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NASA’s James Webb spots carbon dioxide in a planet beyond our solar system

The James Webb Space Telescope captures the first direct images of carbon dioxide in a distant planetary system, HR 8799, providing new insights into planet formation and supporting the core accretion theory.
March 19, 2025 / 17:49 IST
NASA’s James Webb Space Telescope has provided the clearest look in the infrared yet at the iconic multi-planet system HR 8799. The closest planet to the star, HR 8799 e, orbits 1.5 billion miles from its star, which in our solar system would be located between the orbit of Saturn and Neptune. (Image: NASA)

The James Webb Space Telescope has taken a major step forward. It has captured the first direct images of carbon dioxide in a distant planetary system. This system, known as HR 8799, lies 130 light-years away. The discovery offers new insights into planet formation, NASA confirmed.

Webb’s advanced coronagraphs played a crucial role in this finding. These instruments block bright starlight to reveal hidden planets. This allowed scientists to focus on infrared wavelengths and detect gases. The presence of carbon dioxide supports the core accretion theory. This process also shaped Jupiter and Saturn in our solar system.

The HR 8799 system is just 30 million years old. Its young planets still radiate heat from their formation. This makes them ideal for studying planetary evolution. Scientists compare these planets with stars and brown dwarfs. They aim to understand different planet formation processes.

New Insights Into Planet Formation

There are two main ways giant planets form. One is core accretion, where solid cores slowly collect gas. The other is disk instability, where planets collapse from a cooling disk. Studying HR 8799 can help determine which process is more common.

"By detecting carbon dioxide, we see heavy elements like carbon and oxygen," said William Balmer of Johns Hopkins University. "Since we know the star’s composition, this supports core accretion."

Future of Exoplanet Imaging

Directly imaging exoplanets remains a challenge due to their faintness. The James Webb Telescope is changing this with its advanced technology. It can now capture planets at specific wavelengths. This will help scientists distinguish between planets and brown dwarfs.

"Our goal is to compare our solar system with others," Balmer added. "We want to see if our system is unique or common."

This discovery marks a step forward in exoplanet research. It brings scientists closer to understanding planet formation. Webb’s capabilities will continue unlocking secrets of the universe.

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