The Whole Earth Telescope (WET), a worldwide network of observatories coordinated by the University of Delaware, is synchronizing its lenses to provide round-the-clock coverage of a cooling star. As the star dims in the twilight of its life, scientists hope it will shed light on the workings of our own planet and other mysteries of the galaxy.

The dying star, a white dwarf identified as WDJ1524-0030, located in the constellation Ophiuchus in the southern sky, is losing its brightness as it cools, its nuclear fuel spent. It will be monitored continuously from May 15 to June 11 by WET, a global partnership of telescopes which was formed in 1986.

Like an international relay team, observers at Mt. Cuba Observatory in Greenville, Del., will focus on and photograph the white dwarf until sunrise, and then observers at McDonald Observatory in Fort Davis, Texas, and at Kitt Peak National Observatory in Tucson, Ariz., will stand watch while the star is in their sky, followed by observers in New Zealand, Australia, China, and so on, around the globe.

The thousands of photographs of the white dwarf taken by WET will be e-mailed to the command center at Mt. Cuba Observatory staffed by University of Delaware researchers, for archiving and eventual analysis using the fledgling science of "star quakes" known as asteroseismology.

"A white dwarf is the size of the Earth and as dense as the sun. This star pulsates or quakes as waves of energy travel through it - its outer surface sloshes from side to side, like waves on the ocean," says Judi Provencial, assistant professor of physics and astronomy at UD and director of the Delaware Asteroseismic Research Center (DARC).

"What is of interest to scientists is the shape of the pulses," Provencal notes. "From them, we can measure how the atmosphere is moving around in these pulsating stars and figure out what's going on inside them. This one is really sloshing around."

There are thousands of white dwarfs in our galaxy; however, only about 30 percent are bright enough for scientists to study using asteroseismics, which can determine the age, temperature and composition of a star from its oscillations and brightness.

Provencal says that WDJ1524-0030 is one of only about 20 percent of the stars in the universe whose atmosphere is composed of helium versus hydrogen. The WET team hopes to find out the composition of the star's core, whether hydrogen or oxygen.

The process of discovery will take on the order of two years to stitch together all of the images, analyze the data, interpret the data with the input of the WET community and report the results. Eventually, the findings will be applied to other stars, including the sun, and to our own planet, Provencal says.

"We don't understand the weather on Earth, the transport of energy," she says. "We don't understand convection at all. Hopefully, this field of research, which is still very new, will help every aspect of astronomy."

Putting the Observing Run into Focus

Organizing all of the telescopes for an observing run may seem akin to aligning the planets. More than 20 telescopes are participating in the current run. Provencal and Susan Thompson, co-director of DARC, needed to submit applications for some of the major telescopes several years in advance.

Only one in five proposals typically gets selected by such competitive research facilities as the William Herschel Telescope in the Canary Islands. With a lens that is 4.2 meters in diameter, the telescope is the largest that has signed on to participate, Provencal says.

Before the advent of the Internet, Provencal says she and her colleagues at the command center used to have to call each observatory on the telephone to participate.

"In South Africa, we had to call the international operator, who could only get out to the telescope by a hand-cranked phone and you could hear that in the background. The Internet has taken some of the fun out of that, but France still likes to be called every day of the observing run," Provencal says.

"And at Peak-Turskol in Russia, the astronomers say they have several cats that like to participate."

Provencal says that she and her colleagues in the WET community like to study cooling stars "because it's cool."

While the administration of the Whole Earth Telescope is supported by the Crystal Trust Foundation, the observers are not paid to observe.

"Without them, it wouldn't happen," she says. "It's a community effort."

Participating telescopes
These observatories are participating in the Whole Earth Telescope's international observing run, which UD is coordinating, to monitor the white dwarf WDJ1524-0030. Telescope lens diameter is in parentheses:

+ Beijing Astronomical Observatory (BAO), China (2.1 m/6.9 ft)

+ Bohyunsan Optical Astronomy Observatory (BOAO), South Korea (1.8 m/5.9 ft)

+ Cerro Tololo Inter-American Observatory (CTIO), Chile (0.9 m/3 ft)

+ Institut fur Astronomie und Astrophysik Tubingen, Germany (0.8 m/2.6 ft)

+ Kitt Peak National Observatory, Arizona, USA (2.1 m/6.9 ft)

+ Las Cumbres Observatory, California, USA

+ Lulin Observatory, Taiwan (1 m/3.2 ft)

+ McDonald Observatory, Texas, USA (2.1 m/6.9 ft)

+ Moletai Astronomical Observatory, Lithuania (1.5 m/4.9 ft)

+ Mt. Abu Observatory, India (1.2 m/3.9 ft)

+ Mt. Cuba Astronomical Observatory, Delaware, USA (0.6 m/2 ft)

+ Mt. John Observatory of the University of Canterbury, New Zealand (1 m/3.2 ft)

+ Mt. Suhora Astronomical Observatory, Cracow Pedagogical University, Poland (0.6 m/2 ft)

+ Observatoire de Haute-Provence (OHP), France (1.93 m/6.3 ft)

+ Observatrio del Teide, Tenerife, Canary Islands, Spain (0.6 m/2 ft)

+ Osservatorio Astronomico di Bologna, Italy (1.5 m/4.9 ft)

+ Peak Terskol Observatory, Russian Federation (2 m/6.6 ft)

+ South African Astronomical Observatory (SAAO), South Africa (1 m/3.2 ft)

+ Southern Astrophysical Research Telescope (SOAR), Chile (4.2 m/13.8 ft)

+ Paul and Jane Meyer Observatory, Texas, USA (0.6 m/2 ft)

+ Southeastern Association for Research in Astronomy Observatory (SARA), Florida, USA (1 m/3.2 ft)

+ Vienna Observatory, Austria (0.68m/2.2 ft)