Advancing Basic Science for Humanity
Building the Universe Pixel by Pixel
Three 'mapmakers' of the universe – Ralf Kaehler, Stuart Levy and Dylan Nelson – discuss how their dramatically intricate 3-D universes can tell important stories about the cosmos.
RECENTLY, the Harvard-Smithsonian Center for Astrophysics unveiled an unprecedented simulation of the universe’s development. Called the Illustris project, the simulation depicts more than 13 billion years of cosmic evolution across a cube of the universe that’s 350-million-light-years on each side. The goal was to view the formation of galaxies and other large-scale structure we see around us today, to test our understanding of what makes up the universe – including dark matter and dark energy – as well as how those components interact. It was a massive undertaking, one that took more than 5 years to complete. But why was it important to conduct such a simulation?
Highlights from the Illustris simulation, which tracks the expansion of the universe, gravitational interactions, and the formation of stars. (Credit: Illustris Project)
To better understand the science and art of astrophysics visualizations, three experts came together in late July to discuss the ways in which their work benefits both science and the public’s perception of science. The participants:
- RALF KAEHLER - is a physicist and computer scientist by training who now runs the visualization facilities at the Kavli Institute for Particle Astrophysics and Cosmology, located at SLAC National Accelerator Laboratory and Stanford University.
- STUART LEVY - is a research programmer and member of the National Center for Supercomputing Applications’ Advanced Visualization Lab team, which creates high-resolution data-driven scientific visualizations for public outreach.
- DYLAN NELSON - is a graduate student at the Harvard-Smithsonian Center for Astrophysics and a member of the Illustris collaboration, which recently completed a large cosmological simulation of galaxy formation.
The following is an edited transcript of a roundtable discussion. The participants have been provided the opportunity to amend or edit their remarks.
THE KAVLI FOUNDATION: Dylan, you’re a member of the Illustris project team, so let’s start with you. Illustris was a massive undertaking, one that took more than 5 years to complete. Why was it important to conduct this simulation?
DYLAN NELSON: This simulation tested our big-picture understanding of the universe’s evolution. We can’t just compare the observation of one galaxy; we need to compare whole populations of thousands or tens of thousands of galaxies, and the simulation lets us do this by creating a big volume of the universe. In visualizing this simulation, we found some unexpected features that in retrospect really shouldn’t have been unexpected at all. For example, when we made a movie showing the temperature of gas in the universe evolving over time, we saw that galaxies had a tendency to flicker rapidly. We traced this back to one of the three ways in which we let supermassive black holes input energy into the galaxies within which they reside. Although we expected that the energy would affect the temperature of the gas, we didn’t know how intermittent it would be, how it would create these flickers and bursts. That’s really something that we were surprised by, and something that made us rework our models a bit.
TKF: Ralf, what types of insights are gained through the visualizations you create with scientists at the Kavli Institute for Particle Astrophysics and Cosmology? Do you also tend to find unexpected features?
Ralf Kaehler runs the visualization facilities at the Kavli Institute for Particle Astrophysics and Cosmology.
RALF KAEHLER: What I often hear from scientists is that they gain intuition from watching the animations we create, intuition that’s hard to get from just looking at the raw numbers. They see how gas moves, how dark matter clumps on smaller scales and then merges and forms larger and larger clumps of dark matter. And it seems like this intuition is very important for a thorough understanding of the processes.
Another very important advantage visualizations offer is the ability to catch errors in the simulations. By just looking at the numbers, it can be easy to miss these errors. But when watching an animation they can become totally obvious. We can easily see if there’s some discontinuity in the data that shouldn’t be there and then you can investigate further if it’s a feature or an artifact or a bug. The software used to produce these simulations usually consists of hundred thousands or millions of lines of code. Codes of that size often contain bugs and visualizations can help to determine if there’s an error hidden within the code.
TKF: It sounds like visualizations are especially good for identifying issues with your assumptions or the underlying models. Stuart, would you agree with that?
Stuart Levy creates high-resolution data-driven scientific visualizations for public outreach at the National Center for Supercomputing Applications.
STUART LEVY: I think that’s a really good point, and it’s something that people talk about when they’re thinking of doing a visualization. If you reduce things to a graph with some statistics on it, in choosing what the statistics should measure, you’re saying what the interesting things are. And the hope is that if you can present something visually, you might end up bringing in things that you didn’t expect to bring in.
To me, it also seems like visualizations are becoming more and more useful for looking at very large-scale phenomena. As in observational astrophysics, instead of spending a lot of time looking at modest numbers of individual objects, people are looking at huge numbers of objects.
NELSON: I agree with that. Large simulations like Illustris are similar to big observational surveys. When you’re not looking at individual objects, you need sophisticated visualization techniques to pull out the interesting information. For instance, back when the kind of cosmological simulations we do today first started, people plotted a point for each dark matter particle. They learned lots of science from doing that. But these days, when the biggest dark matter simulations include a trillion particles, that’s not going to get you as far. You’re going to need more sophisticated visualization approaches – as well as machine learning techniques or other automated ways of finding interesting trends in the simulation. We’re working on that.
TKF: Even though all three of you create visualizations, your roles and your connections to the scientific questions driving the research are different. How does the process work for each of you? Who comes up with the scientific questions you seek to answer?
KAEHLER: For us, it’s often an interactive process. We sit together in front of the screen and analyze the data in real-time. I try to design a lot of the algorithms in a way that they produce visualizations pretty quickly, so that we can change parameters like the camera position or the color maps in real time and get an updated image in a fraction of a second. That way, we can explore the data together, focusing on regions of interest, zooming in and out, things like that. Other times, it’s more offline, where I’ll render something overnight and send the result to the scientists and let them have a look at that.
I would also say that while half of my work is for scientists, the other half is for outreach. Sometimes we create visualizations purely for outreach purposes, and sometimes we can use the same visualization for both science and outreach. In the latter case, the scientists first analyze the dataset and then we tweak it a little bit, spending more time with the camera path and the color scheme to make it look a little bit prettier before we use it for planetarium shows.
Dylan Nelson is a member of the Illustris collaboration, which recently completed a large cosmological simulation of galaxy formation.
NELSON: The process for me is a little different because my primary responsibility is science. It’s only a secondary responsibility that lets me create visualizations. I always say that when I create visualizations, it’s both for scientific exploration and for dissemination to the public. But I think in reality, in my research group we do those two things in completely different ways.
We need visualizations to understand what is going on in a simulation, to better understand our models and the physical processes we’re simulating. But those visualizations are not pretty; we do them as quickly as possible, and as soon as we have a useful science result, the effort on the visualization stops. On the other hand, when we’re doing a visualization for outreach, that’s really intended to make people say “Oh, wow, that’s really cool!” So there’s a lot more time spent past the point of scientific realization, polishing and making the visualization look visually impressive.
LEVY: My group really focuses on outreach. So we usually have an idea for a show first, then we’ll go and look for scientists who work in that area and can provide the simulation. They’ll also tell us what we should believe from their simulations and what we shouldn’t believe. Often they’ll be making simulations they know are representing some aspects of reality well and others less well. And so they’ll say something like, don’t pay attention to the temperature here, since we’re not including everything that could be heating things up. We’ll go back and forth both with the scientists and the people producing the show to create something that’s both interesting and scientifically correct.
That said, we do occasionally work with scientists on unanswered questions – though it’s not always in the realm of astrophysics. A few years ago, we were working with a simulation of a tornado. One of the things that the scientists were interested in learning was the origin of tornados. Most severe storms don’t create tornados, so what’s special about the subset of storms that do? They had an idea that we should be looking in the simulation for a feature that’s called a rear flank downdraft – a storm that’s flowing in a certain way. We were looking for this signature in the visualizations and just not finding it. But then one of the graduate students picked out this sort of rolling feature – a horizontal bunch of rolling air – and succeeded in convincing his senior professors that, in this simulation at least, it was that feature and not a rear flank downdraft that triggered the tornado. That was a surprising result, one made possible by the visualization.
TKF: What have been the big breakthroughs in visualization in the past five years? Are there new technologies or revelations that make possible all you’ve just described?
LEVY: Bigger disks! It seems a little mundane, but the ability to store huge amounts of data is really important. A couple of years ago, we got about four terabytes of data from a scientist. A few years earlier, that would have been an overwhelming amount, but today we could easily take on several of those. That makes a really big difference. The billion-dollar gaming industry has also been an incredible boon to us. It’s on the back of that industry that high performance graphics cards have been built. Fifteen years ago, the fastest graphics hardware cost the price of a house. In just a few years, that was superseded by hardware that you could get for a couple of thousand dollars. Now it’s come down to a few hundred dollars, and we’re able to use it routinely. If not for the gaming industry, we wouldn’t have all of the graphics processor power that we need.
KAEHLER: I completely agree with Stuart here. The ever-evolving capabilities of graphics hardware are very important for this work. You can now realize interactive visualizations of datasets that were far out of the reach of standard desktop workstations five or ten years ago.
This visualization follows the formation of the universe over billions of years, as filaments of dark matter (shown in black) begin to take shape. The intersections of those filaments host massive clusters of galaxies (shown in yellow). (Credit: Ralf Kaehler, Carter Emmart, Tom Abel, Oliver Hahn)
KAEHLER: I would say that there’s a lot of creativity involved in the process. It might be comparable to taking a photograph of some object. You have all of this freedom of how to choose your camera position, lighting conditions, color filters and so on. Similarly, with the same numerical simulation, you can end up with millions of different images by changing around these variables. So it really depends on the audience you’re targeting, what features in the original dataset you want to highlight, and what story you want to get across. If different people work on visualizations for the same dataset, the results can be totally different.
One of our most recent visualizations was a collaboration with the Hayden Planetarium at the American Museum of Natural History in New York. It shows the role of dark matter in forming the larger structures in the universe. For this audience, we took the term dark matter a bit more literally than usual. If we had done this rendering for scientists, we would have represented higher dark matter densities in brighter colors. But studies have shown that often confuses the general public. So in this visualization, we actually turned it around and rendered the dark matter in darker colors and added some background light. That helped guide the audience and clarified what was dark matter and what was not.
LEVY: I agree. I think we should look at visualization like mapmakers look at map making. A good mapmaker will be deliberate in what gets included in the map, but also in what gets left out. Visualizers think about their audience, as Ralf says, and the specific story they want to tell. And so even with the same audience in mind, you might set up the visualization very differently to tell different stories. For example, for one story you might want to show only what it’s possible for the human eye to see, and in others you might want to show the presence of something that wouldn't be visible in any sort of radiation at all. That can help to get a point across.
TKF: It sounds like there’s quite a bit of room for artistic choice. For outreach purposes, then, why is it important for the visualizations to be based on scientifically accurate data? Why are you creating them, rather than a movie house?
KAEHLER: Using sophisticated numerical simulations ensures that the science is depicted correctly. Besides this, it’s hard to model a lot of the phenomena in astrophysics using the artistic tools that Hollywood movies employ. The phenomena are just too complex to draw by hand. I think more and more of these artistic tools are now starting to incorporate some sort of simplified simulation codes in order to model things like explosions, to make it look more realistic.
This visualization of the surface of the sun was produced for an upcoming production at Chicago’s Adler Planetarium. (Visualization: NCSA Advanced Visualization Lab / Data and simulation: Mathias Rempel, M.C.M. Cheung and Steele Hill)
NELSON: It’s kind of amazing, to be honest, the amount of press and public interest that’s come out of the Illustris project. Actually, just yesterday I got a call from my father, who had been browsing the news on his phone and saw an image from Illustris on the front page of the New York Times website. This was a still image that we made just for the purposes of putting it on the website, and it’s probably appeared in a dozen newspapers so far. It’s great that there’s so much interest, and that the images are becoming almost iconic.
LEVY: For me, it’s great to watch visualizations in planetarium domes. It’s the most wonderful thing to lie down in the middle of a planetarium – or even in an IMAX theater – and just look up. Having the audience completely surrounded by what they’re seeing can be really breathtaking.
KAEHLER: I love it when visualizations are shown in planetariums, too. It just looks so impressive – much more impressive than looking at the visualizations on a flat monitor in my office. I’ve worked on visualizations that were shown in places like the American Museum of Natural History and the Morrison Planetarium at the California Academy of Sciences. These are great places to reach a lot of people in a nice, inspiring environment. Even though when I’m sitting in the audience it’s too dark to gauge other people’s reactions, sometimes we get emails from people who saw the planetarium shows and write how much they liked it. It’s really motivating, and shows that our time is being well invested.
— Kelen Tuttle (Summer, 2014)