“Dirty snowballs” have joined together since the planets formed
Across cosmic time and space, stellar systems form. This image shows the Orion Molecular Clouds, the target of the VANDAM survey. Yellow dots are the locations of the observed protostars on a blue background image made by Herschel. Side panels show nine young protostars imaged by ALMA (blue) and the VLA (orange). Protoplanetary disks not only are rich in organic molecules, but contain species that are not often seen in typical interstellar dust clouds. For several million years after the protostar phase completes and the star reaches equilibrium, circumstellar gas-rich material can persist. Credit: ALMA (ESO/NAOJ/NRAO), J. Tobin; NRAO/AUI/NSF, S. Dagnello; Herschel/ESA Molecular gas clouds contract, fragment, and portions of it collapse. This false-color look inside the star-forming region G333.23–0.06 shows ALMA data of multiple systems of high-mass protostars. Within these clumps of matter, ALMA has found multi-star systems, with singlet stars being a relative rarity. Credit: S. Li, MPIA / J. Neidel, MPIA Graphics Department; Data: ALMA Observatory Some fragmented regions form protostars, surrounded by a protoplanetary disk. This planet-forming protoplanetary disk, IRAS 04302+2247, …



