The Beginnings our of Solar System
Origin of the Universe
Our Solar System
Celestial Motion
Solar Phenomena
100

A cloud of gas and dust from which the Sun and planets formed.

Solar Nebula

100

The force that pulls objects toward each other

Gravity

100

Planets with icy compositions (Uranus, Neptune).

Ice Giants

100

Stationary star at the center of our Solar System

Sun

100

A sudden burst of energy from the Sun.

Solar Flare

200

Approximately, how old is our Solar System?

4.6 billion years old

200

How scientists determine the chemical makeup of a star

Spectroscopy

200

Large planets made mostly of gas (Jupiter, Saturn)

Gas Giants

200

The spinning of Earth on its axis.

Rotation

200

Cooler, darker regions on the Sun indicating solar activity.

Sunspots

300

A developing star before nuclear fusion begins

Protostar

300

Approximately, how old is the Universe?

13.8 billion years old

300

Shape of Earth's orbit around the Sun

Almost perfectly circular

300

Term to describe the movement of Earth around the Sun.

Revolution

300

A stream of charged particles from the Sun.

Solar Wind

400

An early form of a planet created by accretion.

Protoplanet

400

Low energy radiation leftover after the Big Bang

Cosmic Background Radiation

400

The galaxy that contains our solar system.

Milky Way

400

Approximately what angle does Earth tilt as it rotates the Sun?

23.5

400

A large release of charged particles from the Sun.

Coronal Mass Ejection (CME)

500

The process of particles sticking together to form larger bodies.

Accretion

500
Wavelength of light increases and shifts towards red, indicating galaxies are moving away from Earth

Redshift

500

The distance light travels in one year.

Light-Year

500

The way celestial objects appear to move in the sky due to Earth’s motion.

Apparent Motion

500

What causes the Aurora Borealis (Northern Lights)?

Collision of charged particles from the sun and gases in Earth's atmosphere cause Aurora Borealis (Northern Lights)

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