A typical dense core of an interstellar gas & dust cloud might have a density of 100 hydrogen atoms per cubic centimeter and a temperature of ~15 K. Roughly how massive must such a cloud be in order to become unstable to gravitational collapse and begin to form stars?

Choose one answer

Type a concept, like “slope” or “photosynthesis”.

↑ ↓ to choose · Enter to openSearch explanations and problems