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Wednesday, January 31st, 2018

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    1:00p
    Reading and writing DNA

    Thanks to the invention of genome sequencing technology more than three decades ago, we can now read the genetic blueprint of virtually any organism. After the ability to read came the ability to edit — adding, subtracting, and eventually altering DNA wherever we saw fit. And yet, for George Church, a professor at Harvard Medical School, associate member of the Broad Institute, and founding core faculty and lead for synthetic biology at the Wyss Institute — who co-pioneered direct genome sequencing in 1984 — the ultimate goal is not just to read and edit, but also to write.

    What if you could engineer a cell resistant to all viruses, even the ones it hadn’t yet encountered? What if you could grow your own liver in a pig to replace the faulty one you were born with? What if you could grow an entire brain in a dish? In his lecture on Jan. 24 — which opened the Department of Biology’s Independent Activities Period (IAP) seminar series, Biology at Transformative Frontiers — Church promised all this and more.

    “We began by dividing the Biology IAP events into two tracks: one related to careers in academia and another equivalent track for industry,” says Jing-Ke Weng, assistant professor and IAP faculty coordinator for the department. “But then it became clear that George Church, Patrick Brown, and other speakers we hoped to invite blurred the boundaries between those two tracks. The Biology at Transformative Frontiers seminar series became about the interface of these trajectories, and how transferring technologies from lab bench to market is altering society as we know it.”

    The seminar series is a staple in the Department of Biology’s IAP program, but during the past several years it has been oriented more toward quantitative biology. Weng recalls these talks as being relegated to the academic sphere, and wanted to show students that the lines between academia, industry, and scientific communication are actually quite porous.

    “We chose George Church to kick off the series because he’s been in synthetic biology for a long time, and continues to have a successful academic career even while starting so many companies,” says Weng.

    Church’s genomic sequencing methods inspired the Human Genome Project in 1984 and resulted in the first commercial genome sequence (the bacterium Helicobacter pylori) 10 years later. He also serves as the director of the Personal Genome Project, the “Wikipedia” of open-access human genomic data. Beyond these ventures, he’s known for his work on barcoding, DNA assembly from chips, genome editing, and stem cell engineering.

    He’s also the same George Church who converted the book he co-authored with Ed Regis, "Regenesis: How Synthetic Biology Will Reinvent Nature and Ourselves," into a four-letter code based on the four DNA nucleotides (A, T, C, and G), subsisted on nutrient broth from a lab vendor for an entire year, and dreams of eventually resurrecting woolly mammoths. He’s being featured in an upcoming Netflix Original documentary, so when he arrived at the Stata Center to give his lecture last week he was trailed by a camera crew.

    According to Church, the transformative technologies that initially allowed us to read and edit DNA have grown exponentially in recent years with the invention of molecular multiplexing and CRISPR-Cas9 (think Moore’s Law but even more exaggerated). But there’s always room for improvement.

    “There’s been a little obsession with CRISPR-Cas9s and other CRISPRs,” said Church. “Everybody is saying how great it is, but it’s important to say what’s wrong with it as well, because that tells us where we’re going next and how to improve on it.”

    He outlined several of his own collaborations, including those aimed at devising more precise methods of genome editing, one resulting in 321 changes to the Escherichia coli genome — the largest change in any genome yet — rendering the bacterium resistant to all viruses, even those it had not yet come into contact with. The next step? Making similarly widespread changes in plants, animals, and eventually perhaps even human tissue. In fact, Church and his team have set their sights on combatting the global transplantation crisis with humanlike organs grown in animals.

    “Since the dawn of transplantation as a medical practice, we’ve had to use either identical twins or rare matches that are very compatible immunologically, because we couldn’t engineer the donor or the recipient,” said Church.

    Since it’s clearly unethical to engineer human donors, Church reasoned, why not engineer animals with compatible organs instead? Pigs, to be exact, since most of their organs are comparable in size and function to our own.

    “This is an old dream; I didn’t originate it,” said Church. “It started about 20 years ago, and the pioneers of this field worked on it for a while, but dropped it largely because the number of changes to the genome were daunting, and there was a concern that the viruses all pigs make — retroviruses — would be released and infect the immunocompromised organ recipient.”

    Church and his team successfully disrupted 62 of these retroviruses in pig cells back in 2015, and in 2017 they used these cells to generate living, healthy pigs. Today, the pigs are thriving and rearing piglets of their own. Church is also considering the prospect of growing augmented organs in pigs for human transplantation, perhaps designing pathogen-, cancer-, and age-resistant organs suitable for cryopreservation.

    “Hopefully we’ll be doing nonhuman primate trials within a couple of years, and then almost immediately after that human trials,” he said.

    Another possibility, rather than cultivating organs in animals for transplant, is to generate them in a dish. A subset of Church’s team is working on growing from scratch what is arguably the most complicated organ of all, the brain.

    This requires differentiating multiple types of cells in the same dish so they can interact with each other to form the complex systems of communication characteristic of the human brain.

    Early attempts at fashioning brain organoids often lacked capillaries to distribute oxygen and nutrients (roughly one capillary for each of the 86 billion neurons in the human brain). However, thanks to their new human transcription factor library, Church and colleagues have begun to generate the cell types necessary to create such capillaries, plus the scaffolding needed to promote the three-dimensional organization of these and additional brain structures. Church and his team have not only successfully integrated the structures with one another, but have also created an algorithm that spits out the list of molecular ingredients required to generate each cell type.

    Church noted these de novo organoids are extremely useful in determining which genetic variants are responsible for certain diseases. For instance, you could sequence a patient’s genome and then create an entire organoid with the mutation in question to test whether it was the root cause of the condition.

    “I’m still stunned by the breadth of projects and approaches that he’s running simultaneously,” says Emma Kowal, a second-year graduate student, member of Weng’s planning committee, and a former researcher in Church’s lab. “The seminar series is called Biology at Transformative Frontiers, and George is very much a visionary, so we thought it would be a great way to start things off.”

    The four-part series also features Melissa Moore, chief scientific officer of the Moderna Therapeutics mRNA Research Platform, Jay Bradner, president of the Novartis Institutes for BioMedical Research, and Patrick Brown, CEO and founder of Impossible Foods. 

    7:00p
    Modeling the universe

    A supercomputer simulation of the universe has produced new insights into how black holes influence the distribution of dark matter, how heavy elements are produced and distributed throughout the cosmos, and where magnetic fields originate. 

    Astrophysicists from MIT, Harvard University, the Heidelberg Institute for Theoretical Studies, the Max-Planck Institutes for Astrophysics and for Astronomy, and the Center for Computational Astrophysics gained new insights into the formation and evolution of galaxies by developing and programming a new simulation model for the universe — “Illustris - The Next Generation” or IllustrisTNG

    Mark Vogelsberger, an assistant professor of physics at MIT and the MIT Kavli Institute for Astrophysics and Space Research, has been working to develop, test, and analyze the new IllustrisTNG simulations. Along with postdocs Federico Marinacci and Paul Torrey, Vogelsberger has been using IllustrisTNG to study the observable signatures from large-scale magnetic fields that pervade the universe. 

    Vogelsberger used the IllustrisTNG model to show that the turbulent motions of hot, dilute gases drive small-scale magnetic dynamos that can exponentially amplify the magnetic fields in the cores of galaxies — and that the model accurately predicts the observed strength of these magnetic fields.

    “The high resolution of IllustrisTNG combined with its sophisticated galaxy formation model allowed us to explore these questions of magnetic fields in more detail than with any previous cosmological simulation," says Vogelsberger, an author on the three papers reporting the new work, published today in the Monthly Notices of the Royal Astronomical Society.

    Modeling a (more) realistic universe 

    The IllustrisTNG project is a successor model to the original Illustris simulation developed by this same research team but has been updated to include some of the physical processes that play crucial roles in the formation and evolution of galaxies. 

    Like Illustris, the project models a cube-shaped piece of the universe. This time, the project followed the formation of millions of galaxies in a representative region of the universe with nearly 1 billion light years on a side (up from 350 million light years on a side just four years ago). lllustrisTNG is the largest hydrodynamic simulation project to date for the emergence of cosmic structures, says Volker Springel, principal investigator of IllustrisTNG and a researcher at Heidelberg Institute for Theoretical Studies, Heidelberg University, and the Max-Planck Institute for Astrophysics.

    The cosmic web of gas and stars predicted by IllustrisTNG produces galaxies quite similar to the shape and size of real galaxies. For the first time, hydrodynamical simulations could directly compute the detailed clustering pattern of galaxies in space. In comparison with observational data — including the newest large galaxy surveys such as the Sloan Digital Sky Survey — IllustrisTNG demonstrates a high degree of realism, says Springel. 

    In addition, the simulations predict how the cosmic web changes over time, in particular in relation to the underlying backbone of the dark matter cosmos. “It is particularly fascinating that we can accurately predict the influence of supermassive black holes on the distribution of matter out to large scales,” says Springel. “This is crucial for reliably interpreting forthcoming cosmological measurements.” 

    Astrophysics via code and supercomputers 

    For the project, the researchers developed a particularly powerful version of their highly parallel moving-mesh code AREPO and used it on the "Hazel-Hen" machine at the Supercomputing Center in Stuttgart, Germany's fastest mainframe computer.

    To compute one of the two main simulation runs, more than 24,000 processors were used over the course of more than two months.

    “The new simulations produced more than 500 terabytes of simulation data,” says Springel. “Analyzing this huge mountain of data will keep us busy for years to come, and it promises many exciting new insights into different astrophysical processes." 

    Supermassive black holes squelch star formation

    In another study, Dylan Nelson, researcher at the Max-Planck Institute for Astrophysics, was able to demonstrate the important impact of black holes on galaxies.

    Star-forming galaxies shine brightly in the blue light of their young stars until a sudden evolutionary shift quenches the star formation, such that the galaxy becomes dominated by old, red stars, and joins a graveyard full of old and dead galaxies. 

    “The only physical entity capable of extinguishing the star formation in our large elliptical galaxies are the supermassive black holes at their centers,” explains Nelson. “The ultrafast outflows of these gravity traps reach velocities up to 10 percent of the speed of light and affect giant stellar systems that are billions of times larger than the comparably small black hole itself.“

    New findings for galaxy structure

    IllustrisTNG also improves researchers' understanding of the hierarchical structure formation of galaxies. Theorists argue that small galaxies should form first, and then merge into ever-larger objects, driven by the relentless pull of gravity. The numerous galaxy collisions literally tear some galaxies apart and scatter their stars onto wide orbits around the newly created large galaxies, which should give them a faint background glow of stellar light.

    These predicted pale stellar halos are very difficult to observe due to their low surface brightness, but IllustrisTNG was able to simulate exactly what astronomers should be looking for. 

    “Our predictions can now be systematically checked by observers,” says Annalisa Pillepich, a researcher at Max-Planck Institute for Astronomy, who led a further Illustris-TNG study. “This yields a critical test for the theoretical model of hierarchical galaxy formation.” 

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