Disk Detective

Last updated

Disk Detective
DiskDetectiveLogo black.png
DiskDetectiveFlipbook.gif
Type of site
 Citizen science project
Available inEnglish, Spanish, German, Polish, Chinese, Indonesian, Hungarian, Romanian, Russian, Portuguese
Created byDisk Detective Team
URL www.diskdetective.org
CommercialNo
RegistrationOptional
Launched31 January 2014;
10 years ago (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]

Contents

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 Peter Pan disk WISE J080822.18-644357.3.png
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:

Related Research Articles

<span class="mw-page-title-main">Brown dwarf</span> Type of substellar object larger than a planet

Brown dwarfs are substellar objects that have more mass than the biggest gas giant planets, but less than the least massive main-sequence stars. Their mass is approximately 13 to 80 times that of Jupiter (MJ)—not big enough to sustain nuclear fusion of ordinary hydrogen (1H) into helium in their cores, but massive enough to emit some light and heat from the fusion of deuterium (2H). The most massive ones can fuse lithium (7Li).

<span class="mw-page-title-main">Rogue planet</span> Planetary objects without a planetary system

A rogueplanet, also termed a free-floating planet (FFP) or an isolated planetary-mass object (iPMO), is an interstellar object of planetary mass which is not gravitationally bound to any star or brown dwarf.

<span class="mw-page-title-main">Subdwarf</span> Star of luminosity class VI under the Yerkes spectral classification system

A subdwarf, sometimes denoted by "sd", is a star with luminosity class VI under the Yerkes spectral classification system. They are defined as stars with luminosity 1.5 to 2 magnitudes lower than that of main-sequence stars of the same spectral type. On a Hertzsprung–Russell diagram subdwarfs appear to lie below the main sequence.

<span class="mw-page-title-main">NGC 2547</span> Open cluster in the constellation Vela

NGC 2547 is a southern open cluster in Vela, discovered by Nicolas Louis de Lacaille in 1751 from South Africa. The star cluster is young with an age of 20-30 million years.

<span class="mw-page-title-main">HR 4796</span> Binary star system in the constellation Centaurus

HR 4796 is a binary star system in the southern constellation of Centaurus. Parallax measurements put it at a distance of 235 light-years from the Earth. The two components of this system have an angular separation of 7.7 arcseconds, which, at their estimated distance, is equivalent to a projected separation of about 560 Astronomical Units (AU), or 560 times the separation of the Earth from the Sun. The star and its ring resemble an eye, and it is sometimes known by the nickname "Sauron's Eye".

WISE J0521+1025 is a nearby brown dwarf of spectral type T7.5, located in the constellation Orion at approximately 21.7 light-years from Earth.

<span class="mw-page-title-main">HD 115600</span> Star in the constellation Centaurus

HD 115600 is a star in the constellation Centaurus and a member of the Scorpius–Centaurus association, the nearest OB association to the Sun and the host star of a bright Kuiper belt-like debris ring.

2MASS J11193254–1137466 AB is a planetary mass binary located 86±23 light-years from the Earth in the constellation Crater. The components of 2MASS J1119–1137 are each roughly four Jupiter masses. The planetary-mass objects are probably a part of the TW Hydrae association which has an age of approximately 10 million years. The planetary-mass objects are candidate rogue planets.

<span class="mw-page-title-main">WISE J1147−2040</span>

WISEA J114724.10−204021.3 is a brown dwarf in the TW Hydrae association, a nearby group of very young stars and brown dwarfs. The object is notable because its estimate mass, 6±1 times the mass of Jupiter, places it in the mass range for rogue planets. Nevertheless, it is a free-floating object, unassociated with any star system.

HD 74389 is a double star system approximately 425 light years from Earth. The primary, HD 74389 A, was initially listed in the Hipparcos catalog as an A0V spectral type star, but this was subsequently updated in 1990 as A2V when Sanduleak and Pesch imaged it with the Burrell Schmidt telescope at Kitt Peak.

<span class="mw-page-title-main">WISE J080822.18-644357.3</span> Red dwarf star in the constellation Carina

WISE J080822.18-644357.3, also called J0808, is a 45+11
−7 Myr old star system in the Carina constellation with a circumstellar debris disk orbiting an M-type red dwarf about 331 lightyears from Earth.

<span class="mw-page-title-main">Backyard Worlds</span> NASA-funded citizen science project

Backyard Worlds: Planet 9 is a NASA-funded citizen science project which is part of the Zooniverse web portal. It aims to discover new brown dwarfs, faint objects that are less massive than stars, some of which might be among the nearest neighbors of the Solar System, and might conceivably detect the hypothesized Planet Nine. The project's principal investigator is Marc Kuchner, an astrophysicist at NASA's Goddard Space Flight Center.

<span class="mw-page-title-main">WISEA 1101+5400</span>

WISEA 1101+5400 is a T-type brown dwarf approximately 100 light-years away in the constellation Ursa Major. It was discovered in March 2017 by members of the citizen science project Backyard Worlds. Initial photometric analysis suggested it was a T5.5 dwarf, which was later confirmed by a spectrum of the object obtained with the NASA Infrared Telescope Facility. It is the first confirmed brown dwarf found by the project.

<span class="mw-page-title-main">LSPM J0207+3331</span> Star in the constellation Taurus

LSPM J0207+3331 is, as of 2023, the oldest and coldest known white dwarf star to host a circumstellar disk, located 145 light-years from Earth. It was discovered in October 2018 by a volunteer participating in the Backyard Worlds citizen science project.

A Peter Pan disk is a circumstellar disk around a star or brown dwarf that appears to have retained enough gas to form a gas giant planet for much longer than the typically assumed gas dispersal timescale of approximately 5 million years. Several examples of such disks have been observed to orbit stars with spectral types of M or later. The presence of gas around these disks has generally been inferred from the total amount of radiation emitted from the disk at infrared wavelengths, and/or spectroscopic signatures of hydrogen accreting onto the star. To fit one specific definition of a Peter Pan disk, the source needs to have an infrared "color" of , an age of >20 Myr and spectroscopic evidence of accretion.

<span class="mw-page-title-main">Tucana-Horologium association</span> Large stellar association

The Tucana-Horologium association (Tuc-Hor), or Tucana Horologium moving group, is a stellar association with an age of 45 ± 4 Myr and it is one of the largest stellar associations within 100 parsecs. The association has a similar size to the Beta Pictoris moving group (BPMG) and contains, like BPMG, more than 12 stars with spectral type B, A and F. The association is named after two southern constellations, the constellation Tucana and the constellation Horologium.

<span class="mw-page-title-main">Planet Patrol (project)</span>

Planet Patrol is a NASA citizen science project available in Zooniverse and aimed at discovering new exoplanets with data from the TESS telescope.

<span class="mw-page-title-main">WISEA 1810−1010</span> Substellar object in Serpens constellation

WISEA J181006.18-101000.5 or WISEA 1810-1010 is a substellar object in the constellation Serpens about 8.9 parsec or 29 light-years distant from earth. It stands out because of its peculiar colors matching both L-type and T-type objects, likely due to its very low metallicity. Together with WISEA 0414−5854 it is the first discovered extreme subdwarf (esd) of spectral type T. Lodieu et al. describe WISEA 1810-1010 as a water vapor dwarf due to its atmosphere being dominated by hydrogen and water vapor.

<span class="mw-page-title-main">WISEA J120037.79-784508.3</span> Brown dwarf in the constellation Chamaleon


WISEA J120037.79-784508.3, also called W1200-7845 or 2MASS J12003792-7845082, is a brown dwarf with a primordial disk 333.73 ± 3.13 lightyears from Earth in the 3.7+4.6
−1.4 Myr-old ε Chamaeleontis association, currently making it the closest known brown dwarf with an associated circumstellar disk. It was discovered by citizen scientists in 2020 volunteering for the Disk Detective project.

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. Archived from the original on 16 March 2012. 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. 30 March 2018. 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.
This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.