1. You can often predict how a baby will look as an adult by looking at other family members.
Astronomers observe stars of different ages to infer how stars evolve.

2. How Stars Form
How do stars form?
A star is formed when a contracting cloud of gas and dust becomes so dense and hot that nuclear fusion begins.

3. How Stars Form
A nebula is a large cloud of gas and dust spread out over a large volume of space.
Some nebulas are glowing clouds lit from within by bright stars.
Other nebulas are cold, dark clouds that block the light from more-distant stars beyond the nebulas.

4. How Stars Form
A contracting cloud of gas and dust with enough mass to form a star is called a protostar.
As a protostar contracts, its internal pressure and temperature continue to rise.
Pressure from fusion supports the star against the tremendous inward pull of gravity.

5. How Stars Form
A group of bright young stars can be seen in the hollowed-out center of the Rosette Nebula.
Can you formulate a picture of how this happens?

6. Adult Stars
What determines how long a star remains on the main sequence?
A star’s mass determines the star’s place on the main sequence and how long it will stay there.

7. The Death of a Star
What happens to a star when it runs out of fuel?
The dwindling supply of fuel in a star’s core ultimately leads to the star’s death as a white dwarf, neutron star, or black hole.

8. The Death of a Star
When a star’s core begins to run out of hydrogen, gravity gains the upper hand over pressure, and the core starts to shrink.
The core temperature rises enough to cause the hydrogen in a shell outside the core to begin fusion.
The energy flowing outward increases, causing the outer regions of the star to expand. The expanding atmosphere moves farther from the hot core and cools to red.
The star becomes a red giant.

9. The mass of a star determines the path of its evolution.
The Death of a Star
The mass of a star determines the path of its evolution.
Where would you predict our sun to end up at?

10. Low- and Medium-Mass Stars
The Death of a Star
Low- and Medium-Mass Stars
Low-mass and medium-mass stars, which can be as much as eight times as massive as the sun, eventually turn into white dwarfs.
Stars remain in the giant stage until their hydrogen and helium supplies dwindle and there are no other elements to fuse.
The energy coming from the star’s interior decreases.
With less outward pressure, the star collapses.

11. The Death of a Star
The dying star is surrounded by a glowing cloud of gas, called a planetary nebula.
As the dying star blows off much of its mass, only its hot core remains.
This dense core is a white dwarf. A white dwarf is about the same size as Earth but has about the same mass as the sun.
White dwarfs don’t undergo fusion, but glow faintly from leftover thermal energy.

12. The Death of a Star
Planetary nebulas, such as the Hourglass Nebula, are clouds of gas that surround a collapsing red giant.

13. The Death of a Star
The Crab Nebula is the remnant of a supernova explosion that was observed on Earth in A.D The supernova was so bright that people could see it in the daytime.
Construct a public point of view of the event at the time.

14. The Death of a Star High-Mass Stars
The life cycle of high-mass stars is very different from the life cycle of lower-mass stars.
As high-mass stars evolve from hydrogen fusion to the fusion of other elements, they grow into brilliant supergiants, which create new elements, the heaviest being iron.
A high-mass star dies quickly because it consumes fuel very rapidly.

15. The Death of a Star
As fusion slows in a high-mass star, pressure decreases.
Gravity eventually overcomes the lower pressure, leading to a dramatic collapse of the star’s outer layers.
This collapse produces a supernova, an explosion so violent that the dying star becomes more brilliant than an entire galaxy.

16. Supernovas produce enough energy to create elements heavier than iron.
The Death of a Star
Supernovas produce enough energy to create elements heavier than iron.
These elements, and lighter ones such as carbon and oxygen, are ejected into space by the explosion.
As a supernova spews material into space, its core continues to collapse.

17. The Death of a Star
If the remaining core of a supernova has a mass less than about three times the sun’s mass, it will become a neutron star, the dense remnant of a high-mass star that has exploded as a supernova.
In a neutron star, electrons and protons are crushed together by the star’s enormous gravity to form neutrons.
Neutron stars are much smaller and denser than white dwarfs.

18. The Death of a Star
A neutron star spins more and more rapidly as it contracts. Some neutron stars spin hundreds of turns per second!
Neutron stars emit steady beams of radiation in narrow cones.
A spinning neutron star that appears to give off strong pulses of radio waves is called a pulsar.

19. The Death of a Star
Pulsars emit steady beams of radiation that appear to pulse when the spinning beam sweeps across Earth.
Hypothesis the results if this happen close to the earth?

20. The Death of a Star
If a star’s core after a supernova explosion is more than about three times the sun’s mass, its gravitational pull is very strong.
The core collapses beyond the neutron-star stage to become a black hole.
A black hole is an object whose surface gravity is so great that even electromagnetic waves, traveling at the speed of light, cannot escape from it.

21. Assessment Questions
As a protostar contracts, what happens to its pressure and temperature?
They stay constant.
The temperature increases while the pressure stays constant.
They both decrease.
They both increase.

22. Assessment Questions
As a protostar contracts, what happens to its pressure and temperature?
They stay constant.
The temperature increases while the pressure stays constant.
They both decrease.
They both increase. ANS: D

23. Assessment Questions
Which type of main sequence star would be likely to remain in the main sequence for about 100 billion years?
red
yellow
white
blue

24. Assessment Questions
Which type of main sequence star would be likely to remain in the main sequence for about 100 billion years?
red
yellow
white
blue ANS: A

25. Assessment Questions
Based on its position on the H-R diagram, what will the sun become when it finally runs out of fuel?
nebula
supernova
neutron star
white dwarf

26. Assessment Questions
Based on its position on the H-R diagram, what will the sun become when it finally runs out of fuel?
nebula
supernova
neutron star
white dwarf ANS: D