When it comes to searching for newly born planets that are tens, if not hundreds, if not thousands of light years away, we don’t often get too lucky. Planets are formed in thick clouds of dust and gas, known as protoplanetary discs, that swirl around a star. As such, it’s very difficult to observe young planets directly through all the debris. Instead scientists must rely on clues that might infer the presence of a protoplanet, but most of those clues are pretty circumstantial at best.
But Feng Long, a postdoctoral fellow at the Harvard-Smithsonian Center for Astrophysics, has discovered a new clue that might indicate a protoplanet’s existence – material at the Lagrange points. Sifting through data from Chile’s Atacama Large Millimeter/submillimeter Array (ALMA) pertaining to protoplanetary disc LkCa 15,…