WASP-39 b was already on scientists’ radar. In 2018 NASA’s Spitzer Space Telescope revealed hints of carbon dioxide in its atmosphere. Previous observations from other telescopes had revealed water vapor, sodium, and potassium.

Thus the exoplanet was the ideal candidate for a follow-up using the new and improved JWST, said López-Morales.

Another factor: WASP-39 b is a transiting planet. During a transit, some of the starlight is eclipsed by the planet completely, causing overall dimming, and some is transmitted through the atmosphere. The atmosphere filters out some colors more than others depending on what it is made of, how thick it is, and whether there are clouds. Because different gases absorb different combinations of colors, researchers can analyze small differences in brightness of the transmitted light across a spectrum of wavelengths to determine the exact make-up of an atmosphere.

In this case, the resulting spectrum scientists obtained was significant: the first clear, detailed, indisputable evidence for carbon dioxide ever detected in a planet outside our solar system.

“The remarkably strong signal is a testament to [JWST’s] exquisite precision and revolutionary wavelength range, and demonstrates how much we stand to learn from this awesome observatory,” Kirk said.