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Activity
NASA

Exploring Exoplanets with Kepler

For Teachers 6th - 12th Standards
Calculate the movement and properties of planets like professional astronomers! Scholars use Kepler's third law to find Mercury and Venus's distance from the sun. Using changes in brightness of distant stars and Kepler's third law,...
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Interactive
Las Cumbres Observatory

Agent Exoplanet

For Students 6th - 12th
Not everything revolves around the sun! Believe it or not, there are planets, called exoplanets, that orbit stars other than our sun. Learners use an interactive online resource to research several of these planets. They learn about the...
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Lesson Plan
PBS

Data Plots of Exoplanet Orbital Properties

For Teachers 9th - 12th Standards
Scientists discovered the first exoplanet in 1995 and by early 2018, they confirmed the existence of more than 3,700—that's a lot of data! As part of the PBS 9-12 Space series, scholars interpret data about exoplanets. They compare...
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Interactive
PBS

Analyzing Light Curves of Transiting Exoplanets

For Teachers 9th - 12th Standards
Scientists detected exoplanets by measuring how the brightness of stars changed over time. Young astronomers interpret and analyze the same data that led to exoplanet discoveries. They learn to apply light curve graphs and connect the...
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Lesson Plan
PBS

Light Curves of Kepler's First Five Discoveries

For Teachers 9th - 12th Standards
The Kepler missions discovered and confirmed more than 2,650 exoplanets to date. A video shares the data from the first five discoveries. It provides graphs and diagrams to put each discovery in perspective to help scholars discuss the...
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Lesson Plan
PBS

Exoplanets through Kepler’s Laws

For Teachers 9th - 12th Standards
The majority of all confirmed exoplanets relied on Kepler's laws to discover their locations. Scholars learn how to apply Kepler's laws and then practice using data to discover exoplanets. They benefit from NASA video footage, NOVA...
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Lesson Plan
Space Awareness

The Engine of Life

For Teachers 5th - 11th Standards
There is a specific zone, or distance from a star, that a planet must be in order to have water in a liquid form. The activity demonstrates how flux density depends on its distance from the source. A photovoltaic cell gets power to drive...