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Adam Crain holds a motor from SOAR telescope’s spectrograph
control
system for which he wrote software.

Carolina professors Wayne Christiansen and Bruce Carney.

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Sky's the Limit
SOAR, a new telescope like no other, exists because of work by Carolina
scientists and students who collaborated with scientists worldwide.
SOAR, the Southern Observatory for Astrophysical Research, is a state-of-the-art,
lightweight, computer-controlled, 4-meter telescope that sits atop Cerro
Pachon, a 9,000-foot mountain in Chile's northern Andes. Four partners
fund ed the $32-million research facility: UNC-Chapel Hill, Michigan State
University, the U.S. National Optical Astronomy Observatory (NOAO) and
the Ministry of Science of Brazil.
With a formal dedication on April 17, 2004 SOAR joined the
world's exclusive fraternity of cutting-edge research telescopes
studying the Southern Skies.
Students and faculty in Carolina's
Department of Physics and Astronomy will not only be among the first to use SOAR,
but also will carr y on a long tradition of astronomical
research at Carolina. In 1824, UNC President Joseph Caldwell
brought the university's first telescope from England. Seven
years later, Caldwell oversaw construction of the first astronomical
observatory at a U.S. university. SOAR will collect 3,400
times more light than that original telescope.
“SOAR will detect objects well over a billion times fainter
than the eye can see, and about 20 million times fainter
than did that first telescope,” department chair and Samuel
Baron Professor Bruce Carney said. “So we can see dimmer
objects and stars out to vastly greater distances, and, hence,
further back in time.”
SOAR's networked computer system will allow researchers
to study the skies above Chile from Chapel Hill. Because
the university is guaranteed time on SOAR, researchers will
create a list of projects and astronomical conditions ( e.g.
dark of the moon) needed to see them. When the right conditions
happen, Chapel Hill astronomers will be notified to log onto
computers in Chapel Hill to direct the observations and download
data in real time.
“We'll get our first cut at science right away and if things
aren't going as expected, you can switch filters or make
other changes on the fly,” professor Wayne Christiansen said. “Once
you've finished, you can get your data over the Internet
or by airmail for further analysis. For the most part, we
won't need to go to Chile.”
SOAR is not just your average telescope. Recent advances
in equipment design and computer technology mean SOAR will
allow astronomers to study and learn in ways only dreamed
possible a few years ago , Christiansen said.
For starters, SOAR's location is ideal. Based in the foothills
of the 20,000-foot Andes mountain range, SOAR sits far away
from smog, lights and other visual distractions of city life.
The flowing offshore winds and lack of annual rainfall are
just right for optimal viewing, Christiansen said. “The seeing
is superb,” he said. “In Chile, the center of the Milky Way
galaxy passes right over your head. You can observe it for
a much longer period of time, and your images aren't distorted
as much by atmospheric effects.”
Chile is among the best sites in the Southern Hemisphere
for viewing the Milky Way, our home galaxy encompassing Earth
and the other planets in our solar system. In addition, the
Magellanic Clouds [our closest neighboring galaxies], are
in the Chilean skies .
Besides offering an unfettered view of the universe, SOAR
is a technological marvel compared with conventional telescopes,
Christiansen said. SOAR delivers the highest quality images
possible with a large, ground-based telescope.
A major advance will be SOAR's “quick change” instruments.
Currently, 4-meter telescopes — such as NOAO's Blanco telescope
on the neighboring Chilean mountain, Cerro Tololo — use equipment
weighing tons. Depending on what type of equipment an astronomer
needs to view the universe, such as infrared or visual cameras
or spectrographs, it can take a day or more to change settings
and tools.
That scenario won't happen with SOAR. Thanks to improved
design, lightweight equipment and computerized remote controls,
SOAR can “quick change,” allowing researchers to respond
immediately to astronomical phenomena when they happen.
“With SOAR, the minute something like a supernova comes
up, we'll be all over it,” Christiansen said. “We'll be able
to react to unexpected events when they happen.”
Adam Crain, a 2003 Carolina graduate from Hickory, N.C.,
developed software to drive SOAR's remote astronomy. “I spent
three months in La Serena, Chile working with the SOAR team.
I wrote software, participated in design meetings and learned
about software control of instrumentation in general.”
Crain's first software piece was for the Goodman Spectrograph
control system, an imaging spectrograph built at UNC. “The
control system coordinates the motions of eleven motors and
two actuators,” Crain said. “The system's distinguishing
features include its multithreaded architecture, remote capability,
automated configuration changes and observing deck control
via a PDA. Astronomers around the world will use the
system to perform measurements without traveling to Chile.”
To handle large data files containing images and spectral
datasets from SOAR instruments, Crain created a remote observing
tool. The tool consists of two pieces of software, a server
and a client that facilitate the data transfer. Astronomers
can compress data and view glossy representations within
seconds of acquisition. The full datasets transfer
in parallel, arriving minutes later. The toll automatically
displays the images and overlays celestial coordinates on
the images, allowing astronomers to make intelligent adjustments
to the telescope position.
Prior to SOAR, department faculty and students have primarily
used national facilities for observations. These include
the National Optical Astronomy
Observatory, the National
Radio Astronomy Observatory, the Hubble
Space Telescope, the Chandra
X-ray Observatory, and other facilities including the
Australia Telescope, the Anglo-Australia Telescope, and the
Keck Observatory. Teaching and research facilities include
a 24-inch remote-controlled telescope at the Morehead
Observatory on campus, and two small robotic telescopes
out in the mountains at the Pisgah
Astronomical Research Institute .
For more information:
SOAR site webcam
http://www.physics.unc.edu/research/astro/soar_cams.php
SOAR telescope website
http://www.soartelescope.org/
SOAR interior webcam
http://www.ctio.noao.edu/soar/netcam.html |