Life Cycle of a Star · seed 1 · A4, ink-friendly. The answer key prints on its own page for grown-ups.
The Life Cycle of a Star
Science · Space Systems & Earth's History · ages 13-14
Name ______________________ Date ____________
Which two endings are possible only for very massive stars?
White dwarf or red giant
Neutron star or black hole
Nebula or protostar
Look at the star's life cycle below. What is stage 1, the highlighted stage, called?
Nebula
Red giant
White dwarf
Nuclear fusion inside a star can build elements heavier than hydrogen and helium.
Circle one: TrueFalse
A star ten times heavier than the Sun finally runs out of fuel. What happens next?
It explodes as a supernova, leaving a neutron star or black hole
It quietly shrinks into a white dwarf
It turns back into a nebula
Put these stages of a Sun-like star in the order they happen.
Red giant, then nebula, then main sequence
Main sequence, then nebula, then red giant
Nebula, then main sequence, then red giant
Count the stages shown in this Sun-like star's life cycle. How many stages are there?
Answer: ______________
Two stars start as identical nebulae, but Star A is far more massive than Star B. What happens to each?
Both stars will always end the same way, since they started the same way
Star B will explode first because smaller stars burn fuel faster
Star A is more likely to end in a supernova and leave a neutron star or black hole, while Star B likely becomes a white dwarf
A classmate says the iron in your blood came from the Sun exploding. What's the mistake?
Iron does not come from stars at all
The Sun isn't massive enough to explode as a supernova; the iron came from a different, more massive star that died long ago
The Sun already exploded when the solar system formed
Answer key
For grown-ups. Fold this page away before handing over the rest.
The Life Cycle of a Star W1-mt_lHasFmgvnT-s1
Neutron star or black hole · Massive stars explode as a supernova and leave behind a neutron star or, if massive enough, a black hole.
Nebula · Every star's life starts inside a nebula, a cloud of gas and dust pulled together by gravity.
True · Fusion fuses lighter atoms into heavier ones, like carbon, oxygen, and iron.
It explodes as a supernova, leaving a neutron star or black hole · Only stars far more massive than the Sun end their lives in a supernova.
Nebula, then main sequence, then red giant · A star starts as a nebula, spends most of its life on the main sequence, then swells into a red giant.
5 · Nebula, protostar, main sequence, red giant, and white dwarf: five stages in all.
Star A is more likely to end in a supernova and leave a neutron star or black hole, while Star B likely becomes a white dwarf · A star's mass decides its ending: heavier stars burn fast and end dramatically, while lighter stars like the Sun end quietly.
The Sun isn't massive enough to explode as a supernova; the iron came from a different, more massive star that died long ago · Sun-like stars end quietly as white dwarfs. Making enough iron takes a supernova from a much more massive star.