Hubble Deep Fields

What Are the Hubble Deep Fields?

Telescopes are time machines. When we look out at space, we are looking back in time. The light arriving at our location from the farthest objects in the universe is light that left those objects billions of years ago. We see those objects not as they are today, but as they appeared long ago.

For 10 straight days in 1995, Hubble stared at a tiny and nearly empty patch of sky near the Big Dipper. The telescope gathered all the light it could, slowly building a picture.  What emerged — the Hubble Deep Field — revealed galaxies fainter than had ever been seen before. The light from some of these has traveled for 10 billion years to reach us.

It showed us a sliver of the early universe, from long before our sun was born. This is really a three-dimensional picture, a cosmic core sample. The results are a treasure trove: 3,000 galaxies, large and small, shapely and amorphous, burning in the depths of space. There are a few foreground stars, many remote galaxies and more galaxies in between. The galaxies vary in shape, size and color.  We can see how they changed through time. With the Hubble Deep Field, we reach back nearly to the time when galaxies emerged from the chaos of the big bang. 

In subsequent years, Hubble teamed with other observatories to examine small patches of the sky in high resolution with long exposures and multiple wavelengths. Surveys like the Hubble Ultra Deep Field (HUDF), and the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDLES) have provided pictures of vast, deep collections of galaxies — including some that existed when the universe was less than a billion years old.

In 2014, astronomers released the most colorful and comprehensive picture of the evolving universe ever captured by Hubble. The observation, called the Ultraviolet Coverage of the Hubble Ultra Deep Field, provides the missing link in star formation. Astronomers previously studied the Hubble Ultra Deep Field (HUDF) in visible and near-infrared light in a series of images captured from 2003 to 2009.

Now, using ultraviolet light, astronomers combined the full range of colors available to Hubble, stretching all the way from ultraviolet to near-infrared light. Ultraviolet light comes from the hottest, largest and youngest stars. By observing at these wavelengths, researchers get a direct look at which galaxies are forming stars and where the stars are forming within those galaxies. Studying the ultraviolet images of galaxies in this intermediate time period enables astronomers to understand how galaxies grew in size by forming small collections of very hot stars. Because Earth’s atmosphere filters most ultraviolet light, this work can only be accomplished with a space-based telescope.

The resulting image — made from 841 orbits of telescope viewing time — contains approximately 10,000 galaxies, extending back in time to within a few hundred million years of the big bang. Hubble can see even farther back in time by using gravitational lensing to find more distant galaxies that formed even earlier in the universe, such as in the CLASH survey and Frontier Fields. With its powerful infrared vision, the James Webb Space Telescope will see even farther back in time.

Last Updated: June 02, 2019