Astronomers Release Spectacular
Survey of the Distant Universe
Survey of the Distant Universe
June 28, 2016, University of Nottingham
-- Astronomers at The University of Nottingham have released spectacular new
infrared images of the distant Universe, providing
the deepest view ever obtained over a large area of sky. The team, led by Omar Almaini, Professor of Astrophysics in the
School of Physics and Astronomy, is presenting
their results at the National Astronomy Meeting taking place this week at the
University’s Jubilee Campus.
The final data release from the Ultra-Deep
Survey (UDS) maps an area four times the size of the full Moon to
unprecedented depth. Over 250,000 galaxies have been detected, including
several hundred observed within the first billion years after the Big Bang.
Astronomers around the world will use the new images to study the early stages
of galaxy formation and evolution.
The release of the final UDS images represents the
culmination of a project that began taking data in 2005. The scientists used
the United Kingdom
Infrared Telescope (UKIRT) on Hawaii
to observe the same patch of sky repeatedly, building up more than 1000 hours
of exposure time. Observing in the infrared is vital for studying the distant
Universe, as ordinary starlight is "redshifted" to longer wavelengths
due to the cosmological expansion of the Universe.
Because of the finite speed of light, the most distant
galaxies are also observed very far back in time.
Professor Almaini said: "With the UDS we can
study distant galaxies in large numbers, and observe how they evolved at
different stages in the history of the Universe. We see most of the galaxies in
our image as they were billions of years before the Earth was formed.”
The UDS is the deepest of 5 projects, collectively
known as the UKIRT Infrared Deep Sky Survey (UKIDSS).
Earlier releases of data from the UDS have already
produced a wide range of scientific advances, including studies of the earliest
galaxies in the first billion years after the Big Bang, measurements of the
build-up of galaxies through cosmic time, and studies of the large-scale
distribution of galaxies to weigh the mysterious ‘dark matter’ that pervades
the cosmos. The added depth from the new release is expected to produce many
new breakthroughs.
Dr David Maltby, a postdoctoral research fellow at The
University of Nottingham whose research focusses on morphological evolution of
galaxies, said: "Here in Nottingham we
are aiming to understand how galaxies evolved to produce the rich diversity we
see today. For example, we still don't understand
why the most massive galaxies are usually elliptical in shape, while less
massive galaxies tend to be disk-shaped with spiral arms. By looking back in
time to the early Universe we can catch these galaxies in their infancy, and
observe them as they change and evolve over many billions of years."
Images are available.
Shown is an image of a small section (0.4%) of the UDS
field. Most of the objects in the image are very distant galaxies, observed as
they were over 9 billion years ago. In the full image, 250,000 galaxies have
been detected over an area of sky four times the size of the full Moon.
More images are available via this link.
Please credit: Professor Omar Almaini, The University of Nottingham.
UKIRT
The 3.8-metre United Kingdom Infrared Telescope
(UKIRT) is the world’s second largest telescope dedicated to infrared
astronomy. UKIRT is sited near the summit of Mauna Kea , Hawaii ,
at an altitude of 4194 metres (13760 feet) above sea level. The telescope was
owned and operated by the UK Science and Technology Facilities Council until
2014, when ownership transferred to the University of Hawaii .
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