‘Disk Detective’ Needs Your Help Finding Disks Where Planets Form

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 C√≥rdoba,
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

“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!”

About Disk Detective

Disk Detective is a NASA-funded
citizen science project that is part of the NASA-sponsored Zooniverse citizen science

Check out the revamped Disk Detective
project at:


Learn more about NASA Citizen
Science at:



NASA’s Jet Propulsion Laboratory
in Southern California managed and operated WISE for NASA’s Science Mission Directorate
from 2009 to 2011. Edward Wright at the University of California, Los Angeles was
the principal investigator. The mission was selected competitively under NASA’s
Explorers Program managed by the agency’s Goddard Space Flight Center in Greenbelt,
Maryland. In late 2013, the spacecraft was reactivated and renamed NEOWISE.

For more information
about NEOWISE, visit:



For more information
about WISE, visit:



News Media Contact

Calla Cofield

Jet Propulsion Laboratory, Pasadena, Calif.



Elizabeth Landau

NASA Headquarters




Source: Jet Propulsion Laboratory

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