The Hubble Deep Field Images
One of the main scientific justifications for building Hubble was to measure the size and age of the Universe and test theories about its origin. Images of faint galaxies give ‘fossil’ clues as to how the Universe looked in the remote past and how it may have evolved with time. The Deep Fields gave astronomers the first really clear look back to the time when galaxies were forming. The first deep fields – Hubble Deep Field North and South – gave astronomers a peephole to the ancient Universe for the first time, and caused a real revolution in modern astronomy.
Subsequent deep imagery from Hubble, including the Hubble Ultra Deep Field, has revealed the most distant galaxies ever observed. Because of the time it has taken their light to reach us, we see some of these galaxies as they were less than a billion years after the Big Bang.
Deep field observations are long-lasting observations of a particular region of the sky intended to reveal faint objects by collecting the light from them for an appropriately long time. The ‘deeper’ the observation is (i.e. longer exposure time), the fainter are the objects that become visible on the images. Astronomical objects can either look faint because their natural brightness is low, or because of their distance. In the case of the Hubble Deep and Ultra Deep Fields, it is the extreme distances involved which make them faint, and hence make observations challenging. In addition, these distant objects appear so tiny on the sky that Hubble’s precise vision is required to resolve them.
Using the different Hubble Deep Fields astronomers were able to study young galaxies in the early Universe and the most distant primeval galaxies. The different Deep Fields are also good gathering grounds to find the most distant objects ever observed.
10 days in the making
The idea for the Hubble Deep Fields originated in results from the first deep images taken after the repair in 1993. These images showed many galaxies, which were often quite unlike those we see in the local Universe and could not otherwise be studied using conventional ground-based telescopes. The first Deep Field, the Hubble Deep Field North (HDF-N), was observed over 10 consecutive days during Christmas 1995. The resulting image consisted of 342 separate exposures, with a total exposure time of more than 100 hours, compared with typical Hubble exposures of a few hours. The observed region of sky in Ursa Major was carefully selected to be as empty as possible so that Hubble would look far beyond the stars of our own Milky Way and out past nearby galaxies.
The results were astonishing! Almost 3,000 galaxies were seen in the image. Scientists analysed the image statistically and found that the HDF had seen back to the very young Universe where the bulk of the galaxies had not, as yet, had time to form stars. Or, as the popular press dramatically reported, “Hubble sees back to Big Bang”. These very remote galaxies also seemed to be smaller and more irregular than those nearer to us. This was taken as a clear indication that galaxies form by gravitational coalescence of smaller parts.
In 1996 it was decided to observe a second Deep Field, the Hubble Deep Field South (HDF-S), to assess whether the HDF-N was indeed a typical area and thus representative of the Universe as a whole. This time the field also contained a quasar, which was used as a cosmological lighthouse and provided valuable information about the matter between the quasar and the Earth.
After the Hubble observations of HDF-N and -S, other ground and space-based instruments targeted the same patches of sky for long periods. Some of the most interesting results seem to emerge from these fruitful synergies between instruments of different sizes, in different environments and with sensitivity to different wavelengths.
The Hubble Ultra Deep Field
The Hubble Ultra Deep Field from 2004 represents the deepest portrait of the visible universe ever achieved by humankind. Using the improved capabilities of the Advanced Camera for Surveys, the camera installed during the 2002 servicing mission, a new Deep Field was observed, in the constellation of Fornax (the Furnace). It reveals some of the first galaxies to emerge from the “dark ages”, the time shortly after the Big Bang when the first stars reheated the cold, dim universe.
Because the Universe expands, light waves from very distant objects are stretched during their long journey to us. The further away objects are from us, the more their light is stretched. As longer wavelengths appear redder than shorter wavelengths, this phenomenon is known as “redshift”, and it is somewhat similar to the Doppler effect heard when an ambulance siren drops in pitch as the vehicle speeds away.
For very distant objects, their light is shifted so far that they drop out of the visible spectrum altogether, and can only be seen in infrared light. This means that the Hubble Ultra Deep Field cannot be improved on by building a more sensitive optical telescope — Hubble has reached the limit of what is possible in visible light.
The Hubble Ultra Deep Field — Infrared
The only way to see further than the Hubble Ultra Deep Field is to look beyond the optical wavelengths and observe in infrared instead.
Using NICMOS, its first near infrared camera, Hubble made infrared observations of the original Hubble Deep Field, the Hubble Deep Field South and Hubble Ultra Deep Field. These images revealed more distant objects, though the picture quality achieved by this instrument could not compete with optical images.
The next breakthrough came after the 2009 servicing mission in which astronauts installed a new instrument capable of making greatly improved infrared observations. The resulting image, covering most of the field of view of the 2004 Ultra Deep Field observations, is the deepest ever made of the cosmos. It is unlikely to be surpassed until the NASA/ESA/CSA James Webb Space Telescope is operational, later this decade.
The 2009 infrared image of the Hubble Ultra Deep Field has been an extremely fertile hunting ground for scientists who study the early Universe. Several candidates for the most distant galaxy ever observed have been spotted in this image.
The Hubble eXtreme Deep Field — and more
Published in 2012, the Hubble eXtreme Deep Field is a combination of many existing exposures (over 2,000 of them) into one image. Combining the Hubble Ultra Deep Field, the Hubble Ultra Deep Field – Infrared, and many other images of the same small spot of sky taken over almost 10 years, the Hubble eXtreme Deep Field pushes the limit even further. It is made up of a total of 22 days of exposure time (and 50 days of observing time, as the telescope can only observe the deep field for around half of every orbit.)
The last Hubble Ultra Deep Field released in 2014 was observed in ultraviolet. This image allowed astronomers to study star formation in a region 5 to 10 billion light-years away from us. The study is called the Ultraviolet Coverage of the Hubble Ultra Deep Field (UVUDF) project. The addition of ultraviolet data to the Hubble Ultra Deep Field using Hubble’s Wide Field Camera 3 gives astronomers access to direct observations of regions of unobscured star formation and may help to understand how rapidly stars formed over cosmic time.
Credit: The Hubble Deep Fields
Flight Through the Hubble eXtreme Deep Field
This video begins with a zoom into the small area of sky that the Hubble Space Telescope observed to construct the eXtreme Deep Field, or XDF. The region is located in the southern sky, far away from the glare of the Milky Way, the bright plane of our galaxy. In terms of angular size, the field is a fraction of the angular diameter of the full Moon, yet it contains thousands of galaxies stretching back across time.
The video then depicts a flight through the galaxies in the XDF. Using measured and estimated redshifts for approximately three thousand galaxies, astronomers and visualizers constructed a three-dimensional model of the XDF galaxy distribution. The camera starts from Hubble’s viewpoint, traverses more than thirteen billion light-years of space, and exits the data set past a “red dot” galaxy (or proto-galaxy) with a redshift of 7.82. For cinematic reasons, the exceedingly vast distances in the 3D model have been greatly compressed.