protostellar coreThe smallest opaque clump into which a collapsing interstellar cloud fragments. The characteristic mass of a protostellar core is about 0.01 solar mass. It subsequently grows by accretion as surrounding matter falls toward it, attaining stellar mass, and becoming a protostar, within 100,000 years after its initial formation. Related entry• variable starsRelated category• TYPES OF STARAlso on this site: Encyclopedia of Alternative Energy & Sustainable Living Encyclopedia of History |