Astronaut Lawrence DeLucas will reminisce his training to be a NASA astronaut and share his experiences flying on the Columbia Space Shuttle Mission STS-50, launched on June 25, 1992. He will descibe the materials, technology, and research performed in that mission and summarize the research underway on the International Space Station. He will discuss NASA's plans for a human-piloted mission to Mars.

Lawrence DeLucas' talk is part of "An Evening of Wonder: Life and Art on Earth and Beyond." This astrobiology fun-and-learning event for the whole family is made possible by the organizers of AbGradCon 2018.

AbGradCon (Astrobiology Graduate Conference) is a popular gathering of early-career scientists interested in astrobiology research, held in a different location every year. 

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Understanding earthquake triggering and fault slip behavior based on complete earthquake catalogs

Large mainshocks can alter stress field on subsurface asperities across broad spatial and temporal windows, which would promote or inhibit fault motion. Beyond rapid rupture during earthquakes, fault can also slip at a steady rate without seismic radiation. In between these two end members, slow slip events have been documented within the conditionally stable transition zone.

Wildfires in Earth System: The Driver, Transport, and Feedback

Wildfires release large amounts of greenhouse gases, carbonaceous aerosols, and other pollutants, therefore having complex impacts on the earth climate, local weather, and air quality. To study the transport of the wildfire emissions, a plume height dataset has been developed. The resulting dataset from 2002 to 2010 captured well the observed MISR plume height distribution. By adding the plume height dataset in the climate model, the plume-rise enhanced AOD downstream of the wildfire spots by 20 to 50%.

December 31, 1969 |

When Amy Lynn Williamson moved to Georgia to attend Georgia Tech, it was the first time she had ever moved from Ohio, where most of her family lives. She completed her B.S. in Geosciences at Denison University, in Granville, a small town close to home. For Williamson, the move to Midtown Atlanta was a big step.

But she couldn’t resist the draw of Georgia Tech. “I was attracted to Georgia Tech because of its close-knit geophysics department,” Williamson says, “Even though Georgia Tech is a large research-oriented institute, EAS [School of Earth and Atmospheric Sciences] maintains a small and supportive environment.” Interdepartmental group meetings, yearly student symposia, and a graduate student activity group are some features of EAS that, she says, made her feel part of the community.

Williamson is receiving a Ph.D. in Earth and Atmospheric Sciences.

What is the most important thing you learned at Georgia Tech?

Georgia Tech taught me not only how to conduct research but also how to communicate it to a wider audience. In the research group of Andrew Newman, everyone worked on the same broad topics but each one had distinct research projects. This means constantly presenting and discussing our work and learning about everyone else’s projects. I had opportunities to present my research in small group meetings and in domestic and international conferences.

Georgia Tech and EAS were helpful every step of the way, from travel to large conferences to facilitating small symposia and events in the school.

"Georgia Tech and the School of Earth and Atmospheric Sciences were helpful every step of the way, from travel to large conferences to facilitating small symposia and events in the school."

What is your proudest achievement at Georgia Tech?

Defending my Ph.D. dissertation.

Not only am I in the first generation of my family to attend college, but I also will be the first person in my family to hold a doctorate degree.

What is your most vivid memory of Georgia Tech?

The hours spent in the gym with my groupmate discussing research and getting in shape to prepare for lugging instruments up the side of Costa Rica’s Arenal Volcano.  

Who knew that lunges and talks about crustal deformation would mix?

What unique learning activities did you undertake?

During my first summer, I joined a research cruise to retrieve ocean bottom seismometers from off the coast of Vancouver Island. This experience showed me the breadth of research in seismology and geodesy. It was also my first to be on a research ship, and – given my new-found knowledge of sea sickness – it might be my last.

Midway through my Ph.D., I participated in a research-abroad program hosted by the National Science Foundation and the Australian Academy of Sciences. The program allowed me to work with new research collaborators in Canberra, Australia. 

During this trip, I gained new perspective about my research by interacting with research groups that I otherwise would have interacted with only occasionally. I also experienced living and working abroad and the surreal situation of having a mob of kangaroos live right outside my front door.

What advice would you give to incoming graduate students at Georgia Tech?

Be involved in the greater Atlanta community. Get involved in outreach related to your field, attend events off campus, and make Atlanta more like a home, and not just a place where you work and study.

Even though I love Georgia Tech, it was great to get off campus, explore, and meet new people. I did this through running, with the local running club. Keeping up with a hobby off campus also helps manage the stressful moments during graduate studies.

Where are you headed after graduation?

I am headed to the University of Oregon where I will be a postdoctoral researcher focusing on tsunami hazards for the Pacific Northwest. My studies in the Newman research group helped me prepare for this role. Even though my dissertation topic and my future work in Oregon focus on a field that is not currently a major research area in Georgia Tech, my advisor has been incredibly helpful.

December 31, 1969 |

For the foreseeable future, the only real tool to find life on potentially habitable planets that are light years away from Earth is to probe their atmospheres for biological fingerprints of life, called biosignatures.

This approach has two drawbacks, according to School of Earth and Atmospheric Sciences Assistant Professor Christopher Reinhard. “Some biosignatures can be made by abiotic processes, leading to false positives. Others can be masked by processes that consume biosignatures, leading to false negatives.”

To overcome these problems, Reinhard and colleagues in the NASA Astrobiology Institute Alternative Earths and Virtual Planetary Laboratory Teams are proposing use of dynamic biosignatures based on seasonal changes in Earth’s atmosphere. The approach – described recently in Astrophysical Journal Letters – uses the seasonal variation of biologically important gases as a way to deal with false positives and false negatives, Reinhard says.

Seasonality of Atmospheric Gases

As Earth orbits the sun, its tilted axis means different regions receive more rays at different times of the year. The most visible signs of this phenomenon are changes in the weather and length of the days, but atmospheric composition is also affected. For example, in the Northern Hemisphere, which contains most the world’s vegetation, plant growth in summer results in noticeably lower levels of carbon dioxide in the atmosphere. The reverse is true for oxygen.

“Atmospheric seasonality is a promising biosignature because it is biologically modulated on Earth and is likely to occur on other inhabited worlds,” says lead author Stephanie Olson, a graduate student in the Department of Earth Sciences of the University of California, Riverside (UCR). “Inferring life based on seasonality wouldn’t require a detailed understanding of alien biochemistry because it arises as a biological response to seasonal changes in the environment, rather than as a consequence of a specific biological activity that might be unique to Earth.”

In the study – funded by the NASA Astrobiology Institute and the National Science Foundation Frontiers in Earth System Dynamics – the researchers identify the opportunities and pitfalls in monitoring the seasonal ebbs and flows of oxygen, carbon dioxide, methane, and ozone. They also modeled fluctuations of atmospheric oxygen on a life-bearing planet with low oxygen content, just as Earth was billions of years ago. “Based on these evaluations,” Reinhard says, “seasonal variations in ozone could be a sensitive biosignature on planets with undetectable levels of oxygen in their atmospheres.”

Ozone as Indicator of Life

At Georgia Tech, the Reinhard research group develops comprehensive models for the production and maintenance of robust atmospheric biosignatures on habitable planets, and it played a key role in developing the concept of ozone seasonality as a fingerprint for life on low-oxygen planets. The idea emerged in part as an answer to the “biosignature blind spot” problem Reinhard and colleagues posed in the 2017 Astrobiology paper “False Negatives for Remote Life Detection on Ocean-Bearing Planets: Lessons from Early Earth.” 

“We are particularly excited about the prospect of characterizing oxygen fluctuations at the low levels we would expect to find on an early version of Earth,” says Timothy Lyons, a professor of biogeochemistry in UCR’s Department of Earth Science and director of the Alternative Earths Astrobiology Center. “Seasonal variations as revealed by ozone would be most readily detectable on a planet like Earth was billions of years ago, when most life was still microscopic and ocean dwelling.”

“Although we think the conceptual framework for this approach is robust,” Reinhard says, “observing and quantifying seasonality represents a daunting challenge. Research will need to take into account modulation of seasonal signals by the angle at which we observe a planet and the shape of its orbit, among other factors. Nevertheless, seasonality represents a potentially powerful approach toward finding life beyond our solar system.”

December 31, 1969 |

In 2017, Georgia Tech researchers were still celebrating the discovery of gravitational waves rippling through space-time when another celestial phenomenon captured their attention. College of Sciences Dean Paul Goldbart, who leaves us this summer to join the University of Texas at Austin, recalls the excitement over kilonovas and how they may be responsible for the gold in your wedding ring.

In this second part of our conversation with Goldbart, he charts the rapid growth of the new neuroscience degree program, tells us where he sees future opportunities for the College of Sciences, and explains why science matters — not just on campus, but in many aspects of daily life.

This audio news story also serves as a preview of ScienceMatters, the College of Sciences podcast coming in the summer. If you want to learn more about ScienceMatters, click here.

Click at the image on the right to listen or read the full transcript below.

Renay San Miguel: Hello. I’m Renay San Miguel with the Georgia Tech College of Sciences. We continue our conversation with Paul Goldbart, outgoing dean of the Georgia Tech College of Sciences, also the college’s Betsy Middleton and John Clark Southerland Chair. We taped this interview in February. With Paul’s appointment as the next dean of the College of Natural Sciences in the University of Texas at Austin, we’ve recast the interview as a two-part audio story serving as a valedictory for Paul, as well as a preview of our podcast “ScienceMatters,” coming in summer 2018.

A different kind of cosmic collision

We left off with a discussion of how College of Sciences’ researchers were part of a Nobel Prize-winning effort to confirm the existence of gravitational waves, something Einstein predicted 100 years ago. The first gravitational waves detected were the result of black holes colliding. It was a different kind of collision in summer 2017 that Georgia Tech’s researchers heard and saw while working with LIGO, or the Laser Interferometer Gravitational-Waves Observatories in Washington State and Louisiana. Here is School of Physics professor and LIGO deputy spokesperson Laura Cadonati, speaking in a 2017 Georgia Tech video.

Laura Cadonati: On August 17, something special happened. For the first time, we detected a  gravitational wave that was coming not from the collision of black holes, but from the collision of two neutron stars. A neutron star is what’s left after a star burns some of its fuel and implodes under its own weight. And this is going to give us important clues in where heavy elements are formed, how matter as we know it is formed, and which processes.

This has been exciting because we are really making use of both gravitational wave and the electromagnetic wave information to learn new things. We have really— [audio fades]

Renay San Miguel: Again, here is College of Sciences Dean Paul Goldbart.

Paul Goldbart: So if you take a cubic kilometer of Earth, it weighs about as much as a thimble full of neutron star matter, so incredibly dense. I believe if you were to take the sun and have it become a neutron star it would be about the size of the Georgia Tech campus. So incredibly dense matter and remarkable astrophysical objects.

And every now and again, these are present in pairs out there in the cosmos orbiting around one another. And in this event, two neutron stars rotated around one another, radiated out energy, and merged. And as they did, in this cataclysmic eruption of merger, which is called a “kilonova,” that was where nature manufactures roughly half of the heavy elements.

So if I look now as I am at my wedding ring, it has gold in it, I believe. And that gold was almost certainly cooked, manufactured, through the collision of two neutron stars out there in the cosmos.

[Music]

A fast start for neuroscience at Georgia Tech

Renay San Miguel: Tell me about some of the disciplines that are offering some exciting potential for scientists and researchers here at Georgia Tech. You talked about astrobiology. What other research are you wanting to keep an eye on here in the future?

Paul Goldbart: Yes, let me tell you a little bit about neuroscience. Neural engineering at Georgia Tech has been a growth field for a number of years and is doing very well. It has an international reputation, very strong. We have also begun to grow in neuroscience—neuroscience as opposed to neural engineering, although as with many science and engineering disciplines, there’s a great deal of overlap; a very soft zone separating them. So we’re delighted, in fact, that we have a tremendously strong community of neural engineers here at Georgia Tech.

I’ll tell you a short story: About four years ago or so, my colleagues in the College of Engineering dropped by the College of Sciences to say, “Hello.” I’d been dean for a few months. And we sat down, and they chatted, and they said we should have a neuroscience degree. And I thought about it for a little while, and I thought, they’re absolutely right.

And I went to see Associate Dean David Collard, and we discussed the idea and both of us agreed that this would be a marvelous step forward. Tremendous campus support, tremendous campus enthusiasm, we’ve been hiring neuroscience faculty to complement the neural engineers and build a really thriving and broad community of neural researchers here at Georgia Tech.

Let me emphasize: That was not my idea. That was already running, well before I became dean. And it’s really been doing very well with great campus support.And the centerpiece of this step forward is the creation of a neuroscience bachelor’s degree at Georgia Tech. And so until the summer of 2017, if one wanted to study neurosciences in undergraduate, much as we would love to have you, Georgia Tech was not the place for you.

It is now! And I have to say I’m tremendously excited, and we are finding that students are wildly enthusiastic about this new major. And it’s actually quite a delight to construct a major after they have been constructed at other places, as you can look around and you can think and you can really focus on the future. So I think we’ve caught it just right: great neuroscience but also neural technology options built in so that you really can train yourself as an undergraduate to be a neuroscientist of the future right here at Georgia Tech.

Renay San Miguel: And it’s my understanding you expected a certain amount of interest in the first year of the program, but you exceeded that.

Paul Goldbart: We certainly did. We certainly did. So the numbers are somewhere like 150 students in the first cohort, and that is marvelous, and the more the merrier. Of course, growth like that brings the occasional strain, but those are the strains that every dean loves to have. No complaints from me.

Renay San Miguel: This is a problem you want! [Chuckles]

[Music]

Making the case for science: Why science matters

Renay San Miguel: The name of the [forthcoming College of Sciences] podcast is “ScienceMatters.” Tell me why all of the science and research that we’ve talked about here so far, why that matters. What’s in it for all of us?

Paul Goldbart: Yeah, so there’s a tremendous amount in it for all of us. Let me start with the obvious. So the obvious is that science brings new understanding, and new understanding brings new capabilities and new power for humankind to control, and work with, and adapt and manipulate, ideally for sound, solid, good purposes, the world around us. And so science has given us tremendous opportunities to do that.

I like to look—to take the long sweep. I was at the dentist yesterday, and I was very fondly thinking of the folks who came up with anesthetics —

[Laughter]

— and it’s not very long ago. And so the same with vaccinations — vaccinations are tremendously important. Let me take the example of weather forecasting. A hundred years ago or so, catastrophic weather events in the city of Galveston, but all around the world and throughout history, we’re now in a situation where we may not be able to forecast weather with the kind of precision that any naysayer might choose to impose. 

But the fact is we are saving human lives; we are saving property by the millions of people per year and improving the human condition through that.

Now how does it come about? It doesn’t come about just by focusing on weather. It comes about by handshaking between all sorts of disciplines.

So without the understanding that silicon, in fact, is a semiconductor, we wouldn’t be in the situation of having solid-state circuitry and high-speed computers. And without beautiful ideas in applied mathematics, we wouldn’t be in a position to take accurate solutions of the complex nonlinear equations that describe the patterns of weather. Without electromagnetics, we wouldn’t have ultra-fast communications.

And so this handshaking of the web of understanding of the way the world works comes together and helps move forward to really change the human condition. Of course, that happens perhaps nowhere more importantly than in the fields of medicine where, across the board, one is confronted by examples in which it’s scientific understanding that has provided one, not all, but one of the keys to forward progress.

The example that I often like to cite is the laser. Lasers have had an amazing impact in eye surgery. I have friends who are ophthalmic surgeons, and they’re brilliant and I really appreciate them, but I don’t think any of them would have come up with the laser.

And so it’s this handshaking, this relationship, between the international web of science, international in space, but also going back in time, that has given human kind a sense of understanding, an ability to control, an ability to manipulate the world around us in terms of matter and energy; that is incredibly empowering.

A model for taking on complex problems

But I want to take it one step further if you don’t mind, Renay. I would like to argue, and I believe this quite deeply, that although science is not in a position to solve all our problems by any means — there are complex cultural and social and political problems that are challenging and hard to address, and I wouldn’t want to argue that all you need is a scientist to address them by any means — but I do think that we provide a model for how to think about and make progress with complex problems.

And I think the reason is that the scientific approach to problem solving has found a rather elegant and powerful balance between, on the one hand, reason, on the other hand, data, and on the other hand, third hand, creativity. And it’s this kind of intersection between all three together with the ability to let go of ideas that no longer seem to work and happily move on, that I think gives science not only its power in its own domain, but also serves as a great exemplar to the way that we, human beings, can address some of the deepest and most challenging issues that we face in economics and in politics and public health, so forth.

And I’ll also say that you may think of us, we scientists, as people who sit and solve complex equations. And we do do that from time to time.

But actually, what we really do is construct cartoon pictures of the way the world works in our heads or in our notebooks or on the chalkboard. And then what we do is make what we call back-of-the-envelope estimates: We sit down and we just ponder and reflect and put together the different pieces of scientific understanding and we make simple estimates — “Do I need a field that has the strength of one gauss to do this experiment, or do I need a field a million times bigger?” I need to know that before I consider the experiment or propose it to a funding agency.

So what we do all the time is make these estimates, and we get a feel for things. And that way of thinking, I think, is enormously empowering. I’ll call it semi-quantitative reasoning, and it’s something that I think we really need to advertise and propagate out into the world.

Just as an example: if I’m thinking about, let’s say, a topic like employment, I need to have some feeling for the numbers: What fraction of people are out of work? What fraction of people are looking for work? How many new jobs were created over the past eight years for example? So one has to have a kind of framework, a kind of feeling for numbers and relationships between them before one really seriously enters into arguments. And that way, one’s steered away from dogma and towards the light and that, I think, is what science can help us do.

[Music]

Planning for College of Sciences" growth

Renay San Miguel: Given what you’ve just talked about here since you’ve been here at the College of Sciences, what about your vision for the future here? How do you want to grow this college over the next, let’s say, five years?

Paul Goldbart: Yeah. So in my first five years or so as dean, we focused on many things including strengthening the infrastructure under which people can undertake research, building up tremendous capabilities in nuclear magnetic resonance and mass spectrometry and other areas, too, and I think that’s been great. We’ve also built facilities that people share and that creates community and promotes interaction. So I think we’ve supported the research endeavor with partnership with the campus well and I’m pleased with that.

We’ve also, I would say, we’re beginning to figure out how to create the best platforms for early-career scientists to learn how to navigate the complex web that is an academic life rather than leaving them to their own devices, but also without a heavy hand so we don’t too strongly influence the research that they choose to do. We are trying to find the middle ground to lift people up and really elevate the prospects for really great success.

I think we’ve also had an impact on the scale and energy in the undergraduate programs. We’re really in a marvelous partnership with the campus to increase the fraction of science majors and math majors at Georgia Tech from about 10 percent aiming for something like 20 percent just to give a kind of balance to the Georgia Tech community, and that’s coming along, I think, really well.

Looking forward to the next five years, I think for the college, one of the key objectives is to grow and strengthen the graduate programs. One of the reasons for this is that the reputation that we have worldwide and the impact, more importantly, that we have worldwide comes to a considerable degree from the quality and quantity of the research that we produce, and that signal is quite strongly carried by the people who we’re fortunate to train, and so by having an even stronger and even larger graduate program, we will be sending out into the world these marvelously trained, exciting, and thoughtful people who are carrying with them the Georgia Tech seal out into the scientific and mathematical worlds and carrying our story with them.

And so from my perspective, I think growing the graduate — growing and strengthening the graduate program is a key to our future success.

[Music]

Renay San Miguel: That was Paul Goldbart, dean of the Georgia Tech College of Sciences until the end of July. In August, Paul will take the position of dean of the College of Natural Sciences in the University of Texas at Austin. We wish him the best, and we thank him for his extraordinary work here in midtown Atlanta. I’m Renay San Miguel with the Georgia Tech College of Sciences.

[Music]

 

 

Astrobiology for the Family, brought to you by AbGradCon 2018

Is life in other planets possible?

Come to the Ferst Center in Georgia Tech and find out what young scientists have to say about the possibility of life in other planets.

Explore the wonders of life on our planet and outer space in a place where science and art meet. 

Marvel at the light- and computer-generated simulations of environments outside Earth, such as that of Mars! 

Interact with robots.

Talk to a real astronaut!

Join the organizers and participants of AbGradCon 2018 to have fun and learn about astrobiology

SCHEDULE

5:30-7.00 pm. Food and Exploration. Ferst Center Atrium.

Walk through demonstration stations to explore questions such as: How diverse is life on Earth? How might life look outside Earth? How do we search for life? What makes you wonder? Food for purchase will be available from food trucks.

7-7.30 pm. The Golden Record Performance, a Performance. Ferst Center Outdoor Amphitheater

This movement-based performance is inspired by the contents of The Golden Record, a 12-inch gold-plated copper disk containing sounds and images selected to portray the diversity of life and culture on Earth. The disk was carried by the space probes Voyager 1 and 2, when they blasted off for interstellar space in 1977. The Golden Record is a time capsule, intended to communicate a story of our world to extraterrestrials. The contents were selected by a NASA committee chaired by Carl Sagan

We will imagine through modern dance, aerial arts, live music, and projected images, how humanity might look through the eyes of the life forms that may one day encounter Voyager 1 or 2  and The Golden Record.

7.30-8 PM  In Space, Within the Stars: A Conversation with an Astronaut. Ferst Center Outdoor Ampitheater

Directions and Parking: http://arts.gatech.edu/directions-and-parking-0

 

 

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