Kepler's Laws
The Solar System
Coevolution of Earth and Life
The Role of Oxygen
Probability of Life Elsewhere
100

Planets orbit around the Sun in elliptical orbits according to this law.

Kepler's First Law

100

This planet is third from the Sun and located in the habitable zone of our solar system.

Earth

100

This process describes how Earth and life have changed and grown together over time.

Coevolution

100

This material found in red beds and banded iron formations formed from the reaction of free oxygen in the air with iron in rocks.

Rust
200

A planet is moving fastest when it is at this point in its orbit.

Perihelion

200

Rocks can be classified as sedimentary, igneous, or metamorphic based primarily upon differences in their

Origin

200

This process began releasing oxygen into the atmosphere about 2.7 billion years ago.

Photosynthesis

300

According to Kepler's Second Law, planets sweep out equal areas in equal this.

Equal time
300

During this period of time about 500 million years after the solar system formed, the Earth and other inner planets were being struck with asteroids.

The Late Heavy Bombardment

300

Earth's fossil record shows evidence that more complex life-forms probably emerged from less complex life-forms through this process.

Evolution

300

These processes break up and move rocks to different locations.

Weathering, erosion, and deposition

300

These types of events can wipe out 70, 80, or even up to 90% of life in a very short period of time.

Mass extinction events

400

According to Kepler's Third Law, the greater distance a planet is from the Sun, the greater its this.

Orbital period (length of year)

400

In this type of model, the Sun, other stars, and the Moon orbit around the Earth.

Geocentric

400

This protective layer in the atmosphere is formed by three oxygen molecules bound together.

Ozone layer

500

This planet’s orbit around the Sun is most nearly circular.

Venus (0.007)

500

This process measures the amount of a decayed isotope in order to determine the age of an object.

Radiometric dating (radioactive dating)

500

This life-form appeared first, and is our earliest undisputed evidence of life from about 3.5 billion years ago.

Stromatolite

500

Oxygen was very toxic and killed off these types of organisms who were unable to utilize it to produce energy.

Anaerobic

500

This equation attempts to estimate the number of intelligent civilizations we can communicate with.

The Drake Equation

M
e
n
u