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Help Discover Worlds With NASA

A picture of the night sky in Skull Valley Utah from June 2021 shows the constellation Scorpius to the upper right of the silhouette of a desert butte. The dark blue sky is filled with countless bright stars. Credit: NASA/Bill Dunford
Members of the public can help astronomers observe and study the night sky through NASA’s Universe of Learning Exoplanet Watch program.
NASA/JPL-Caltech/Bill Dunford

The Exoplanet Watch project invites you to use your smartphone or personal telescope to help track worlds outside our solar system.

More than 5,000 planets have been confirmed to exist outside our solar system, featuring a wide array of characteristics like clouds made of glass and twin suns. Scientists estimate there could be millions more exoplanets in our home galaxy alone, which means professional astronomers could use your help tracking and studying them.This is where Exoplanet Watch comes in. Participants in the program can use their own telescopes to detect planets outside our solar system, or they can look for exoplanets in data from other telescopes using a computer or smartphone.

Exoplanet Watch began in 2018 under NASA’s Universe of Learning, one of the agency’s Science Activation programs that enables anyone to experience how science is done and discover the universe for themselves. Until recently there were limits on how many people could help look through the data collected by other telescopes, but now this program is easily available to anyone. By following the site’s instructions, participants can download data to their device or access it via the cloud, and then assess it using a custom data analysis tool.

“With Exoplanet Watch you can learn how to observe exoplanets and do data analysis using software that actual NASA scientists use,” said Rob Zellem, the creator of Exoplanet Watch and an astrophysicist at NASA’s Jet Propulsion Laboratory in Southern California. “We’re excited to show more people how exoplanet science is really done.”

Helping Without a Telescope

Participants without telescopes can help astronomers comb through data that’s already been taken. The project has 10 years of exoplanet observations, collected by a small ground-based telescope south of Tucson, Arizona. This year, the project will start collecting additional data from two other telescopes at the Table Mountain facility in Southern California, which JPL manages.

These telescopes look at nearby stars and search for what scientists call exoplanet transits: regular dips in a star’s brightness caused by a planet passing between the star and Earth. Essentially, a transit is an observation of a planet’s silhouette against the bright glare of its star.

An infographic portrays an icon of a planet passing in front of a star and the measurement of the star's brightness dimming as the planet crosses the star, or transits.
A planet passing in front of its parent star creates a drop in the star’s apparent brightness, called a transit. Exoplanet Watch participants can look for transits in data from ground-based telescopes, helping scientists refine measurements of the length of a planet's orbit around its star.
NASA’s Ames Research Center

Multiple NASA telescopes look for exoplanet transits as a way to discover new planets, but Exoplanet Watch participants primarily observe transits by planets that have already been discovered to gain more information about their orbits. The time between exoplanet transits reveals how long it takes an exoplanet to orbit its parent star; the more transits that are measured, the more precisely the length of the orbit is known. If the timing of the orbit isn’t measured precisely, scientists who want to study those planets in more detail with large ground-based or space-based telescopes can lose valuable observing time while they wait for the planet to appear. Having volunteers sort through the data will save significant computing and processing time.

Exoplanet Watch participants will also look for variations in the apparent brightness of stars – changes caused by features such as flares (outbursts of light) and star spots (dark spots on a star’s surface). In transit measurements, these changes make a planet appear smaller or larger than it actually is. This work will help scientists anticipate the variability of a particular star before they study its exoplanets with large, sensitive telescopes like NASA’s James Webb Space Telescope.

The welcome page for the EXOTIC software program for Exoplanet Watch. Convert images into important data for scientific discovery. Use of EXOTIC requires a Google or Gmail account. Links are provided for the basic tutorial.
Participants in NASA’s Universe of Learning Exoplanet Watch will use the EXOplanet Transit Interpretation Code (EXOTIC) software to analyze data. No experience is necessary, and the project website includes tutorials and guides.

Helping With Your Own Telescope

Want to take your own data? Although the number of targets you can see increases with the size of the telescope used, there’s no minimum size requirement. For example, Exoplanet Watch can help you detect exoplanet transits for hundreds of nearby stars with just a 6-inch (15-centimeter) telescope.

Exoplanet Watch combines observations of the same target by multiple sky watchers in order to get a higher-fidelity measurement. Combining observations is also useful if the planet’s transit lasts longer than the time a star is visible in the sky for a single observer: Multiple participants at different locations around the globe can collectively watch the duration of a long transit.

That was the case with a planet called HD 80606 b, which Webb will observe this year. A recent study of this planet led by Kyle Pearson, the Exoplanet Watch deputy science lead at JPL, combined observations from more than 20 Exoplanet Watch participants. The volunteer effort on HD 80606 b will free up almost two hours of time on Webb for other observations. And on missions that aim to observe hundreds or thousands of exoplanets, the number of minutes saved by refining planet transit measurements can add up and free a significant amount of observing time, according to Zellem.

One of the program’s policies requires that the first paper to make use of the observations or analysis done by volunteers will list those volunteers as co-authors, which was the case with the study led by Pearson. “I hope this program lowers barriers to science for a lot of people and inspires the next generation of astronomers to join our field,” said Zellem.