Image List

In this artist's conception, planets form from the gas and dust in the protoplanetary disk surrounding a young star. The gas is made up of many different molecules, including hydrogen cyanide and more complex nitriles—linked to the development of life on Earth. The soup of molecules in a particular location in the disk shapes the future of the planet forming there and determines whether or not that planet could support life as we know it.

This composite image of ALMA data from the young star HD 163296 shows hydrogen cyanide emission laid over a starfield. The MAPS project zoomed in on hydrogen cyanide and other organic and inorganic compounds in planet-forming disks to gain a better understanding of the compositions of young planets and how the compositions link to where planets form in a protoplanetary disk.