Webb image archive

Protoplanetary Disk (Artist's Concept)  

This is an artist’s impression of a young star surrounded by a disk of gas and dust. An international team of astronomers has used NASA’s James Webb Space Telescope to study th...

Date
Jun 6, 2024
Observatory
James Webb Space Telescope
Credit
NASA / ESA / CSA / STScI
Archive ID
01HZ2NDC0Z5G822ZM3GTNMHK4X

This is an artist’s impression of a young star surrounded by a disk of gas and dust. An international team of astronomers has used NASA’s James Webb Space Telescope to study the disk around a young and very low-mass star known as ISO-ChaI 147. The results reveal the richest hydrocarbon chemistry seen to date in a protoplanetary disk.

The science team explored the region around ISO-ChaI 147, a very low-mass star of 0.11 solar masses. They found that the gas in the planet-forming region of the star is rich in carbon. This could mean that the building blocks for planets may lack carbon because all of the carbon-containing chemicals have evaporated and been lost into the surrounding gas. As a result, any rocky planets that form might be carbon-poor.

Credits

Illustration

NASA-JPL

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