Vatican’s Celestial Eye, Seeking Not Angels but Data
An image of a spiral galaxy 102 million light-years from Earth taken by the Vatican Advanced Technology Telescope in Arizona.
Vatican’s Celestial Eye, Seeking Not Angels but Data
Published: June 22, 2009
MOUNT GRAHAM, Ariz. — Fauré’s “Requiem” is playing in the background, followed by the Kronos Quartet. Every so often the music is interrupted by an electromechanical arpeggio — like a jazz riff on a clarinet — as the motors guiding the telescope spin up and down. A night of galaxy gazing is about to begin at the Vatican’s observatory on Mount Graham.
“Got it. O.K., it’s happy,” says Christopher J. Corbally, the Jesuit priest who is vice director of the Vatican Observatory Research Group, as he sits in the control room making adjustments. The idea is not to watch for omens or angels but to do workmanlike astronomy that fights the perception that science and Catholicism necessarily conflict.
Last year, in an opening address at a conference in Rome, called “Science 400 Years After Galileo Galilei,” Cardinal Tarcisio Bertone, the secretary of state of the Vatican, praised the church’s old antagonist as “a man of faith who saw nature as a book written by God.” In May, as part of the International Year of Astronomy, a Jesuit cultural center in Florence conducted “a historical, philosophical and theological re-examination” of the Galileo affair. But in the effort to rehabilitate the church’s image, nothing speaks louder than a paper by a Vatican astronomer in, say, The Astrophysical Journal or The Monthly Notices of the Royal Astronomical Society.
On a clear spring night in Arizona, the focus is not on theology but on the long list of mundane tasks that bring a telescope to life. As it tracks the sky, the massive instrument glides on a ring of pressurized oil. Pumps must be activated, gauges checked, computers rebooted. The telescope’s electronic sensor, similar to the one in a digital camera, must be cooled with liquid nitrogen to keep the megapixels from fuzzing with quantum noise.
As Dr. Corbally rushes from station to station flicking switches and turning dials, he seems less like a priest or even an astronomer than a maintenance engineer. Finally when everything is ready, starlight scooped up by the six-foot mirror is chopped into electronic bits, which are reconstituted as light on his video screen.
“Much of observing these days is watching monitors and playing with computers,” Dr. Corbally says. “People say, ‘Oh, that must be so beautiful being out there looking at the sky.’ I tell them it’s great if you like watching TV.”
Dressed in blue jeans and a work shirt, he is not a man who wears his religion on his sleeve. No grace is offered before a quick casserole dinner in the observatory kitchen. In fact, the only sign that the Vatican Advanced Technology Telescope is fundamentally different from the others on Mount Graham, the home of an international astronomical complex operated by the University of Arizona, is a dedication plaque outside the door.
“This new tower for studying the stars has been erected on this peaceful site,” it says in Latin. “May whoever searches here night and day the far reaches of space use it joyfully with the help of God.” At that point, religion leaves off and science begins.
The Roman Catholic Church’s interest in the stars began with purely practical concerns when in the 16th century Pope Gregory XIII called on astronomy to correct for the fact that the Julian calendar had fallen out of sync with the sky. In 1789, the Vatican opened an observatory in the Tower of the Winds, which it later relocated to a hill behind St. Peter’s Dome. In the 1930s, church astronomers moved to Castel Gandolfo, the pope’s summer residence. As Rome’s illumination, the electrical kind, spread to the countryside, the church began looking for a mountaintop in a dark corner of Arizona.
Building on Mount Graham was a struggle. Apaches said the observatory was an affront to the mountain spirits. Environmentalists said it was a menace to a subspecies of red squirrel. There were protests and threats of sabotage. It wasn’t until 1995, three years after the edict of Inquisition was lifted against Galileo, that the Vatican’s new telescope made its first scientific observations.
The target tonight is three spiral galaxies — Nos. 3165, 3166, 3169 in the New General Catalog — lying about 60 million light-years from Earth, a little south of the constellation Leo. Sitting at a desk near Dr. Corbally is Aileen O’Donoghue, an astronomer from St. Lawrence University in Canton, N.Y., who is interested in how these gravitational masses tug at one another, creating the stellar equivalent of tides.
“Exposing, 30 minutes,” she says. As Celtic ballads play in the control room, data is sucked up by hard drives, and a column of numbers scrolls down her computer screen. Dr. O’Donoghue, who was raised Roman Catholic, is the author of “The Sky Is Not a Ceiling: An Astronomer’s Faith,” in which she describes how she lost and then rediscovered God “in the vastness, the weirdness, the abundance, the seeming nonsensicalness, and even the violence of this incredible universe.”
In person she’s not nearly so intense. While waiting for an image to gel, she steps out on a balcony for a look at the unprocessed sky. The Beehive Cluster, one of the first things Galileo saw with his telescope, is sparkling in the constellation Cancer. Next to it is Leo, where Dr. O’Donoghue is looking for the gravitational tides.
“It’s the real sky that matters,” she says. She describes how she makes her undergraduate students go outside and look at the Big Dipper at different times of the night. “They come back and say, ‘It moves!’ ” — words Galileo legendarily muttered after he was forced to recant. “You can tell students that the Earth rotates, but until they see that with their eyeballs, they’re not doing science,” she said. “You might as well be teaching theology and Scripture.”
Back inside the control room she explains how the gravitational tides she is studying might be stellar nurseries. As one galaxy brushes by another, clouds of gas are stirred so violently that they give birth to stars.
In the Vatican Observatory’s annual report, at the point where a corporation might describe its business strategy, is a section delineating the difference between creatio ex nihilo (creation from nothing) and creatio continua: “the fact that at every instant, the continued existence of the universe itself is deliberately willed by God, who in this way is continually causing the universe to remain created.”
Theologians call these “primary causes,” those that flow from the unmoved mover. Sitting atop this eternal platform is another layer, the “secondary causes,” which can be safely left to science.
Dr. Corbally and Dr. O’Donoghue continue working through the night, collecting data on secondary causes — galactic tides, stellar birth. Sleep will wait until morning, and thoughts about primary causes for another time.
Correction: June 25, 2009
A picture on Tuesday with an article about the
http://www.nytimes.com/2009/06/23/science/23Vatican.html?_r=1&ref=science
Salt Finding
June 24, 2009
RELEASE : 09-147
PASADENA, Calif. -- For the first time, scientists working on NASA's Cassini mission have detected sodium salts in ice grains of Saturn's outermost ring. Detecting salty ice indicates that Saturn's moon Enceladus, which primarily replenishes the ring with material from discharging jets, could harbor a reservoir of liquid water -- perhaps an ocean -- beneath its surface.
Cassini discovered the water-ice jets in 2005 on Enceladus. These jets expel tiny ice grains and vapor, some of which escape the moon's gravity and form Saturn's outermost ring. Cassini's cosmic dust analyzer has examined the composition of those grains and found salt within them.
"We believe that the salty minerals deep inside Enceladus washed out from rock at the bottom of a liquid layer," said Frank Postberg, Cassini scientist for the cosmic dust analyzer at the Max Planck Institute for Nuclear Physics in Heidelberg, Germany. Postberg is lead author of a study that appears in the June 25 issue of the journal Nature.
Scientists on Cassini's cosmic dust detector team conclude that liquid water must be present because it is the only way to dissolve the significant amounts of minerals that would account for the levels of salt detected. The process of sublimation, the mechanism by which vapor is released directly from solid ice in the crust, cannot account for the presence of salt.
"Potential plume sources on Enceladus are an active area of research with evidence continuing to converge on a possible salt water ocean," said Linda Spilker, Cassini deputy project scientist at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "Our next opportunity to gather data on Enceladus will come during two flybys in November."
The makeup of the outermost ring grains, determined when thousands of high-speed particle hits were registered by Cassini, provides indirect information about the composition of the plume material and what is inside Enceladus. The outermost ring particles are almost pure water ice, but nearly every time the dust analyzer has checked for the composition, it has found at least some sodium within the particles.
"Our measurements imply that besides table salt, the grains also contain carbonates like soda. Both components are in concentrations that match the predicted composition of an Enceladus ocean," Postberg said. "The carbonates also provide a slightly alkaline pH value. If the liquid source is an ocean, it could provide a suitable environment on Enceladus for the formation of life precursors when coupled with the heat measured near the moon's south pole and the organic compounds found within the plumes."
However, in another study published in Nature, researchers doing ground-based observations did not see sodium, an important salt component. That team notes that the amount of sodium being expelled from Enceladus is actually less than observed around many other planetary bodies. These scientists were looking for sodium in the plume vapor and could not see it in the expelled ice grains. They argue that if the plume vapor does come from ocean water the evaporation must happen slowly deep underground rather than as a violent geyser erupting into space.
"Finding salt in the plume gives evidence for liquid water below the surface," said Sascha Kempf, also a Cassini scientist for the cosmic dust analyzer from the Max Planck Institute for Nuclear Physics. "The lack of detection of sodium vapor in the plume gives hints about what the water reservoir might look like."
Determining the nature and origin of the plume material is a top priority for Cassini during its extended tour, called the Cassini Equinox Mission.
"The original picture of the plumes as violently erupting Yellowstone-like geysers is changing," said Postberg."They seem more like steady jets of vapor and ice fed by a large water reservoir. However, we cannot decide yet if the water is currently 'trapped' within huge pockets in Enceladus' thick ice crust or still connected to a large ocean in contact with the rocky core."
The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Cassini cosmic dust analyzer was provided by the German Aerospace Center. The Cassini orbiter was designed, developed and assembled at JPL. JPL manages the mission for the Science Mission Directorate at NASA Headquarters in Washington.
More information about the Cassini mission is available at: