James Webb telescope discovers carbon compounds crucial to life in star system 1,000 light-years from Earth

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Atoms are like Lego bricks: Each little building block combines to make something more complicated — from molecules, to enzymes, to DNA. For the first time, astronomers have detected a crucial step in this process: the molecule methyl cation (CH3+), which plays an important role in creating the complex carbon chemistry required for life as we know it. Astronomers described the first-of-its-kind detection in a study published June 26 in the journal Nature.

This particular swath of methyl cation lives in a protoplanetary disk called d203-506. This infant solar system is located in the Orion Nebula, about 1,350 light-years from Earth. Astronomers made the observations thanks to NASA’s powerful James Webb Space Telescope (JWST), which can resolve smaller details than past telescopes could. It can also pick out the signatures of specific molecules — also called molecules’ emission lines — with great precision.

Related: 25 gorgeous nebula photos that capture the beauty of the universe

These Webb images show a part of the Orion Nebula known as the Orion Bar. The largest image, on the left, is from Webb’s NIRCam (Near-Infrared Camera) instrument. At upper right, the telescope is focused on a smaller area using Webb’s MIRI (Mid-Infrared Instrument). At the very center of the MIRI area is a young star system with a protoplanetary disk named d203-506. The pullout at the bottom right displays a combined NIRCam and MIRI image of this young system. (Image credit: ESA/Webb, NASA, CSA, M. Zamani (ESA/Webb), and the PDRs4All ERS Team)

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