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Wide Field 30 Doradus UVIS

Wide Field 30 Doradus UVIS

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    05h 38m 42.4s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -69° 6' 3.35"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Dorado
  • Distance
    DistanceThe physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
    Approximately 170,000 light-years (52,000 parsecs)

About the Data

  • Data Description
    Data DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
    Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
    The ACS/WFC3 data are from the following HST proposals: 12499: D. Lennon (ESA), E. Sabbi (ESA/STScI), J. Anderson, R. van der Marel, T. Sohn, and N. Walborn (STScI), L. Bedin (INAF, Padua), C. Evans (Royal Observatory Edinburgh), H. Sana (STScI/ESA), N. Langer (University of Bonn), S. de Mink (Carnegie Institution of Washington), P. Crowther (University of Sheffield), A. Herrero (IAC, Tenerife), N. Bastian (USM, Munich), and E. Bressert (Australia Telescope National Facility); 12939: E. Sabbi (ESA/STScI), A. Aloisi, J. Anderson, K. Gordon, A. Koekemoer, R. van der Marel, N. Panagia, and C. Christian (STScI), M. Boyer (NASA/GSFC), C. Evans (Royal Observatory Edinburgh), J. Gallagher (University of Wisconsin, Madison), E. Grebel (Astronomisches Rechen-Institut Heidelberg), S. de Mink (Carnegie Institution of Washington), S. Larsen (Radboud Universiteit Nijmegen), D. Lennon (ESA), M. Tosi (INAF, Osservatorio Astronomico di Bologna), and D. Zaritsky (University of Arizona)
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>WFC3/UVIS
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F275W, F336W, F775W (i)
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    30 Doradus
  • Object Description
    Object DescriptionThe type of astronomical object.
    Emission Nebula in the Large Magellanic Cloud
  • Release Date
    January 9, 2014
  • Science Release
    Electronic Book for Students with Visual Impairments Reaches for the Stars
  • Credit
    NASA, ESA, and E. Sabbi (STScI)

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Details

Last Updated
Feb 17, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov