The Universe "Down Under" is the Latest Target for Hubble's Latest Deep-View
Turning its penetrating vision toward southern skies, the Hubble telescope has peered down a 12- billion-light-year-long corridor loaded with a dazzling assortment of thousands of never-before-seen galaxies. The observation, called the Hubble Deep Field South, doubles the number of far-flung galaxies available to astronomers for deciphering the history of the universe.
This new far-look complements the original Hubble "deep field" taken in late 1995, when Hubble was aimed at a small patch of space near the Big Dipper. Hubble's sharp vision allows astronomers to sort galaxy shapes. The image is dominated by beautiful pinwheel-shaped disk galaxies, which are like our Milky Way.
Turning its penetrating vision toward southern skies, NASA's Hubble Space Telescope has peered down a 12 billion light-year long corridor loaded with a dazzling assortment of thousands of never-before seen galaxies. The observation called the Hubble Deep Field South (HDF-S) doubles the number of far-flung galaxies available to astronomers for deciphering the history of the universe.
This new far-look complements the original Hubble "deep field" taken in late 1995, when Hubble was aimed at a small patch of space near the Big Dipper. The new region is in the constellation Tucana, near the south celestial pole.
The 10-day-long observation was carried out in October 1998 by a team of astronomers at the Space Telescope Science Institute (STScI), Baltimore, MD, and NASA's Goddard Space Flight Center, Greenbelt, MD. It is being made available today to the worldwide astronomy community for further research, and to the general public interested in the most distant reaches of the cosmos.
"The southern field promises to be the most studied area of the sky over the next five years," says STScI astronomer Robert Williams, when as STScI Director, he used his discretionary time to undertake the first deep field campaign, and has overseen the latest observation.
"We have eagerly awaited this new set of images ever since the first HDF, which had a dramatic impact on the entire science of astronomy. Hubble's deep field views revealed a large, heretofore unseen fraction of the universe and opened it up to interpretation and understanding."
It will take months for astronomers to digest what new secrets of the universe are within this latest look. At first glance the HDF-S appears to validate the common assumption that the universe should look largely the same in any direction.
The two deep fields now give astronomers two "core samples" of the universe for better understanding the history of the cosmos. The pair of observations can be compared to more confidently infer the state of the cosmos as a whole. It would take astronomers 900,000 years to use Hubble to survey the entire sky to the depths of the HDF. So, they must rely on a thin "looking-through-soda straw" view across the cosmos and infer the history of star and galaxy formation.
The new deep field also provides an astronomical gold mine for powerful new ground-based telescopes located in the southern hemisphere to undertake follow-up observations of galaxies and precisely measure their distances.
All of Hubble's new cameras and other instruments were trained on the sky simultaneously for the observation. The Space Telescope Imaging Spectrograph was used to dissect light from a quasar (bright, active core of a distant galaxy) in its field of view. The light from the quasar has traveled nearly three-quarters of the way across the universe, and provides a powerful three-dimensional probe of the universe's hidden structure. Invisible clouds of primeval hydrogen gas strung along billions of light-years between us and the quasar will be detectable in the signature of the quasar's light. The quasar is so brilliant it is like a searchlight shining through haze.
The original HDF engaged hundreds of astronomers around the world. Broad conclusions were drawn based on meticulous follow-up studies of the myriad galaxies along Hubble's extremely narrow line-of-sight. To date, conclusions about the rate of star formation and evolution of galaxy shapes have been based on this one narrow "core-sample" of the universe. Because the original HDF was picked as a seeming bland example of what the universe at large probably looks like, astronomers have assumed it was a representative sample. But they needed a second sample to validate early assumptions, and they needed a field that contained a distant quasar to give them important additional information that the northern field did not contain.