First Detection of Carbon Dioxide on Exoplanets Revealed by James Webb Space Telescope

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Scientists have made a groundbreaking discovery by detecting carbon dioxide (CO2) on four exoplanets located in the HR 8799 system, approximately 130 light-years from Earth. This finding, reported in The Astronomical Journal, suggests that these giant planets likely formed similarly to Jupiter and Saturn, through a core accretion process. William Balmer, an astrophysicist at Johns Hopkins University, emphasized the significance of identifying heavier elements in the atmospheres of these planets, which provides insights into their formation.

The HR 8799 system is relatively young, at 30 million years, and emits significant infrared light, allowing researchers to analyze its characteristics and compare them to our solar system. Balmer stated that understanding these exoplanets could illuminate the habits of Earth-like planets in the future. The James Webb Space Telescope played a crucial role in this discovery, using its coronagraphs to block starlight and directly measure the atmospheric composition of these distant worlds. Future observations are planned to explore the commonality of such formations among other long-period exoplanets.

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