A star is a
massive, luminous ball of ionized gas (or plasma)
that form in giant, slowly rotating clouds of dust called stellar nurseries. A cloud’s gravity
gradually causes it to condense into a sphere; as it collapses, this ball becomes
hotter and denser, eventually forming a protostar.
Under incredibly high
pressure, atoms that normally repel each other begin to collide and combine in
a process called nuclear fusion. In
the case of a new star, molecules of hydrogen collide to form helium. When the
protostar’s heat and pressure hit 1 million °C, fusion begins and the star ignites.