The now world-famous James Webb Space Telescope detected the signs of carbon dioxide for the first time in the atmosphere of a planet outside of the solar system.
Although the exoplanet would never be able to support life as we know it, the successful discovery of carbon dioxide gives researchers hope that similar observations could be carried out on rocky objects more hospitable to life.
"My first thought: wow, we really do have a chance to detect the atmospheres of terrestrial-size planets," tweeted Natalie Batalha, a professor at the University of California at Santa Cruz and one of the hundreds who worked on the Webb project.
Their study of exoplanet WASP-39, a hot gas giant closely orbiting a star 700 light years away, will soon be published in the journal Nature.
"For me, it opens a door for future research on super-Earths (planets larger than Earth but smaller than Neptune), or even Earth-sized planets," Pierre-Olivier Lagage, an astrophysicist with France's Atomic Energy Commission (CEA), told Agence France-Presse (AFP).
The detection of carbon dioxide will also help scientists learn more about how WASP-39 formed, NASA said in a press release. The exoplanet, which orbits its star once every four Earth days, has a mass one-quarter that of Jupiter but a diameter 1.3 times bigger.
The frequency of its orbit and large atmosphere made WASP-39 an ideal candidate for an early test of Webb's state-of-the-art infrared sensor, known as NIRSpec.
Each time the exoplanet crosses in front of its star, it blocks out an almost imperceptible amount of light.
But around the edges of the planet, a tiny amount of light passes through the atmosphere.
Webb's highly sensitive NIRSpec can detect the small changes that the atmosphere has on the light, allowing scientists to determine its gas composition.
The Hubble and Spitzer telescopes had already detected water vapor, sodium, and potassium in WASP-39's atmosphere, but carbon dioxide can now be added to that list thanks to Webb and its NIRSpec instrument.
"It was a special moment, crossing an important threshold in exoplanet sciences," said Zafar Rustamkulov, a Johns Hopkins University researcher, in the NASA press release.
