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Distribution of Dark Matter – 3.5 Billion Years Ago

Distribution of Dark Matter - 3.5 Billion Years Ago

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    10h 0m 28.6s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    02° 12' 21.0"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Sextans

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 Hubble image was created from HST data from proposals: 9822 and 10092 – Principal Investigator: Scoville

    The Subaru image: Principal Investigator: Taniguchi

    The VLT image: Principal Investigator: Kneib

    The XMM/Newton image: Principal Investigator: Hasinger

  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Cosmological Evolution Survey Field, COSMOS Field
  • Object Description
    Object DescriptionThe type of astronomical object.
    Dark Matter Distribution Map, Astronomical Survey
  • Release Date
    January 7, 2007
  • Science Release
    Hubble Maps the Cosmic Web of “Clumpy” Dark Matter in 3-D
  • Credit
    NASA, ESA, and R. Massey (California Institute of Technology)

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Details

Last Updated
Mar 28, 2025
Contact
Media

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