UNITE: Unistellar Network Investigating TESS Exoplanets
A NASA Citizen Science project

Use your telescope to confirm the existence of newly discovered worlds

Join the worldwide Unistellar Network of citizen scientists and professional astronomers to discover and characterize some of the most interesting exoplanets in our galaxy!

Giant exoplanets resembling Jupiter that have been recently discovered by TESS, NASA’s current exoplanet hunting mission, need your help. Astronomers don’t have enough information to fully understand the orbits of these planets, which take months or years to circle their star once. This is usually because TESS and other telescopes haven’t had many chances to catch the temporary dimming of the exoplanet’s star as the planet passes, or transits, in front it.

This is where you and UNITE come in! Only a network of people around the world, cooperating to observe the same target, will be able to catch more transits by these exoplanets. This can be because these planets take many hours to transit their star (much longer than a single night on Earth) or because the dates of future transits cannot yet be accurately predicted. With your observations, scientists can understand the orbits and conditions of these foreign worlds like never before.

Explore below to learn about exoplanets or get started tonight!

Don’t have a Unistellar telescope? Here’s how you can still be part of the UNITE mission.

Featured Exoplanet Transit for March 2023:

Observation dates: 12 March – 13 March

We need your help investigating the orbit of Kepler-1704b, a flash-heated planet!

Kepler-1704b is a giant exoplanet discovered by the Kepler space telescope in 2009, but since then, only one other transit has been observed! This is in part because Kepler-1704b’s orbit takes 989 days (2.7yrs) and is one of the most eccentric, or oblong, orbits ever found among exoplanets (as shown above in comparison to planetary orbits in our Solar System). This orbit takes Kepler-1704b far away from its Sun-like star before swooping in for a close pass that heats the gaseous exoplanet over a thousand degrees Fahrenheit. This huge change in distance from its star means this planet’s temperature changes drastically over the course of its year, and its atmosphere may even “defrost” as it gets flash-heated near its star. This atmospheric action makes it a great target for JWST, so join the efforts and help astronomers understand Kepler-1704b’s orbit and prepare for potential future observations of its atmosphere!

Join this mission and learn more at the Pick Your Target page!

Featured Results: TOI 1812.01

In the first of several NASA-sponsored exoplanet hunts in 2022, Citizen Astronomers searched for a transit of TOI 1812.01. This planet, the outermost of three gaseous planets around a relatively cool star, is Saturn-sized with its radius nine times the size of Earth’s. Despite having two transits observed by TESS, its period (the length of its year) was poorly known: previous estimates ranged from 71 – 157 days. To nail down the orbit, 20 Citizen Astronomers tracked TOI 1812.01 for three nights over the course of two months. Only on the third night, August 27, did they spot the exoplanet and confirm that it takes 112 days to orbit its star.

Meet the Team

Meet the SETI Institute scientists behind the Unistellar Network’s NASA-Sponsored Exoplanet Programs:

Paul Dalba, PhD – Exoplanets Lead, Observation Planning, Data Analysis
Tom Esposito, PhD – UNITE Principal Investigator, Exoplanets Co-Lead, Pipeline Development
Lauren Sgro, PhD – Data Analysis, Communications
Franck Marchis, PhD – Outreach, Communications