. He realized that the software that turns computer code into a Milky Way for the daytime audience could transform the cluster simulators columns into a sky full of careening, caroming stars. Sitting under the dome, the scientists could see whats happening as if they were hovering outside the cluster or even sitting inside it. "Seeing it in three dimensions is different, said Simon Portegies Zwart, a stellar dynamist at the Massachusetts Institute of Technology.
Hut got in touch with Emmart, a computer and graphics expert who designs and runs the Planetariums simulations. Certainly doable, Emmart said. In fact, the project, which began last summer, has gone so well that the scientists are working with the creators of Virtual Director -- the software the museum uses to run its shows -- and theyre starting to think about ways the model could depict non-stellar processes, such as gases in turbines, global economies or panicky crowds, for instance.
"I think the basic issues we are trying to address -- large ranges in spatial and temporal scales, and the need to handle huge volumes of data -- are by no means unique to starcluster dynamics, so we would hope that many of our techniques would find application well beyond astronomy," McMillan said.
Far out
This summer, I met Hut, McMillan, Portegies Zwart and a few other astronomers and computer mavens in a dark museum corridor, and we paced over to the planetarium, under the shadows of Polynesian totem poles and past the yellow glow of stuffed animals and plaster people in the museums dioramas. This was the maiden voyage for the project -- a simulation of 10,000 clustered stars as presented by the planetariums image-making computers and projectors. It began after dinner, with an hour or so of computer massaging, after which we all walked into the cavernous dome and sat down.
The gray dome turned a pure black, and what looked like a clear night sky filled with white and orange stars gliding around like ice skaters. When two came close, theyd fall toward each other as if they sky had formed a slope. Some collided, forming new stars. Others would whirl round and round each other and then go waltzing off together.
"Thats a nice binary," said McMillans voice in the dark, as one of these couples sailed over our heads. Another binary sped by with a different style -- one star running straight and level, the other boing-boinging around it like a cartoon kangaroo. We watched as the binary fad spread, and more and more stars formed pairs. Sometimes binaries grabbed a third party, spinning it around before sending it zooming off in another direction.
When Emmart changed the parameters to show pathways as well as dots, the sky seemed to fill with sloping, twisting, corkscrewing paths in yellow and blue. Scale vanished. It was as easy to imagine these forms as proteins twisting into functional shapes as it was to see stellar paths. The movements seemed patterned, yet in no obvious way. It was like swimming in a pond full of lively microbes, or watching a movie in a language you dont speak.
"Its really beautiful, said Portegies Zwart, looking up at this surreal sky. "Im very impressed."
After about an hour of craning our heads, McMillan said: "Were not really getting it all."
"Right," others echoed.
We moved to the center of the floor. A giant Zeiss projector usually sits there during shows, but it was stored underneath us for the night. We lay down, staring straight up, like kids on a summer night, and watched a few more millions of years go by. As McMillan emailed me afterwards, "It certainly gives a whole new meaning to being immersed in one's work!"
After a 2 a.m. beer and a few days to think it over, the scientists agreed: the dome images looked great, and it was cool that they worked, but best of all, they were useful.
In the dome, McMillan said, "you get to take in the whole system at once. Usually we focus on specific interactions, but we have never really had the capability of following many at once, or for long periods of time."
"We saw how a few stars in the center of the cluster had chaotic orbits which could not at all be described by the standard orbital theories in which we are used to think, wrote Portegies Zwart via e-mail.
The next stage is to ramp up to more stars in the dome. And then to add individuality -- variations in luminosity, temperature and size that will make the simulated cluster more like the ones observing astronomers see through their telescopes. As the simulations get ever more complex, stellar dynamists will keep returning to the dome to see how it all looks from the center of a cluster, as millions of years fly by like minutes.
"Thats science," said Portegies Zwart. "Seeing what no one has seen before."