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PSZ1 G311.65-18.48

PSZ1 G311.65-18.48

This NASA Hubble Space Telescope photo reveals a cosmic kaleidoscope of a remote galaxy, which has been split into multiple images by an effect called gravitational lensing.

Gravitational lensing means that the foreground galaxy cluster is so massive that its gravity distorts the fabric of space-time, bending and magnifying the light from the more distant galaxy behind it. This “funhouse mirror” effect not only stretches the background galaxy image, but also creates multiple images of the same galaxy.

The lensing phenomenon produces at least 12 images of the background galaxy, distributed over four major arcs. Three of these arcs are visible in the top right of the image, while one counter arc is visible in the lower left — partially obscured by a bright foreground star within the Milky Way.

The galaxy, nicknamed the Sunburst Arc, is almost 11 billion light-years from Earth and has been lensed into multiple images by a massive foreground cluster of galaxies 4.6 billion light-years away.

Hubble uses these cosmic magnifying glasses to study objects that would otherwise be too faint and too small for even its extraordinarily sensitive instruments. The Sunburst Arc is no exception, despite being one of the brightest gravitationally lensed galaxies known.

The lens makes images of the Sunburst Arc that are between 10 and 30 times brighter than the background galaxy would normally look. The magnification allows Hubble to view structures as small as 520 light-years across that would be too small to see without the turboboost from the lensing effect. The structures resemble star forming regions in nearby galaxies in the local universe, allowing astronomers to make a detailed study of the remote galaxy and its environment.

Hubble’s observations show that the Sunburst Arc is similar to galaxies which existed at a much earlier time in the history of the universe, perhaps only 150 million years after the Big Bang.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    15:50:06.82
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -78:11:30.76
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Apus
  • 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.
    4.6 billion light-years
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    Image is 2.64 arcmin across (about 3.5 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 HST observations include those from programs 15377 (M. Bayliss), 15418 (M. Bayliss), and 15101 (H. Dahle)
  • Instrument
    InstrumentThe science instrument used to produce the data.
    WFC3/UVIS; WFC3/IR; ACS/WFC
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    Feb 2018 to April 2019
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F275W, F606W, F814W, F160W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    PSZ1 G311.65-18.48
  • Object Description
    Object DescriptionThe type of astronomical object.
    Lensed Galaxy in Galaxy Cluster
  • Release Date
    November 7, 2019
  • Science Release
    Hubble Captures a Dozen Galaxy Doppelgangers
  • Credit
    NASA, ESA, and E. Rivera-Thorsen (Institute of Theoretical Astrophysics Oslo, Norway)

Downloads

  • 2000 × 1785
    png (5.36 MB)
  • Full Res, 5290 × 4722
    png (37.12 MB)
  • Full Res, 5290 × 4722
    tif (37.68 MB)
PSZ1 G311.65-18.48
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 WFC3/UVIS, WFC3/IR, and ACS/WFC 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 Cyan: F606W Yellow: F814W Red: 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