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Astronomy at the Frontier Matt Mountain, Ph.D. Director, Space Telescope Science Institute As Director of the Gemini Observatory, Charles Mattias (“Matt”) Mountain led the design, construction, and operation of Gemini’s two 8-meter telescopes in Hawaii and Chile. Since 2005, he has served as Director of the Space Telescope Science Institute (STScI) in Baltimore, Maryland, where he is responsible for the science operations of the Hubble Space Telescope. He is also the Telescope Scientist for NASA’s James Webb Space Telescope, as well as a professor in the Johns Hopkins University Department of Physics and Astronomy. Unique observations At school, I became interested in physics because it allowed me to work in a lab and build things and see how they worked. I could try to understand how the universe worked and how rockets worked. I got my degree in physics at Imperial College in London. Afterward, I considered becoming a particle physicist, but then I was given the opportunity to see a telescope operating in the Canary Islands. In those days—this was the 1980s— astronomy was still a science that allowed an individual to make unique observations. It was small science, and that appealed to me. I went on to get my Ph.D. in observational astrophysics. Impossible discoveries A lot has changed since then. Today, the average ground telescope weighs 300 tons. It takes hundreds of people just to build and operate. Astronomy has become a multidisciplinary science that requires not only physicists and astrophysicists, but also optical scientists, cryogenicists, engineers, and computer scientists. Astronomy, at the frontier, has become a big science where you need large teams of people working together. Astronomers still speak romantically of how it used to be so nice to be alone, off on the summit, looking out at the stars, but that’s no longer how we do it. Nobody “looks through” the Hubble: you upload commands and the Hubble downloads data, which is then processed and sent out 6 imagine to the observer on the Internet. This separation between astronomer and machine represents a dramatic change, but this huge base of talent and these amazing machines are allowing us to make discoveries we thought were impossible two decades ago. A scientific renaissance When I got into the field, the only planets we knew were in our own solar system. Black holes were figments of a theorist’s imagination. Now we’ve identified over 3,000 planets. We know that every star in our galaxy has at least one planet and that there are approximately 100 billion planets in our galaxy. Black holes are in the center of every galaxy. We have dark energy and dark matter. We know the age of the universe, and all this has happened in the last 20 years. It’s like a renaissance of science. It’s also been somewhat humbling, though. We discovered that we understand only four percent of the universe. Dark matter and dark energy dominate the other 96 percent, and we haven’t a clue what they are. But those very facts, and the fact that we now know there are planets around every star and that we’re on the verge of measuring what might be on those planets—you couldn’t have imagined that 20 years ago. There are two big factors that have contributed to these advances. One is the sheer power of the telescopes and technology. Then there’s the explosion of data and the inter-comparison of data across different wavebands. It’s now quite normal for scientists to take data from the Hubble, the infrared Spitzer telescope, and ground-based telescopes, and combine them into data sets. Data-driven discoveries Twenty years ago, astronomers agreed amongst themselves, internationally, on a standard format for all their data irrespective of which telescope it came from or what waveband they use. This has allowed us to build amazing archives of data. Today, half the refereed papers from Hubble—which is a measure of scientific output—come from the data in our archives, not from the telescope. By applying new computing techniques to old Hubble data, we’re discovering planets that had been hidden in the data. When I started, we had radio astronomers, infrared astronomers, and optical astronomers. Today we have specialists in exoplanets, galaxies, or black holes. They comb Sept/Oct 2014 NASA, ESA, H. Teplitz and M. Rafelski (IPAC/Caltech), A. Koekemoer (STScI), R. Windhorst (Arizona State University), and Z. Levay (STScI) in my own words Hubble Ultra Deep Field 2014 roughly 300 miles an hour. To get it into orbit, it has to fly at 17,000 miles an hour. You need at least 1,000 times more energy than a 747 has to get the shuttle into orbit, and that’s really hard. Even though rocketry’s been around since World War II, it’s still very hard. That also means it’s very expensive. Now we have NASA-funded private players like SpaceX. They’re just launching cargo and they’re still finding it really hard to launch into space. But because private companies can innovate and be flexible, they have the ability to cut the cost to orbit—and maybe even cut the cost to deep space. through data from the various telescopes looking for the phenomena they’re interested in. They use the multi-wavelength bands and the archives, and they apply for telescope time so they can contribute new observations to the archive. This generation is completely at ease using big data to cross-compare, and they’re making a lot of discoveries. When Adam Riess and his collaborators discovered dark energy, they did so using a network of telescopes all over the planet and off the planet. They used small telescopes, then followed up with ground-based telescopes, and then used the Hubble Space Telescope, and they cross-compared the data. It couldn’t have been done without the interconnection of all these data sets. No looking back The Space Telescope Science Institute is a very exciting place to be. Every day, we’re deciding what the Hubble is going to do. We’re getting to see what the new data looks like and what discoveries our community is going to make. We’re also preparing for the James Webb Space Telescope. With the Webb we will, for the first time, be able to detect the presence of liquid water on planets in just-right regions—the so-called Goldilocks zone. Which immediately leads to the question, Is there life out there? Knowing that there is life on another planet would change everything, because once we’ve discovered that, there’s no looking back. Discovering life on another planet would change our whole perspective as a species. Astronomical challenges But getting a seven-ton telescope like the Webb into space is no easy matter. If you’ve watched Star Trek or Star Wars, it looks easy to get out into space. It isn’t. Consider the Space Shuttle, which was about the size of a 747. A 747 flies at www.cty.jhu.edu/imagine An expensive endeavor Not only is it hard to get anything into space, but once it’s there, it’s in a vacuum. We’ve got to build equipment that will work in a very cold, radiation-filled vacuum. We’ve had to carry all that mass into orbit, which is really expensive, and most of the time, if we make a mistake, we can’t fix it. The Hubble is unique. It was designed so that astronauts could fix it. At the time, we had the shuttle system to take astronauts up to fix it, but we no longer have that capability. The Webb will be tested for two years to ensure there are no mistakes. Then we’ll launch it on an Ariane 5 rocket out beyond the Moon, about a million miles from here, where it will be completely inaccessible to humankind. It has to work reliably for at least a decade. That means a lot of testing, thought, and engineering, which is extraordinarily expensive. Managing big science This is not a field for the faint-hearted. You have to be very patient to accumulate the good will, consensus, and partnerships to get the resources you need for something like the Webb, which will cost $8 billion to launch. You need very large multinational collaborations and agencies, like NASA, and you have to be willing to work in the kind of bureaucracy big organizations have. On the other hand, the rewards are enormous. The young people who work here get to help decide what the Hubble does or what the Webb will do. They’re brimming over with excitement at the opportunity to control where the U.S.’s premier telescopes look and to be the first to see the data that comes down. We’ve been working on new technologies in order to produce a second-generation Webb 10 or 15 years from now that could actually discover life on other planets. Yours may be the generation that makes that discovery. It may be your telescope that we build. n imagine 7