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Gravitationally Lensed REQUIEM Galaxies

Four-panel image of gravitationally lensed REQUIEM survey galaxies in lensing galaxy clusters MACS J1341 and MACS J2129

These images are composites from NASA's Hubble Space Telescope and the Atacama Large Millimeter/submillimeter Array (ALMA). The boxed and pullout images show two of the six, distant, massive galaxies where scientists found star formation has ceased due to the depletion of a fuel source—cold hydrogen gas.

Hubble, together with ALMA, found these odd galaxies when they combined forces with the "natural lens" in space created by foreground massive galaxy clusters. The clusters' gravity stretches and amplifies the light of the background galaxies in an effect called gravitational lensing. This phenomenon allows astronomers to use massive galaxy clusters as natural magnifying glasses to study details in the distant galaxies that would otherwise be impossible to see.

The yellow traces the glow of starlight. The artificial purple color traces cold dust from ALMA observations. This cold dust is used as a proxy for the cold hydrogen gas needed for star formation.

Even with ALMA's sensitivity, scientists do not detect dust in most of the six galaxies sampled. One example is MRG-M1341, at upper right. It looks distorted by the "funhouse mirror" optical effects of lensing. In contrast, the purple blob to the left of the galaxy is an example of a dust-and-gas-rich galaxy.

One example of the detection of cold dust ALMA did make is galaxy MRG-M2129 at bottom right. The galaxy only has dust and gas in the very center. This suggests that star formation may have shut down from the outskirts inward.

About the Object

  • 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.
    M1341 z=1.5943 (9.63 billion light-years); M2129 z=2.1478 (10.63 billion light-years)

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 images were created from HST data from proposals 12100 (M. Postman) and 15663 (M.Akhshik)

  • Instrument
    InstrumentThe science instrument used to produce the data.
    WFC3/UVIS and WFC3/IR
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    May - Aug 2011 and Feb - Mar 2020
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F814W, F125W, F160W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    MACS J1341 and MACS J2129
  • Object Description
    Object DescriptionThe type of astronomical object.
    Lensing galaxy clusters
  • Release Date
    September 22, 2021
  • Science Release
    Hubble Finds Early, Massive Galaxies Running on Empty
  • Credit
    NASA, ESA, Katherine Whitaker (UMass); Image Processing: Joseph DePasquale (STScI)

Downloads

  • Full Res, 3408 × 3425
    tif (20.47 MB)
  • Full Res, 3408 × 3425
    png (15.54 MB)
  • 1990 × 2000
    png (5.64 MB)
  • 995 × 1000
    png (1.52 MB)
  • Unannotated Full Res, 3408 × 3425
    tif (20.63 MB)
  • Unannotated Full Res, 3408 × 3425
    png (15.41 MB)
  • Unannotated, 1990 × 2000
    png (5.59 MB)
  • Unannotated, 995 × 1000
    png (1.51 MB)
  • MACS J1341, 1750 × 1750
    tif (7.59 MB)
  • MACS J1341, 1750 × 1750
    png (5.43 MB)
  • MACS J2129, 1995 × 1995
    tif (8.57 MB)
  • MACS J2129, 1995 × 1995
    png (6.27 MB)
Four-panel image of gravitationally lensed REQUIEM survey galaxies in lensing galaxy clusters MACS J1341 and MACS J2129
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 obtained by the WFC3 instrument 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: F814WGreen: F125WRed: 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