After shining for many millions of years, stars end their lives, mainly, in two ways: very high mass stars die very
violently as supernovae, while low mass stars end as planetary nebulae.
Not exact matches
This calcium and other heavy elements could have been created in
supernova explosions, and then incorporated into new stars, but the clusters
as they are today are too small to keep hold of the material
violently thrown out by
supernovae.
A shock wave from that collapse will speed outward,
violently expelling the star's outer layers in a massive explosion known
as a
supernova.
Astronomers know that while large stars can end their lives
as violently cataclysmic
supernovae, smaller stars end up
as planetary nebulae — colourful, glowing clouds of dust and gas.
The
supernova explosions that follow further whip up those shock waves, and then
violently accelerate the material from previous
supernovas as well.