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Hubble Gallery of Ultra-Bright Galaxies

Rose gold-colored galaxies against the black background of space in a grid of two by three.

Hubble Captures Gallery of Ultra-Bright Galaxies

These six images, taken by the Hubble Space Telescope, reveal a jumble of misshapen-looking galaxies punctuated by exotic patterns such as arcs, streaks, and smeared rings. These unusual features are the stretched shapes of the universe's brightest infrared galaxies that are boosted by natural cosmic magnifying lenses. Some of the oddball shapes in the images also may have been produced by spectacular collisions between distant, massive galaxies in a sort of cosmic demolition derby.

This so-called gravitational lensing occurs when the intense gravity of a massive galaxy or cluster of galaxies magnifies the light of fainter, more distant background sources. The "lenses" are foreground massive galaxies whose gravity magnifies and distorts images of the distant bright infrared galaxies behind them.

The faraway galaxies are as much as 10,000 times more luminous than our Milky Way. The lensing phenomenon allows for features as small as about 100 light-years or less across to be seen in the background galaxies.

The galaxies existed between 8 billion and 11.5 billion years ago, when the universe was making stars more vigorously than it is today. The galaxies are ablaze with runaway star formation, pumping out more than 10,000 new stars a year. The star-birth frenzy creates lots of dust, which enshrouds the galaxies, making them too faint to detect in visible light. But they glow fiercely in infrared light, shining with the brilliance of 10 trillion to 100 trillion suns.

The infrared galaxies in these images are part of a Hubble survey of 22 distant ultra-luminous infrared galaxies that were found by ground- and space-based observatories. The images were taken in infrared light by Hubble's Wide Field Camera 3. Color has been added to highlight details in the galaxies.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    J074851.72: 07h 48m 52.20s; J084648.55: 08h 46m 49.35s; J114329.52: 11h 43m 29.53s; J231356.64: 23h 13m 54.483s; J132217.52: 13h 22m 17.53s; J022633.98: 02h 26m 33.95s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    J074851.72: +59° 42' 01.31"; J084648.55: +15° 05' 52.1"; J114329.52: +68° 01' 06.41"; J231356.64: +01° 06' 08.76"; J132217.52: +09° 23' 26.20"; J022633.98: +23° 45' 28.36"

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.

    These data are from the HST proposal 14653 PI: J. Lowenthal (Smith College).

  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>WFC3/IR
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    J074851.72: Oct. 19, 2016; J084648.55: Feb. 19, 2017; J114329.52: Oct. 13, 2016; J231356.64: Oct. 22, 2016; J132217.52: Feb. 3, 2017; J022633.98: Nov. 26, 2016. Exposure Dates: 30 observations between Oct. 13, 2016, and Mar. 11, 2017
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F160W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    J074851.72J084648.55J114329.52J231356.64J132217.52J022633.98
  • Object Description
    Object DescriptionThe type of astronomical object.
    Galaxy Cluster
  • Release Date
    June 6, 2017
  • Science Release
    Jackpot! Cosmic Magnifying-Glass Effect Captures Universe’s Brightest Galaxies
  • Credits
    NASA, ESA, and J. Lowenthal (Smith College)

Downloads

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    tif (9.12 MB)
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  • Full Res, 3190 × 2128
    png (7.92 MB)
Rose gold-colored galaxies against the black background of space in a grid of two by three.
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

This image is a composite of separate exposures acquired by the WFC3/IR instrument on the Hubble Space Telescope. One filter was used for each frame of the composite. The color results from assigning different hues (colors) to each monochromatic (grayscale) image. In this case, the assigned color is yellow 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 12, 2025
Contact
Media

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