Star Formation & Fuel A
Star Formation & Fuel B
HR Diagram A
HR Diagram B
Galaxies
100

This cloud of gas and dust is the birthplace of all stars, pulled together by gravity.

stellar nebula

100

Our Sun is considered to be this type of star, based on its mass.

a low-mass or medium-mass star

100

This is the name for the graph that plots stars' luminosity and temperature.

the Hertzsprung-Russell Diagram (or HR-Diagram)

100

What can we tell by looking at a color of a star

the temperature

100

Where is our solar system located within our galaxy?

In Orion's Arm in the elbow of the arm

200

This is the longest and most stable phase of a star's life, where it fuses hydrogen into helium in its core.

the main sequence

200

This is the single most important factor that determines a star's lifespan and its final fate.

the stars mass

200

The property that is plotted on the X-axis of the HR-Diagram and is represented by a star's color

surface temperature

200

Located in the top-right of the diagram, these stars are very large and bright, but cool and red in color

red giants or supergiants

200

This is the most common galaxy shape, which has a rotating disk with spiral arms extending from a central bulge

Spiral

300

After using up the hydrogen in its core, our Sun will expand into this large, cool star. Which one

red giant

300

This is the massive, bright-red star that forms from a high-mass star after its main sequence stage.

red supergiant

300

Plotted on the Y-axis, this is a measure of a star's actual brightness or energy output

luminosity (or absolute magnitude)

300

ound in the bottom-left of the diagram, these stars are incredibly hot but very dim and small

white dwarfs

300

This type of galaxy is shaped like a giant sphere or flattened oval and contains mostly older stars with little to no new star formation

Elliptical Galaxy

400

This beautiful, colorful cloud of gas is formed when a low-mass star sheds its outer layers at the end of its life.

planetary nebula

400

This cataclysmic stellar explosion marks the end of a high-mass star and creates and scatters heavy elements throughout the universe.

What is a supernova

400

This diagonal band contains about 90% of all stars, including our Sun, and represents the longest stage of a star's life.

the main sequence

400

A star in the upper-left corner of the HR-Diagram would have this color, indicating a very high surface temperature

blue

400

This is the name of our home galaxy

The Milky Way

500

This very dense, small object is the remaining core of a low-mass star after it has shed its outer layers.

white dwarf

500

This is the super-dense core left after a high-mass star collapses in a supernova. It has gravity so strong that even light cannot escape.

black hole

500

Our Sun's temperature and luminosity will place it on the HR-Diagram in this category for most of its life

main sequence star

500

A star in the upper-right corner of the HR-Diagram would have this color, indicating a very low surface temperature

red

500

This type of galaxy has no distinct, regular shape, often due to a collision or gravitational interaction with another galaxy

Irregular Galaxy

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