Astrophysicists Locate 100 New Sunny Neighbors with Citizens’ Help
UC San Diego team contributes to breakthrough discovery, enriching history of the universe
- Cynthia Dillon
- Cynthia Dillon - email@example.com
- Cynthia Dillon
The sun’s neighborhood just got a little more crowded. A new discovery by the Backyard Worlds team of citizen scientists and international astrophysicists, including researchers from UC San Diego, shows that about 100 cool brown dwarfs, never before observed, are in residence in the solar community. This treasure trove of discoveries has also uncovered a missing link within the local brown dwarf population. The findings will be published in the August 20, 2020 issue of The Astrophysical Journal and are available in preprint format on arXiv.org.
Brown dwarfs are celestial objects that are categorized between the most massive planets and the smallest stars. Lacking the mass to sustain nuclear reactions at their core, brown dwarfs are sometimes referred to as “failed stars,” or, because of their cool atmospheres and planet-sized diameters, “super Jupiters.” The small sizes and low temperatures of these objects make them extremely faint, so searches for the very coldest brown dwarfs focus on the immediate neighborhood of the sun, otherwise they would be too distant to detect. Discovering and characterizing these astronomical neighbors is fundamental to understanding the history of the universe and our place in it.
“These free-floating new worlds offer the opportunity for insights into the formation and atmospheres of planets beyond the solar system,” said Aaron Meisner, lead author of the paper and assistant scientist at the National Science Foundation’s (NSF) NOIRLab’s Astro Data Lab facility. “This collection of cold brown dwarfs also allows us to accurately estimate the number of free-floating planets roaming interstellar space near the sun.”
UC San Diego’s Professor of Physics Adam Burgasser and researchers from the Cool Star Lab contributed to the breakthrough discovery. The Cool Star Lab team used the sensitive Near-Infrared Echellette Spectrometer, or NIRES, instrument on the 10-meter W. M. Keck Observatory on Maunakea, Hawaii, to identify several of the faintest and coolest of the newly discovered brown dwarfs.
“We used NIRES to measure the near-infrared spectra of these sources,” said Burgasser, “which allows us to measure the temperature and gases present in their atmospheres. Each spectrum is essentially a fingerprint that allows us to distinguish a cool brown dwarf from other kinds of stars.”
To help find our sun’s coldest, nearest neighbors, the astronomers of the Backyard Worlds project turned to a worldwide network of more than 100,000 citizen scientists. These volunteers diligently inspect trillions of pixels of telescope images to identify the subtle movements of nearby brown dwarfs and planets. Despite the advances of machine learning and supercomputers, there’s still no substitute for the human eye when it comes to finding faint, moving objects.
Backyard Worlds volunteers have already discovered more than 1,500 stars and brown dwarfs near the sun—this new discovery represents about 100 of the coldest in that sample. According to Meisner, this is a record for any citizen science astronomy program, and 20 of the citizen scientists are listed as co-authors of the study. A handful of these cool worlds—which are among the coldest brown dwarfs known—approximate the temperature of Earth, based on measurements made by the recently decommissioned Spitzer Space Telescope.
“This paper is evidence that the solar neighborhood is still uncharted territory, and citizen scientists are excellent astronomical cartographers,” said Jacqueline Faherty, a senior research scientist at the American Museum of Natural History and coauthor on the study. “Mapping the coldest brown dwarfs down to the lowest mass gives us key insights into the bottom of the star formation process and provides a target list for detailed atmosphere studies of Jupiter analogs.”
The availability of decades of astronomical catalogs through the NOIRLab helped make the discoveries possible.
“The technical burden of downloading billion-object astronomical catalogs is typically insurmountable for individual investigators—including most professional astronomers,” Meisner said. “Thankfully, the Astro Data Lab’s open and accessible web portal allowed Backyard Worlds citizen scientists to easily query massive catalogs for brown dwarf candidates.”
He added that Astro Data Lab also enables convenient matching between data sets from NOIRLab telescopes and external facilities, such as NASA’s WISE satellite, that jointly contributed to these brown dwarf discoveries. Archival observations from telescopes at Cerro Tololo Inter-American Observatory and Kitt Peak National Observatory were also key to the discovery.
The approach of the Backyard Worlds project—searching for rare objects in large data sets—is also one of the goals for the upcoming Vera C. Rubin Observatory. Currently under construction on Cerro Pachón in Chile’s Atacama Desert, the Rubin Observatory will image the visible sky from the southern hemisphere of sky every three nights over 10 years, providing a vast amount of data which will enable new ways of doing astrophysical research.
“Vast modern data sets can unlock landmark discoveries, and it’s exciting that these could be spotted first by a citizen scientist,” said Meisner. “These Backyard Worlds discoveries show that members of the public can play an important role in reshaping our scientific understanding of our solar neighborhood.”
In addition to the 20 citizen scientists named as coauthors on the paper, the full collaboration included research teams from: NSF’s NOIRLab; the Department of Astrophysics, American Museum of Natural History; IPAC, California Institute of Technology; School of Earth and Space Exploration, Arizona State University; Gigamon Applied Threat Research; Institute for Research on Exoplanets, Université de Montréal; NASA Goddard Space Flight Center; Center for Astrophysics and Space Science, University of California San Diego; Department of Physics and Astronomy, University of Leicester; ESA for AURA, Space Telescope Science Institute;
Department of Physics, City University of New York; Physics and Astronomy Department, Bucknell University; Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma; Backyard Worlds: Planet 9 Collaboration; IATE-OAC, Universidad Nacional de Córdoba-CONICET and Physics Department, University Of Central Florida.
This research was supported by funding from NASA through the Astrophysics Data Analysis Program and Hubble Fellowship Program.
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