Astronomers may have just pushed the upper size limit of what counts as a planet, thanks to new insights into how giant worlds form.<\/p>\n
New observations from NASA’s James Webb Space Telescope<\/a> (JWST) suggest that even extremely massive gas giants<\/a> \u2014 once thought too large to form like ordinary planets \u2014 may grow through the same basic process, shifting how scientists differentiate massive planets from brown dwarfs.<\/p>\n <\/p>\n The findings come from a close look at the HR 8799 system, a young, sun-like star<\/a> about 133 light-years from Earth that hosts four enormous gas giants orbiting far from their parent star. Each world is between five and ten times the mass of Jupiter<\/a> \u2014 the largest planet in our own solar system \u2014 placing them near the fuzzy boundary between planets and brown dwarfs, which are substellar objects that fuse deuterium, rather than hydrogen like stars, earning them the nickname “failed stars,” according to a statement<\/a> from the University of California, San Diego.<\/p>\n You may like<\/p>\n For years, astronomers have debated whether planets this massive could form through core accretion, the slow, bottom-up process in which solid material clumps together<\/a> into a dense core that then pulls in vast amounts of gas. At extreme orbital distances, where material is sparse and protoplanetary disks fade quickly, many researchers thought this mechanism simply wouldn’t allow enough time for these planets to grow so large.<\/p>\n To test that assumption, the research team used the JWST’s powerful infrared spectrographs<\/a> to analyze the chemical makeup of the planets’ atmospheres. Instead of focusing on common gases like water vapor or carbon monoxide, the scientists searched for sulfur-bearing molecules \u2014 elements that typically begin as solid grains in a young protoplanetary disk and thus suggest the planet formed through core accretion, according to the statement.<\/p>\n The spectral data provided by the JWST revealed hydrogen sulfide in the atmosphere of HR 8799 c<\/a>, one of the system’s inner giants, providing strong evidence that the planet formed by first assembling a solid core before rapidly accreting gas. That chemical fingerprint is otherwise difficult to explain if the planet instead formed through a rapid, star-like collapse of gas. The team also found that the planets were more enriched in heavy elements, like carbon and oxygen, than their star, further supporting that they formed as planets.<\/p>\n “With the detection of sulfur, we are able to infer that the HR 8799 planets<\/a> likely formed in a similar way to Jupiter despite being five to ten times more massive, which was unexpected,” Jean-Baptiste Ruffio, lead author of the study, said in the statement.<\/p>\n Therefore, the study suggests that core accretion can operate efficiently even at extreme masses and distances, expanding the known limits of the planet-building process. If confirmed in other systems, the finding could force astronomers to rethink where \u2014 and how \u2014 the line between giant planets and brown dwarfs<\/a> is drawn.<\/p>\n