Hubble Ultra Deep Field

Hubble Ultra Deep Field

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Fast Facts
News release ID: STScI-2014-27
Release Date: Jun 3, 2014
Image Use: Copyright
About this image

This tiny slice of the universe, speckled with galaxies near and far, tells the story of galaxy evolution over cosmic time. Among the 10,000 or so galaxies pictured here are newborns, adolescents, adults, and retirees. Like looking through a vast collection of family photos, astronomers are poring over this comprehensive image to see how galaxies grew up, matured, and aged.

This portrait of our universe's history is called the Hubble Ultra Deep Field (or HUDF). It is a minuscule patch of sky first targeted by the Hubble Space Telescope in 2002 and revisited over and over again since then. This version of the HUDF is extra special, though. It combines observations of the field taken with Hubble's Advanced Camera for Surveys and the Wide Field Camera 3 from 2002 to 2012, providing one of the farthest views into the universe we've ever seen. Plus, it includes light not just from the visible part of the spectrum but from the (invisible) infrared and ultraviolet ranges, too, giving us different details of the story of how galaxies came to be.

Infrared light lets us see the universe's youngest galaxies. These galaxies lie far, far away from us, and as their light travels across the universe, it gets stretched by the expansion of space. Wavelengths of visible light grow longer, becoming infrared light by the time it reaches us. Combining Hubble's observations of the HUDF in visible and infrared light, a team of astronomers led by Garth Illingworth of the University of California identified more than 5,500 galaxies in a central portion of the field, some so faint that they are just one ten-billionth the brightness of what the human eye can see. Another team, headed by Richard Ellis of the California Institute of Technology (Caltech), used Hubble's infrared observations to find galaxies more than 13 billion light-years away, when the universe was only about 400 million years old — or about three percent of its present age.

Alternatively, to understand slightly older, growing galaxies that are not so far away, observing in ultraviolet light is best. The hottest and youngest stars give off huge amounts of ultraviolet light, making them easy to spot at those wavelengths of light. Most recently, a team of astronomers led by Harry Teplitz of Caltech used the ultraviolet-sensing abilities of Hubble's Wide Field Camera 3 to add the ultraviolet piece to this view of the HUDF. With this part of the galaxy evolution picture in hand, astronomers are investigating how galaxies grew through bursts of star formation and exactly where, when, and how many stars formed over time.

Because our atmosphere blocks or absorbs most infrared and ultraviolet light that reaches Earth, only a telescope in space, like Hubble, can provide such insights into the history of galaxies. Without both infrared and ultraviolet light, the tale is incomplete.

Constellation: Fornax

Distance: 13.2 billion light-years

Instrument: Advanced Camera for Surveys/WFC and /SBC, and Wide Field Camera 3/IR and /UVIS

Image Filters: ACS/SBC: F150LP;
WFC3/UVIS: F225W (U), F275W (U), F336W (U);
ACS/WFC: F435W (B), F606W (V), F775W (I), F814W (I), F850LP (z);
WFC3/IR: F105W (Y), F125W (J), F140W (JH), F160W (H)

Cosmology, Deep Fields, Distant Galaxies, Hubble Ultra Deep Field, Observations, Survey


2004 HUDF Credit: NASA, ESA, S. Beckwith, M. Stiavelli, A. Koekemoer (STScI), R. Thompson (University of Arizona), and the STScI HUDF Team;

2009 HUDF Credit: NASA, ESA, G. Illingworth, R. Bouwens (University of California, Santa Cruz), and the HUDF09 Team;

2012 HUDF Credit: NASA, ESA, R. Ellis (Caltech), R. McLure, J. Dunlop (University of Edinburgh), B. Robertson (University of Arizona), A. Koekemoer (STScI), and the HUDF12 Team;

2012 XDF Credit: NASA, ESA, G. Illingworth, D. Magee, P. Oesch (University of California, Santa Cruz), R. Bouwens (Leiden University), and the HUDF09 Team;

2014 HUDF / UV-UDF Credit: NASA, ESA, H. Teplitz, M. Rafelski (IPAC/Caltech), A. Koekemoer (STScI), R. Windhorst (Arizona State University), and Z. Levay (STScI)