Sunny Side Up
Core Chemistry
The Pressure's On
Endgame
Alternate Realities
100

This is the current life stage of our Sun.

What is main sequence?

100

The energy released from fusion comes from this.

What is a loss of mass?

100

Pressure from fusion creates this state of balance in a star.

What is hydrostatic equilibrium?

100

The most massive stars cannot stop the force of gravity and become these deep space objects.

What are black holes?

100

In a universe where hydrogen fusion resulted in more mass, this is the end state of all stars.

What is a brown dwarf?

200

After the main sequence, in about 4 billion years, the Sun will become this.

What is a red giant?

200

This is the most massive element produced in stars much bigger than our sun.

What is iron?

200

Without gravity, stars could not form from this deep sky object.

What is a nebula?

(What is a molecular cloud?)

200

This determines what a star's final form will be.

What is mass?

200

Imagine stars fused hydrogen into helium and then could not fuse helium. We would likely not observe these stars.

What are giants?

300

98% of the Sun is composed of these two elements.


What is hydrogen and helium?

Bonus question (300 points).

The percentage of the sun that is currently helium.

300

Fusion takes place in this part of the star.

What is the core?

300

Daily Double opportunity!

If a star does not have enough hydrogen for fusion, what occurs? Be descriptive! Your answer will likely need to be multiple sentences, and it does not need to be in jeopardy format.
300

This is the fate of a small star that cannot support fusion.

What is a brown dwarf?

300

If gravity were weaker, this would happen to the number of stars formed, due to insufficient compression and core heating during star formation.

What are fewer stars?

400

When the Sun dies, it will primarily be composed of these elements.

What is carbon and oxygen.

400

For this reason, stars cannot fuse elements that are more massive than iron.

What is fusion becomes endothermic?


(or what is nucleons gain mass)

400

In neutron stars, this kind of pressure resists further collapse.

What is neutron degeneracy pressure?

Bonus question! (400 points)

In white dwarfs, this kind of pressure resists further collapse.

400

Daily Double opportunity!

Draw an HR Diagram on your whiteboards. Circle the region that is an "endgame."

400

Imagine our universe was made primarily of oxygen and carbon instead of hydrogen and helium. All currently fusing stars would be a part of this stage.

What is a giant?

500

When the Sun dies, it will create these two objects.

What is a white dwarf and a planetary nebula.

500

For hydrogen fusion to occur, hydrogen must overcome this force with immense temperatures and pressures.

What is the electromagnetic force?

Bonus question (500 points).

This force is responsible for fusion.

500

While a nebula is contracting, energy is transferred between these two types of energy.

What is gravitational potential energy and heat (kinetic)?

500

A star more massive than our Sun (but not TOO massive) will form these two objects in its violent death.

What are supernova remnant and neutron star.

500

If we could see the cores of stars instead of their outer layers, stars across the sky would appear more like this color, due to the extreme temperatures at their centers.

What is blue?