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HDUV GOODS-North Field

HDUV GOODS-North Field

Astronomers using the ultraviolet vision of NASA’s Hubble Space Telescope have captured one of the largest panoramic views of the fire and fury of star birth in the distant universe. The field features approximately 15,000 galaxies, about 12,000 of which are forming stars. Hubble’s ultraviolet vision opens a new window on the evolving universe, tracking the birth of stars over the last 11 billion years back to the cosmos’ busiest star-forming period, which happened about 3 billion years after the big bang.

Ultraviolet light has been the missing piece to the cosmic puzzle. Now, combined with infrared and visible light data from Hubble and other space and ground-based telescopes, astronomers have assembled one of the most comprehensive portraits yet of the universe’s evolutionary history.

The image straddles the gap between the very distant galaxies, which can only be viewed in infrared light, and closer galaxies, which can be seen across a broad spectrum. The light from distant star-forming regions in remote galaxies started out as ultraviolet. However, the expansion of the universe has shifted the light into infrared wavelengths. By comparing images of star formation in the distant and nearby universe, astronomers glean a better understanding of how nearby galaxies grew from small clumps of hot, young stars long ago.

Because Earth’s atmosphere filters most ultraviolet light, Hubble can provide some of the most sensitive space-based ultraviolet observations possible.

The program, called the Hubble Deep UV (HDUV) Legacy Survey, extends and builds on the previous Hubble multi-wavelength data in the CANDELS-Deep (Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey) fields within the central part of the GOODS (The Great Observatories Origins Deep Survey) fields. This mosaic is 14 times the area of the Hubble Ultraviolet Ultra Deep Field released in 2014.

This image is a portion of the GOODS-North field, which is located in the northern constellation Ursa Major.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    12:36:54.56
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    +62:14:42.092
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Ursa Major

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 HST observations include those from programs 12444, 12445 (S. Faber), and 13872 (P. Oesch)
  • Instrument
    InstrumentThe science instrument used to produce the data.
    ACS/WFC, WFC3/UVIS, WFC3/IR
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    Sep 2012 - Aug 2013, and Nov 2014 - Nov 2015
  • Filters
    FiltersThe camera filters that were used in the science observations.
    WFC3/UVIS F275W, F336W, ACS/WFC F435W, F606W, F775W, F850LP, WFC3/IR F125W, F160W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    HDUV GOODS North
  • Object Description
    Object DescriptionThe type of astronomical object.
    Deep field image
  • Release Date
    August 16, 2018
  • Science Release
    Hubble Paints Picture of the Evolving Universe
  • Credit
    NASA, ESA, P. Oesch (University of Geneva), and M. Montes (University of New South Wales)

Downloads

  • Full Res, 7190 × 6356
    tif (101.46 MB)
  • 1000 × 884
    png (1.36 MB)
  • Full Res, 7190 × 6356
    png (82.14 MB)
  • 2000 × 1768
    png (5.78 MB)
HDUV GOODS-North Field
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

These images are a composite of separate exposures acquired by the ACS and WFC3 instruments on the Hubble Space Telescope. Several filters were used to sample narrow wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Blue: F275W, F336W, F435W, F606W Green: F775W, F850LP Red: F125W, F160W

Compass and Scale
Compass and ScaleAn astronomical image with a scale that shows how large an object is on the sky, a compass that shows how the object is oriented on the sky, and the filters with which the image was made.

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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