Disk Detective
Type of site
Citizen science project
Available inEnglish, Spanish, German, Polish, Chinese, Indonesian, Hungarian, Romanian, Russian, Portuguese
Created byDisk Detective Team
URLwww.diskdetective.org
CommercialNo
RegistrationOptional
Launched31 January 2014 (2014-01-31)
Current statusOnline

Disk Detective is the first NASA-led and funded-collaboration project with Zooniverse.[1] It is NASA's largest crowdsourcing citizen science project[2] aiming at engaging the general public in search of stars, which are surrounded by dust-rich circumstellar disks, where planets usually dwell and are formed.[3][4] Initially launched by NASA Citizen Science Officer, Marc Kuchner, the principal investigation of the project was turned over to Steven Silverberg.[5]

Details

Disk Detective was launched in January 2014, and was expected to continue until 2017.[6] In April 2019 Disk Detective uploaded partly classified subjects, as Zooniverse did stop to support the old platform for projects,[7] which was completed in May 2019.[8] The project team began working on Disk Detective 2.0[9] that was then launched May 24, 2020, utilizing Zooniverse's new platform.[10]

The project invites the public to search through images captured by NASA's Wide-field Infrared Survey Explorer (WISE)[11] and other sky surveys. Disk Detective 1.0 compared images from the WISE mission to the Two Micron All Sky Survey (2MASS), the Digitized Sky Survey (DSS) and the Sloan Digital Sky Survey (SDSS). Version 2.0 compares WISE images to 2MASS, Panoramic Survey Telescope and Rapid Response System (Pan-STARRS), Australia's SkyMapper telescope, and the unblurred coadds of WISE imaging (unWISE).

The images in Disk Detective have all been pre-selected to be extra bright at wavelengths where circumstellar dust emits thermal radiation. They are at mid-infrared, near-infrared and optical wavelengths. Disks are not the only heavenly objects that appear bright at infrared wavelengths; active galactic nuclei, galaxies, asteroids and interstellar dust clouds also emit at these wavelengths. Computer algorithms cannot distinguish the difference, so it is necessary to examine all images by "eye" to make sure that the selected candidates are stars with disks, and not other celestial objects.

After the initial and subsequent discovery of several Peter Pan disks—M dwarf primordial gas-rich circumstellar disk systems that retain their gas 2 to 10 times longer than that of other disks—by the Disk Detective science team, research began to understand how these unusual systems fit into disk development. On September 29, 2022, NASA announced version 2.1 of the project, releasing new data containing thousands of images of nearby stars located in young star-forming regions and to provide a better view of "extreme" debris disks—circumstellar disks that have brighter than expected luminosity—in the galactic plane. The 2.1 dataset targets stars with brightness at a wavelength of 12 μm in an effort to discover more Peter Pan disks.[12]

Classification

At the Disk Detective website, the images are presented in animated forms which are called flip books. Each image of the flip book is formatted to focus on the subject of interest within a series of circles and crosshairs.[13]

Website visitors—whether or not they are registered member users of Zooniverse—examine the flip book images and classify the target subjects based on simple criteria. Disk Detective 2.0 elimination criteria include whether the subject "moves" off the center crosshairs in 2MASS images only, if it moves off of crosshairs in two or more images, if the subject is not round in Pan-STARRS, SkyMapper, or 2MASS images, if it becomes extended beyond the outer circle in WISE images, and if two or more images show objects between the inner and outer circles. The ideal target is classified as a "good candidate," and is further vetted by the advanced research group into a list of "debris disk of interest" (DDOI) candidates. Particular interest is paid to good candidates that have two or more images where objects other than the subject are present within the inner circle only.[13]

The selected disk candidates will eventually become the future targets for NASA's Hubble Space Telescope and its successor, the James Webb Space Telescope. They will also be the topic for future publications in scientific literature.

Seeking objects

The disks that NASA's scientists at the Goddard Space Flight Center aim to find are debris disks, which are older than 5 million years; and young stellar object (YSO) disks, which are younger than 5 million years.

Advanced user group

Volunteers who have registered as citizen scientists with Zooniverse can join an exclusive group on the Disk Detective project, called "advanced users" or "super users," after they have done 300 classifications. Advanced users might then further vet candidates marked as "good," compare candidate subjects with literature, or analyze follow-up data.[14][15] This advanced user group is similar to other groups that have formed in citizen science projects, such as the Peas Corps in Galaxy Zoo.[16]

Discoveries

WISE J080822.18-644357.3, a ~45 Myr-old pre-transitional disk discovered by volunteers of Disk Detective

The Disk Detective project discovered the first example of a Peter Pan disk. At the 235th meeting of the American Astronomical Society the discovery of four new Peter Pan disks was presented. Three objects are high-probability members of the Columba and Carina stellar associations. The forth object has an intermediate likelihood of being part of a moving group. All four objects are young M dwarfs.[17][18]

The project has also discovered the first debris disk with a white dwarf companion (HD 74389)[19] and a new kind of M dwarf disk (WISE J080822.18-644357.3) in a moving group.[20] The project found 37 new disks (including HD 74389) and four Be stars in the first paper[19] and 213 newly-identified disk candidates in the third paper.[15] Together with WISE J080822.18-644357.3, the Disk Detective project found 251 new disks or disk candidates. The third paper also found HD 150972 (WISEA J164540.79-310226.6) as a likely member of the Scorpius–Centaurus moving group, 12 candidates that are co-moving binaries and 31 that are closer than 125 parsec, making them possible targets for direct imaging of exoplanets.[15]

Additionally, the project published the discovery a nearby young brown dwarf with a warm class-II type circumstellar disk, WISEA J120037.79−784508.3 (W1200−7845), located in the ε Chamaeleontis association. Found 102 parsecs (~333 lightyears) from the Sun, this puts it within the solar neighborhood, making it ideal for study since brown dwarfs are very faint due to their low masses of about 13-80 MJ. Therefore, it is within distance to observe greater details if viewed with large telescope arrays or space telescopes. W1200-7845 is also very young, with measurements putting it at about 3.7 million years old, meaning that—along with its relatively close proximity—it could serve as a benchmark for future studies of brown dwarf system formation.[21]

False positive rate and applications

The project did make estimates about the amount of high-quality disk candidates in AllWISE and lower-limit false-positive rates for several catalogs, based on classification false-positive rates, follow-up imaging and literature review. Out of the 149,273 subjects on the Disk Detective website 7.9±0.2% are likely candidates. 90.2% of the subjects are eliminated by website evaluation, 1.35% were eliminated by literature review and 0.52% were eliminated by high-resolution follow-up imaging (Robo-AO + Dupont/Retrocam). From this result AllWISE might contain ~21,600 high quality disk candidates and 4-8% of the disk candidates from high-quality surveys might show background objects in high-resolution images, which are bright enough to affect the infrared excess.[15]

The project also has a database that is available through the Mikulski Archive for Space Telescopes (MAST). It contains the "goodFraction", describing how often a source was voted as a good source on the website, as well as other information about the source, such as comments from the science team, machine learned classification, cross-matched catalog information and SED fits.[22]

A group at MIT did use the Disk Detective classifications to train a machine-learning system. They found that their machine-learning system agreed with user identifications of debris disks 97% of the time. The group has found 367 promising candidates for follow-up observations with this method.[23][24]

See also

Zooniverse projects:

References

  1. ↑ "Zooniverse".
  2. ↑ http://www.jpl.nasa.gov/news/news.php?release=2014-032 NASA-Sponsored 'Disk Detective' Lets Public Search for New Planetary Nurseries
  3. ↑ Launching Disk Detective: A New Citizen Science Website › Marketing For Scientists
  4. ↑ Sinai Nick and Smith Gayle (6 December 2013). "Second Open Government National Action Plan". whitehouse.gov. Retrieved 6 December 2013 – via National Archives.
  5. ↑ Disk Detective: Team
  6. ↑ "Disk Detective". NASA. Retrieved 3 September 2014.
  7. ↑ @diskdetective (20 April 2019). "There are only 10 days left to finish Disk Detective 1.0 before we shut down and we need your help now!Come to http://DiskDetective.org and help us classify the rest of the partly classified sources before April 30! Please retweet!! #citizenscience" (Tweet). Retrieved 15 November 2019 – via Twitter.
  8. ↑ @diskdetective (30 April 2019). "We are at 100%. Now a new chapter begins" (Tweet). Retrieved 15 November 2019 – via Twitter.
  9. ↑ "Disk Detective: Archive". diskdetective.org. Retrieved 15 November 2019.
  10. ↑ Silverberg, Steven (14 July 2020). "Welcome to Disk Detective v2.0!". Retrieved 14 October 2022.
  11. ↑ "NASA Releases New WISE Mission Catalog of Entire Infrared Sky". NASA. Retrieved 14 March 2012.
  12. ↑ "Disk Detective 2.1 is Live! Come Join the Search!". NASA. Retrieved 16 October 2020.
  13. 1 2 "Disk Detective: Classify".
  14. ↑ marckuchner2014 (4 December 2018). "Our Third Paper: The Advanced Users' Story". Disk Detective. Retrieved 15 November 2019.{{cite web}}: CS1 maint: numeric names: authors list (link)
  15. 1 2 3 4 Silverberg, Steven M.; Kuchner, Marc J.; Wisniewski, John P.; Bans, Alissa S.; Debes, John H.; Kenyon, Scott J.; Baranec, Christoph; Riddle, Reed; Law, Nicholas; Teske, Johanna K.; Burns-Kaurin, Emily (November 2018). "Follow-up Imaging of Disk Candidates from the Disk Detective Citizen Science Project: New Discoveries and False Positives in WISE Circumstellar Disk Surveys". The Astrophysical Journal. 868 (1): 43. arXiv:1809.09663. Bibcode:2018ApJ...868...43S. doi:10.3847/1538-4357/aae3e3. ISSN 0004-637X. S2CID 119026404.
  16. ↑ Cardamone, Carolin; Schawinski, Kevin; Sarzi, Marc; Bamford, Steven P.; Bennert, Nicola; Urry, C. M.; Lintott, Chris; Keel, William C.; Parejko, John; Nichol, Robert C.; Thomas, Daniel (1 November 2009). "Galaxy Zoo Green Peas: discovery of a class of compact extremely star-forming galaxies". Monthly Notices of the Royal Astronomical Society. 399 (3): 1191–1205. arXiv:0907.4155. Bibcode:2009MNRAS.399.1191C. doi:10.1111/j.1365-2966.2009.15383.x. ISSN 0035-8711. S2CID 14663963.
  17. ↑ Silverberg, S.; Wisniewski, J.; Kuchner, M.; Collaboration, Disk Detective (January 2020). "Four New Peter Pan Disk Candidates from Disk Detective". AAS. 52: 161.05. Bibcode:2020AAS...23516105S.
  18. ↑ Silverberg, Steven M.; Wisniewski, John P.; Kuchner, Marc J.; Lawson, Kellen D.; Bans, Alissa S.; Debes, John H.; Biggs, Joseph R.; Bosch, Milton K. D.; Doll, Katharina; Luca, Hugo A. Durantini; Enachioaie, Alexandru (14 January 2020). "Peter Pan Disks: Long-lived Accretion Disks Around Young M Stars". The Astrophysical Journal. 890 (2): 106. arXiv:2001.05030. Bibcode:2020ApJ...890..106S. doi:10.3847/1538-4357/ab68e6. S2CID 210718358.
  19. 1 2 Kuchner, Marc J.; Silverberg, Steven M.; Bans, Alissa S.; Bhattacharjee, Shambo; Kenyon, Scott J.; Debes, John H.; Currie, Thayne; Garcia, Luciano; Jung, Dawoon; Lintott, Chris; McElwain, Michael; Padgett, Deborah L.; Rebull, Luisa M.; Wisniewski, John P.; Nesvold, Erika; Schawinski, Kevin; Thaller, Michelle L.; Grady, Carol A.; Biggs, Joseph; Bosch, Milton; Cernohous, Tadeás; Luca, Hugo A. Durantini; Hyogo, Michiharu; Wah, Lily Lau Wan; Piipuu, Art; Piñeiro, Fernanda (19 July 2016). "Disk Detective: Discovery of New Circumstellar Disk Candidates through Citizen Science". The Astrophysical Journal. 830 (2): 84. arXiv:1607.05713. Bibcode:2016ApJ...830...84K. doi:10.3847/0004-637X/830/2/84. S2CID 28650844.
  20. ↑ Silverberg, Steven M.; Kuchner, Marc J.; Wisniewski, John P.; Gagne, Jonathan; Bans, Alissa S.; Bhattacharjee, Shambo; Currie, Thayne R.; Debes, John R.; Biggs, Joseph R.; Bosch, Milton; Doll, Katharina; Durantini-Luca, Hugo A.; Enachioaie, Alexandru; Griffith, Sr; Hyogo, Michiharu; Piñeiro, Fernanda; Collaboration, Disk Detective (14 October 2016). "A New M Dwarf Debris Disk Candidate in a Young Moving Group Discovered with Disk Detective". The Astrophysical Journal. 830 (2): L28. arXiv:1610.05293. Bibcode:2016ApJ...830L..28S. doi:10.3847/2041-8205/830/2/L28. S2CID 119183849.
  21. ↑ Schutte, Maria C.; Lawson, Kellen D.; Wizniewski, John P.; Kuchner, Marc J.; Silverberg, Steven M.; Faherty, Jacqueline K.; Gagliuffi, Daniella C. Bardalez; Kimon, Rocio; Gagné, Jonathan; Meisner, Aaron; Schneider, Adam C.; Bans, Alissa S.; Debes, John H.; Kovacevic, Natalie; Bosch, Milton K. D.; Luca, Hugo A. Durantini; Holden, Jonathan D.; Hyogo, Michiharu (3 August 2020). "Discovery of a Nearby Young Brown Dwarf Disk". The Astronomical Journal. 160 (4): 10. arXiv:2007.15735v2. Bibcode:2020AJ....160..156S. doi:10.3847/1538-3881/abaccd. S2CID 220920317.
  22. ↑ silverbergastro (9 September 2019). "The Disk Detective Database". Disk Detective. Retrieved 15 November 2019.
  23. ↑ "Computer searches telescope data for evidence of distant planets". MIT News. Retrieved 15 November 2019.
  24. ↑ Nguyen, T.; Pankratius, V.; Eckman, L.; Seager, S. (April 2018). "Computer-aided discovery of debris disk candidates: A case study using the Wide-Field Infrared Survey Explorer (WISE) catalog". Astronomy and Computing. 23: 72–82. Bibcode:2018A&C....23...72N. doi:10.1016/j.ascom.2018.02.004. ISSN 2213-1337.
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