Artist's rendering of proto-planetary disk.

Artist's rendering of a young, Sun-like star encircled by its planet-forming disk of gas and dust. Credit: NASA/JPL-Caltech

Planets form from gas and dust particles swirling around baby stars in enormous spinning disks. But because this process takes millions of years, scientists can only learn about these disks by finding and studying a lot of different examples.

Through a project called Disk Detective, you can help. Anyone, regardless of background or prior knowledge, can assist scientists in figuring out the mysteries of planet formation. Disk Detective is an example of citizen science, a collaboration between professional scientists and members of the public.


Members of the public can help scientists learn how planets form by sifting through data from NASA's WISE mission, managed by the agency's Jet Propulsion Laboratory.

Planets form from gas and dust particles swirling around baby stars in enormous spinning disks. But because this process takes millions of years, scientists can only learn about these disks by finding and studying a lot of different examples.

Through a project called Disk Detective, you can help. Anyone, regardless of background or prior knowledge, can assist scientists in figuring out the mysteries of planet formation. Disk Detective is an example of citizen science, a collaboration between professional scientists and members of the public.

"We're trying to understand how long it takes for planets to form," said astrophysicist Marc Kuchner, the Disk Detective project lead at NASA's Goddard Space Flight Center in Greenbelt, Maryland, and the Citizen Science Officer for NASA's Science Mission Directorate. "Tracing the evolution of these disks is the main way that we know how long planet formation takes."

Disk Detective has just relaunched with a new website and a new dataset of about 150,000 stars. This new version of the project focuses on M dwarfs, which represent the most common type of star in the Milky Way galaxy. It also concentrates on brown dwarfs, which are balls of gas that don't burn hydrogen the way stars do and often more closely resemble giant planets like Jupiter.

After reading the instructions, participants can start identifying disks right away in Disk Detective. The interface presents a series of real astronomical images and asks visitors questions that will help determine more definitively if a disk is present. The images come from NASA's Wide-Field Infrared Survey Explorer (WISE), which now operates as NEOWISE, as well as the ground-based Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) in Hawaii and the NASA-funded Two Micron All-Sky Survey (2MASS), which operated from 1997 to 2001.

"We have multiple citizen scientists look at each object, give their own independent opinion, and trust the wisdom of the crowd to decide what things are probably galaxies and what things are probably stars with disks around them," said Disk Detective's director, Steven Silverberg, a postdoctoral researcher at Massachusetts Institute of Technology's Kavli Institute for Astrophysics and Space Research.

Advanced users learn more about the objects they're studying using professional data archives. Those who contribute substantial insight receive credit on scientific papers describing the discoveries made through Disk Detective's efforts. Professional scientists then follow up on citizen scientists' input using more sophisticated tools and new observations. Fifteen citizen scientists have already become named co-authors on peer-reviewed scientific papers through Disk Detective.

One enthusiastic Disk Detective "superuser" is Hugo Durantini Luca, a computer technician in Córdoba, Argentina. He began classifying disks with the project in 2014 and since then has taken on additional responsibilities: writing tutorials, moderating discussions, and even helping use telescopes in South America to follow up on interesting targets. While he became involved because of his interest in detecting planetary systems and analyzing images, he says he highly values "the way you are able to work with the science team directly." He is in frequent communication with Kuchner and other professional astronomers, and he participates in a weekly video call for superusers.

"I think we are going to have an interesting new season," Durantini Luca said. "The new way we are processing the data will allow us to analyze the image[s] with better detail."

Citizen scientists at Disk Detective made an important discovery in 2016: a new class of disks, called Peter Pan disks. Most disks around young, low-mass stars should lose their gas, due to planet formation and natural dissipation into space, after 5 million years. Yet Disk Detective citizen scientists discovered a disk with plenty of gas orbiting a star that is roughly 45 million years old.

Since then, seven similar mysteriously young-looking disks have been found, each at least 20 million years old. Scientists are still puzzling out why planet formation goes on for so long in these disks. They predict that citizen scientists may find as many as 15 new Peter Pan disks through the newly revamped Disk Detective.

"To figure out how disks evolve, we need a big sample of different kinds of disks of different ages," Kuchner said.

More recently, Disk Detective's efforts resulted in a discovery announced on June 2 at the American Astronomical Society's (AAS) 236th meeting, which was held virtually. With the help of citizen scientists, astronomers identified the closest young brown dwarf disk yet, one that may have the capability to form planets. This 3.7-million-year-old brown dwarf, called W1200-7845, is about 333 light-years away. A light-year is the distance light travels in one year; the closest star beyond the Sun is over 4 light-years away.

"There are not many examples of young brown dwarfs so close to the Sun, so W1200-7845 is an exciting discovery," said Maria Schutte, a predoctoral graduate student at the University of Oklahoma, who led the study and presented the findings at the AAS meeting. Durantini Luca and other citizen scientists were included as coauthors.

Since the last Disk Detective data release, ESA's (European Space Agency's) Gaia satellite has delivered an unprecedented bounty of information about the locations, movements, and types of stars in the Milky Way. The Disk Detective science team used the new data from Gaia to identify M dwarfs of interest to the project. A second improvement to the project is that the new images from the surveys listed above have higher resolution than the previous batch of data, making more background objects visible.

"NASA needs your help," Kuchner said. "Come discover these disks with us!"