Suggested Searches

1 min read

Abell 370 Parallel

Thousands of galaxies appear all across the view.

This is a Hubble Space Telescope view of a random patch of sky that reveals how the universe looks at large: a "wallpaper" of innumerable galaxies spread across space and time. They offer a wide assortment of majestic star cities that vary in age, shape, and stellar populations. It’s a narrow view down a corridor that stretches back in time for billions of years.

The wide range of rich colors comes from the fact that this snapshot is assembled from images taken in visible light as well as near-infrared light. The reddest objects in the image are presumably the farthest galaxies, whose light has been stretched into the red part of the spectrum by the expansion of space. The yellow objects are massive football-shaped elliptical galaxies that contain older stellar populations. The blue galaxies are disk-shaped pinwheels of ongoing star formation. The entire field is peppered with much smaller, fragmentary, blue galaxies – the "building blocks" ancestors of majestic spiral galaxies like our Milky Way.

This so-called "parallel field" was taken while Hubble was looking at the primary target, a massive foreground galaxy cluster, while another camera simultaneously viewed the adjacent, seemingly sparse patch of sky.

Such parallel fields increase the efficiency of Hubble for deep sky surveys, and yield new insights into the evolution of galaxies over billions of 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.
    Abell 370 is part of the Frontier Fields Program. These data are from the HST proposals 11108 (PI: E. Hu, University of Hawaii), 11507 (PI: K. Noll, GSFC), 11591 (PI: J.-P. Kneib, Laboratoire d'Astrophysique de Marseille), 13459 (PI: T. Treu, UCLA), 13790 (PI: S. Rodney, JHU), 14038 (PI: J. Lotz, STScI), and 14216 (R. Kirshner, Harvard University). For more information, see http://www.stsci.edu/hst/campaigns/frontier-fields.
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>ACS/WFC and HST>WFC3/IR
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    September 2009 - February 2015
  • Filters
    FiltersThe camera filters that were used in the science observations.
    ACS/WFC: F435W, F606W, and F814W; WFC3/IR: F105W, F125W, F140W, and F160W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Abell 370 Parallel
  • Release Date
    May 4, 2017
  • Science Release
    A Lot of Galaxies Need Guarding in This NASA Hubble View
  • Credit
    NASA, ESA, and J. Lotz and the HFF Team (STScI)

Downloads

  • Full Res, 4147 × 4638
    tif (37.6 MB)
  • 400 × 400
    png (321.83 KB)
  • 1788 × 2000
    png (6.25 MB)
  • Full Res, 4147 × 4638
    png (31.38 MB)
Thousands of galaxies appear all across the view.
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

Blue: F435W + F606W Green: F814W + F105W Red: F125W + F140W + 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.

Share

Details

Last Updated
Mar 28, 2025
Contact
Media

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