHS 1903 — a red dwarf star, the most common type of star in the universe — and are arranged in a peculiar sequence. The innermost planet is rocky, while the next two are gaseous, and then, unexpectedly, the outermost planet is also rocky.
This arrangement contradicts a pattern commonly seen across the galaxy and in our own solar system, where the rocky planets (Mercury, Venus, Earth and Mars) orbit closer to the sun and the gaseous ones (Jupiter, Saturn, Uranus and Neptune) are farther away.
Astronomers suspect this common pattern arises because planets form within a disk of gas and dust around a young star, where temperatures are much higher close to the celestial body. In these inner regions, volatile compounds such as water and carbon dioxide are vaporized while only materials that can withstand extreme heat — such as iron and rock-forming minerals — can clump together into solid grains. The planets that form there are therefore primarily rocky.
Farther from the star, beyond what scientists call the “snow line,” temperatures are low enough for water and other compounds to condense into solid ice — a process that allows planetary cores to grow quickly. Once a forming planet reaches about 10 times the mass of Earth, its gravity is strong enough to pull in vast amounts of hydrogen and helium, and in some cases, this runaway growth produces a giant gas planet such as Jupiter or Saturn.
“The paradigm of planet formation is that we have rocky inner planets very close to the stars, like in our solar system,” said Thomas Wilson, an assistant professor in the department of physics at the University of Warwick in England and first author of a study on the discovery that was published Thursday in the journal Science. “This is the first time in which we have a rocky planet so far away from its host star, and after these gas-rich planets.”
The unexpected rocky planet, called LHS 1903 e, has a radius about 1.7 times that of Earth, making it what astronomers call a “super Earth” — a larger version of our planet with similar density and composition. But why is it there, defying logic and previous observations?
“We think that these planets formed in very different environments from each other, and that is what’s kind of unique about this system,” Wilson said. “This outer planet, which is rockier compared to the middle two planets, shouldn’t have happened, based on the standard formation theory. But what we think happened is that it formed later than the other planets.”
‘Gas-depleted’ formation
The planetary system was first discovered using a Transiting Exoplanet Survey Satellite, or TESS, a NASA space telescope launched in 2018 to discover new exoplanets. The system was then analyzed using ESA’s CHaracterising ExOPlanet Satellite, or Cheops, which was launched in 2019 to study stars that are already known to host exoplanets. The researchers also used data from other telescopes across the world, leading to a large international collaboration.
After they confirmed the odd finding of an “inside out” planetary system, the scientists tested some hypotheses to explain the presence of the outermost rocky planet, hoping to unders