The vital role of a carbon molecule called methyl cation (CH3+) in interstellar carbon chemistry was predicted in the 1970s, but the unique capabilities of the NASA/ESA/CSA James Webb Space Telescope have finally made observing it possible — in a region of space where planets capable of accommodating life could eventually form. This image taken by Webb’s Near-Infrared Camera shows a part of the Orion Nebula known as the Orion Bar. It is a...
