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N.C. astronomy institute aims to archive a treasure trove of celestial photos 

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However forward-thinking the field of astronomy, professional and amateur stargazers are always looking into the past. The light emanating from distant celestial bodies has traveled millions of light-years before we see it. Some stars may have already died—supernovas exploding in a last gasp before ejecting their mass into space. We may not know their fate for another million years.

"The idea is to understand objects," explains Wayne Osborn, an adjunct professor at Yerkes Observatory at the University of Chicago in Williams Bay, Wis. "Very few people take the time to go back and look at these photos. But there is a lot of data that can be mined and put in a modern context."

For example, in 1904 American astronomer Edward Barnard discovered a nova, a star later named Ross 4, which had exploded. In subsequent photos, Ross 4 dimmed as it aged. But in 1948, Ross 4 exploded a second time. And just last year, it exploded again. Without the photographic record, the recent conflagration would lack context.

What does it mean? "It means that's not a typical nova," Osborn says. It's likely part of a double system in which the collapsed white dwarf—in this case, Ross 4—siphons fuel from its companion star. The hydrogen accumulates on the surface of the white dwarf, igniting a nuclear outburst.

The physical object takes on even greater importance when you consider the data includes not only the contents of the photographs but the photographs themselves. Historians can use astronomers' observation notes to piece together biographies. Scientists can gather pollen from the plates to determine what plants may have been in season when the photo was taken—information that can aid botanists. And since these images were shot through the earth's atmosphere, the photographic spectra—bands of light that contain information about the chemical composition and other properties of the subject—can tell meteorologists and climatologists about the nature of the ozone layer.

At PARI, Barker says he doesn't usually clean the plates unless he has a detailed scan of them "because there are often marks on the non-emulsion side where the observer made a mark. That's valuable in the provenance of the plate and I want to get a scan of that."

"They're irreproducible. For older astronomers it's sacrilege [to throw them out]," says Osborn, who is among a handful of astronomers devoted to salvaging the photos. "It was the gold standard that you kept your photographs. It's like saying, 'No one's using books anymore. They're all online, so let's get rid of libraries.'"

These plates can also correct the scientific record. Predecessors occasionally introduced errors into star catalogs, sometimes merely clerical, other times gross miscalculations.

"There are a lot of ways to go wrong in science," says Brian Skiff, a research assistant at the Lowell Observatory in Flagstaff, Ariz. He consulted PARI's cache of photos for a research paper on stars. After receiving a scan of the plate, Skiff determined that the original astronomer had misclassified the type of star, based on its colors. "The star is broadcasting information about itself," he says. Skiff then could correct the error in the star catalog, a bible of sorts, for astronomers.

"It's arcane," Skiff says. "Preserving the raw data is very important. They're not lost in the mist of time."

On a recent afternoon, Mike Brown, professor of planetary astronomy at the California Institute of Technology, descended from the 14,000-foot summit of Mauna Kea in Hawaii. There, at the Keck Observatory, he was using a powerful telescope to photograph a part of the sky in search of moons orbiting objects in the Kuiper Belt, a region beyond Neptune populated by icy chunks of material, including water, ammonia and methane.

He says that in the early 2000s, many astronomers acted as if they were amateur shutterbugs, mindlessly deleting pictures as if they were bad shots of a birthday party. "No one thought about it," Brown says. "We've lost a part of a generation to the world."

Brown stored many of his digital photos on disc drives. "They're dead," says Brown, author of the book How I Killed Pluto and Why It Had It Coming. "I should have been archiving them—but that's boring, so I didn't do it."

Digital archiving and preservation presents challenges archivists continue to grapple with. "It takes only one accidental click to get rid of a file," says Stephen Fletcher, photographic archivist for the North Carolina Collection at UNC libraries. A physical photograph or negative, while fragile, can last for at least 100 years if properly stored, as have many of PARI's plates.

"But with a digital file," Fletcher says, "there's machine obsolescence, bit rot or malfunctioning equipment. You can't store a digital file and presume it will be sitting on the same shelf for 50 years."

Earlier in the digital age, film had the advantage because it could photograph wide expanses of the sky; however, it wasn't sensitive enough to pick up faint objects. While sophisticated digital cameras used in astronomy can photograph less luminescent bodies, because of the enormous file sizes they only recently became useful for analyzing large areas of the firmament.

PARI's digital collection is so valuable that EMC Corporation, based in Research Triangle Park, donated hundreds of sophisticated hard drives for servers with multiple layers of redundancy. There hasn't been a disc failure at PARI, even though just one high-resolution scan—and there are 140,000 of these scans to be made—can approach a file size of 1 gigabyte.

"We're going to need storage space," Fletcher says of digital archiving. "We're dealing with servers and secure systems. As a profession, we're trying to adapt our tenets of provenance and respect for the original to the digital world."

Archiving and digitizing 140,000 glass-plate photos is time-consuming and expensive. At PARI, Barker and several volunteers painstakingly pick away at the collection. There are virtually no federal grants, including through NASA or the National Science Foundation, available for the project, in part because it is viewed as mundane.

"We are known as an innovation agency at the forefront of the outermost frontiers of knowledge," says NSF spokesperson Lisa Van Pay. This year the NSF, which funds research in non-medical science fields, is expected to greatly reduce the number of astronomy and astrophysics grants, according to space.com.

That money generally is awarded to major projects—the construction of huge telescopes or research into sexy topics like the "co-evolution of supermassive black holes" or "observations of near-earth asteroids."

At the NSF, proposals are peer-reviewed, but Skiff says few astronomers "recognize the value" of these plates. "It's producing new knowledge, but it's more intangible."

Digitizing these photographs allows not only for efficient computer analysis but also for sharing online with professional and amateur astronomers and the public.

Through PARI's SCOPE website, the public can contribute to the body of knowledge by examining digital images of stars and classifying them.

PARI's herculean task of collecting, preserving and digitizing the plates serves science and stokes our curiosity and sense of wonder. When we gaze at the night sky, we cannot help but note our relative insignificance and marvel at the celestial mechanics that drive the farthest reaches of the universe.

"When people come to the [Yerkes] observatory, they're taken by the immensity of it, but also the spirituality of it," Osborn says.

Sometimes that immensity and spirituality can be captured on one small plate, a snapshot of discovery. Brown still has the plate on which astronomer Charles Kowal shot "Object X" in 1977. Kowal, who died last year, had discovered a celestial object, a minor planet, between Jupiter and Neptune. It was named Chiron.

However, the image is not a screensaver on his computer, Brown says. "It's next to my desk so I can look at it."

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