Transporting the ALMA observatory’s 100-ton antenna dishes requires a truck with two 700-hp engines.
The first scientist I meet at the Atacama Large Millimeter/submillimeter Array (ALMA) telescope site is wearing a portable oxygen tank. At 16,400 feet in the Andes, he’d be unable to think clearly without the tube up his nose. He runs the observatory’s brain-a supercomputer as powerful as three million laptops working together that compares light from the telescope’s 66 dishes quadrillions of times every second. Everything about this place is designed for high-altitude survival. The curved roof can withstand 145mph winds. Heated blankets prevent the toilet cistern from freezing. The dishes themselves point to the sky with 0.6-arc-second accuracy, despite the winds and radical temperature swings. It’s the people that are the weak link. Workers are allowed to spend only six hours a day at the ALMA “high site,” the scientist explains. As I write that down, I realize I’m feeling dizzy.
A few minutes later, flat on a cot under an oxygen mask to avoid fainting, I look out the medical room’s window at the lifeless, Mars-like landscape. The silvery radio dishes are engaged in a quiet ballet, swinging above the red dirt in perfect unison. Their synchrony and precision are two of the reasons ALMA is the most ambitious ground telescope ever built. Another is the observatory’s unparalleled adaptability; it has the most dishes that can be trucked around to different locations. Because of all these special features, ALMA will produce images 10 times sharper than the Hubble Space Telescope does.
Telescopes have always had one major problem: the Earth’s atmosphere bends light, distorting images. That’s why telescopes are often built at high altitudes, where the atmosphere is thinner, and why NASA put Hubble in space-to get beyond the atmosphere entirely. But space scopes aren’t perfect. They’re a compromise by definition. They must be big enough to capture faint light but small enough to fit on a rocket, and repairs or upgrades either require exceptionally expensive trips into orbit or are simply impossible. Now, however, increasingly sophisticated adaptive optics that adjust for the atmosphere’s blurring effect are making many telescopes on Earth as good as anything that we could put in the sky. ALMA captures radio waves, and soon workers will break ground on two observatories that see visible light instead: the Thirty Meter Telescope, with a resolution more than 10 times as high as Hubble’s, and the Large Synoptic Survey Telescope, which will photograph the entire sky every few nights.
ALMA’s 66 antenna dishes work as one massive telescope, which can see sharp detail or broad features by changing its aperture from 500 feet to 10 miles. To achieve this flexibility, workers use massive trucks, each with 28 tires, to transport the 100-ton dishes. Each antenna is placed (to a fraction of a millimeter of accuracy) at one of 192 bases that have a hard line to the supercomputer nearby.
ALMA will watch a gas cloud
spiral into the black hole at the center of the Milky Way.By the end of the year, when all of its dishes are online, ALMA will have 100 times the imaging resolution of any scope looking at very short radio waves, which emanate from cool, dark sources such as interstellar dust and from bright, distant galaxies. But it’s already had some impressive finds. In March, astronomers discovered surprising numbers of “starburst” galaxies, where new stars were forming a billion years earlier than anyone thought. This summer, they might have found evidence of dust traps near stars that help the formation of planets, asteroids, and comets. And eventually, ALMA will watch a gas cloud spiral into the black hole at the center of the Milky Way, look for molecular signs of life on faraway worlds, and measure the location and density of the mysterious substance scientists call dark matter-all from a high desert on planet Earth.
This article originally appeared in the September 2013 issue of Popular Science.
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