Star Birth & Basics
The Power of Fusion
Average Stars (The Sun’s Path)
High-Mass Superstars
Reading the H-R Diagram
100

This is a large cloud of gas and dust in space where all stars begin their lives.

What is a nebula?

100

This is the process where two lighter atoms join to form a heavier one, releasing massive amounts of energy.

What is nuclear fusion?

100

Our Sun is currently in this stable, middle-life stage where 90% of a star's life is spent.

What is the main sequence?

100

A high-mass star is defined as having more than this many times the mass of our Sun.

What is two (2x)?

100

The H-R Diagram plots stars based on these two main characteristics.

What are temperature (or color) and luminosity (or brightness/absolute magnitude)?

200

Gravity is the force that pulls particles of gas and dust together to form this "baby star," which is not yet hot enough for nuclear fusion.

What is a protostar?

200

In the core of a star, hydrogen atoms fuse together to create this heavier element.

What is helium?

200

This is the red, expanded stage of an average star that occurs after it runs out of hydrogen fuel.

 What is a red giant?

200

When a massive star runs out of fuel, it collapses and then explodes in this spectacular event.

What is a supernova?

200

On an H-R Diagram, stars that are hot but dim are found in this corner (usually White Dwarfs).

 What is the lower left?

300

This fundamental force is responsible for the formation of stars, planets, and even our entire solar system.

What is gravity?

300

A star is stable when the outward energy from nuclear fusion perfectly matches this inward-pulling force.

What is gravity?

300

After a red giant sheds its outer layers, it leaves behind this "ghostly" cloud of gas and dust.

What is a planetary nebula?

300

This is a final stage for a massive star; it is so dense that it collapses every proton into this neutral particle.

What is a neutron star?

300

As you move from right to left on the x-axis of an H-R Diagram, the star’s temperature does this.

What is increases (gets hotter)?

400

Stars are primarily made of this element, which they use as fuel during the main sequence stage.

What is hydrogen?

400

Scientists can tell a star is getting older when it contains more of this element and less hydrogen.

What is helium?

400

This is the final, white-hot, dense core left behind at the very end of an average star’s life cycle.

What is a white dwarf?

400

If a star is massive enough, its gravity is so strong that not even light can escape its pull.

What is a black hole?

400

These stars are found at the very top right of the H-R diagram because they are both very bright and relatively cool.

What are Supergiants (or Giants)?

500

To become a "true" star, the core must reach a temperature of at least this many degrees Kelvin to start nuclear fusion.

What is 10,000,000 (10 million) K?

500

When a star begins to die and expand into a giant, it starts fusing helium into this element, which is a building block for life.

What is carbon? 

500

Compared to high-mass stars, low-mass stars have a lifespan that is much _______.

What is longer? (They burn fuel slower).

500

Massive stars produce these heavy elements, like oxygen and iron, which are eventually blown into space to form new planets.

What are elements (or metals/heavy elements)

500

This term refers to how bright a star actually is from a standard distance, rather than how bright it looks from Earth.

What is absolute magnitude (or absolute brightness)?

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