Dear Astrobiology, Origins, and Space Enthusiasts,
The ExplOrigins early career group invites you to join the 2021 Exploration and Origins Colloquium! This virtual colloquium will have events spanning two days:
Wednesday, February 17th: Poster Session
Thursday, February 18th: Research talks and Mars 2020 Perserverance Landing viewing
Our aim is to highlight work involving space exploration; biological, geological, and astronomical origins; and astrobiology of any sub-field at Georgia Tech and beyond.
Through this colloquium, we hope to:
forge relationships between diverse individuals of various fields, experience levels, and backgrounds
expand our internal awareness of local work an dinnovations
encourage collaboration and interdisciplinary understanding
provide a professional growth opportunity for early career individuals including undergraduates, graduates, and post-docs
For registration and abstract submission, complete the form linked below by the end of the day on January 21st (see update below). Announcement of selected speakers and poster presentations will be made on January 25th.
Update: The abstract deadline has been extended to January 29th! Get those abstracts in!
A selection of permitted presenter titles and abstracts have been published below.
Plenary Speakers
Dr. Christopher E. Carr
The synthesis of complex organic molecules, including the building blocks of life as we know it, occurs in stellar nebulas, in reducing planetary atmospheres, and through aqueous reaction networks. To the extent that this chemistry is universal, life elsewhere may also utilize amino acids, and nucleic acids or related informational polymers (IPs) for information storage and heredity.
Earth and Mars have exchanged an estimated billion tons of rock due to large meteorite impacts. If life exists on Mars, it could be related to us. Such an assumption is unlikely to hold for any life within Saturn’s moon Enceladus, or at Jupiter’s moon Europa. Here we describe progress towards life detection beyond Earth via single molecule sequencing of nucleic acids: a Search for Extra-Terrestrial Genomes (SETG). We also describe preliminary work to develop the Electronic Life-detection Instrument for Enceladus/Europa (ELIE), which would utilize nanogaps as a solid-state single molecule detector that is agnostic to the precise target chemical identity, extending detection capabilities from life as we know it to life as we don’t know it.
Dr. Mariel Borowitz
The field of astrobiology, with roots more than 100 years old, evolved quickly after the establishment of the National Aeronautics and Space Administration (NASA). This talk explores how the evolution of the field was influenced not only by important developments in science and technology, but also by political and policy issues and decisions. It traces the development of the field over the last sixty years and ends with some discussion of new directions going forward.
Presentations
Dr. Micah Schiable — Chemistry and Biochemistry
The distribution of material throughout our Solar System can place strong constraints on the possible dynamical and thermal histories of small bodies. Only by obtaining a measurement of the large-scale compositional distribution in various regions of the Solar System can questions regarding the origins and history of many small bodies begin to be addressed. Additionally, having a means to rapidly characterize the elemental compositions of bodies could help identify valuable resources for exploration and in situ resource utilization purposes.
The composition of bodies can only be loosely constrained using typical reflected light spectroscopy techniques. Although sample return is the best means of determine details of composition and formation conditions for bodies, it is costly, risky, and limited to a small number of sampling locations. A robust and sensitive technique for obtaining elemental composition of surfaces in high vacuum environments is the collection and analysis of secondary ions ejected due to solar wind and magnetosphere ion sputtering and meteorite impacts. First proposed for space based compositional analysis over 30 years ago [Managadze and Sagdeev, 1988; Johnson and Baragiola, 1991], this technique is commonly known in the laboratory as SIMS and can achieve excellent signal to noise ratios due to low ion backgrounds and high detection sensitivities achievable. Additionally, SIMS measurements at small bodies can help resolve whether these bodies harbor any potentially valuable resources for future exploration missions and how the composition of rocky asteroids varies throughout the Solar System.
Kelvin Smith — Chemical and Biomolecular Engineering
My research focuses on the investigation of the relevant kinetic mechanisms of chiral depsipeptide polymerization and degradation. Once these depsipeptide mechanisms are identified, you can predict behavior of similar peptides used to create biopolymers for pharmaceutical purposes such as drug delivery and tissue engineering. The model provides helpful predictions for future synthesis of other depsipeptides, and it consists of a complex Kinetic Monte Carlo (KMC) framework that simulates growth and degradation of chiral depsipeptides. To use the framework, rate constants of relevant mechanisms must be known a priori through either experimental data or a literary search. To investigate the kinetic mechanisms of ester reactions in depsipeptides, high performance liquid chromatography (HPLC) data of two test molecules are collected and quantified at different pH values and temperatures: multiple oligomers of an HO-dipeptide called glycolic acid alanine (gA) and a methylated molecule of the gA dimer called propionic acid alanine glycolic acid alanine ((PA)AgA). I model and simulate the evolution and degradation of gA using MATLAB to extract rate constants. These degradation rate constants come from a novel model structure that describes two hypothesized mechanisms: scission and backbiting. I perform statistical procedures to determine how good the model fits are to the data, how likely one mechanism describes a model over another, and how confident we can be in the predicted values. Preliminary results show that both scission and backbiting rate constants of the gA oligomers and (PA)AgA follow an Arrhenius relationship and that backbiting is a dominant degradation mechanism at basic pH values in gA oligomers. When the rate constants were plotted against pH, similar behavior can be found in the literature.
Petar Penev — Biological Sciences
The ribosome’s common core connects all life back to a common ancestor and serves as a window to relationships among organisms. In eukaryotes, the common core contains expansion segments (ES’s) that vastly increase ribosomal RNA size. Supersized ES’s have not been observed previously in Bacteria or Archaea, and the origin of eukaryotic ES’s remains enigmatic. We discovered that the large subunit rRNA of Lokiarchaeota, the closest modern cell lineage to the last common ancestor of Archaea and Eukarya, bridges the gap in size between prokaryotic and eukaryotic rRNA. The long large subunit rRNA in Lokiarchaeota is largely due to the presence of two eukaryotic-like, supersized ES’s, ES9 and ES39, which are transcribed in situ. We applied computational models, covariation analysis, and chemical footprinting experiments to study the structure and evolution of Lokiarchaeota ES9 and ES39. We also defined the eukaryotic ES39 fold for comparison. We found that Lokiarchaeota and eukaryotic ES’s are structurally distinct: Lokiarchaeota ES39 has more and longer helices than the eukaryotic ES39 fold. Despite their structural differences, we found that Lokiarchaeota and eukaryotic ES’s originated from a common ancestor that was “primed” for evolution of larger and more complex rRNAs than those found in Bacteria and other archaea.
Dr. Anthony Burnetti
Phototrophy – the ability of a cell to capture light energy for metabolism – is responsible for the vast majority of biomass production and metabolic flux on Earth, and its origin represents an extremely important evolutionary transition. This capability has evolved independently exactly twice in Earth’s history, via chlorophototrophic and retinalophototrophic machinery. Close examination of the properties of these metabolic pathways reveals them to be remarkably complementary in their chemical makeup and ecological roles, suggesting that their properties are the result of ancient ecological interactions between incumbent and novel phototrophs filling initially vacant ecological niches rather than being the random results of rare, difficult innovations. Each origin of phototrophy has filled a particular niche in the tradeoff between efficiency per unit light and efficiency per unit protein infrastructure, and has suppressed the evolution of novel machineries like themselves while failing to suppress each other due to their fundamental architectural differences.
As a “dual evolutionary singularity”, phototrophy can also be used as a touchstone to understand the dynamics of major evolutionary innovations and transitions in the history of life on Earth. Many innovations, such as the singular origin of eukaryotes or the origin of life itself, occurred exactly once and transformed the planet. Others, like the evolution of multicellularity, have occurred many times. This could be due to some innovations being intrinsically rare or difficult, or evolutionary singularities could be singular as a result of ecological interactions by first-movers suppressing innovation by other lineages. The example of phototrophy suggests that many of these singularities could be simpler to evolve than they seem, and could be common in other biospheres.
Aaron Pital
The pace of publication in the sciences has long since outstripped human ability to read and synthesize information. While interdisciplinary work can mitigate some of this burden, there remain fundamental questions about whether attentional blindness and the opportunity cost of reaching beyond the comfort of one’s expertise hold back innovation in speculative fields such as the origins of life. We present a brief model of associative information in scientific publication and propose tools derived from information theory, natural language processing, and data science to search for physical and chemical contexts embedded in literature from fields as diverse and non-traditional as soil science and drug design. The goals of these efforts are 1) to identify physical and chemical information of interest to origins of life researchers which would otherwise be unlikely to rise to the community’s attention and 2) to define rules for correlated information generally to improve literature cataloging, referencing and retrieval.
On behalf of Georgia Tech Astrobiology and the ExplOrigins early career group, we invite you to join us for the 2020 Exploration and Origins Colloquium. Please click HERE to register or submit a poster abstract. The colloquium kicks off with a poster session on Monday January 27th, and continues with a day of plenary lectures, contributed talks, and a breakout networking session on Tuesday, January 28th. If you have any questions regarding the abstract submission process, please email the conference organizers at info.gt.astrob.colloq@gmail.com. Thank you for your consideration.
Schedule:
January 27th, 2020, MoSE 1st and 2nd Floor Atrium 5:00 PM – 7:00 PM: PosterSession
January 28th, 2020, IBB Suddath Seminar Room 8:00 AM – 8:45 AM: Coffee and Poster Viewing 8:45 AM – 8:50 AM: Welcome from College of Sciences Dean Susan Lozier 8:50 AM – 9:00 AM: Exploration and Origins Colloquium Welcome 9:00 AM – 10:00 AM: Plenary 1 Mariel Borowitz: Astrobiology: Science, Technology, Policy, and Politics 10:00 AM – 10:15 AM: Coffee Break 10:20 AM – 12:00 PM: Morning Session (Introduction: Tyler Roche)
Kynan Hughson: Possible pingo analogs may populate Ceres
Micah Schaible: In situ characterization of elemental compositions for small bodies throughout the Solar System
Bradley Burcar: The impact of CO2 and cyanide in prebiotic environments on mineral formation and urea-based phosphorylation reactions
Kelvin Smith: Mechanistic Investigation of Depsipeptides in the Early Earth Through Kinetic Monte Carlo Framework
Petar Penev: Eukaryotic-like ribosomal RNA region in Lokiarchaeota
12:00 PM – 1:00 PM: Lunch (MoSE 1st and 2nd floor atrium) 1:00 PM – 2:00 PM: Plenary 2 — Christopher Carr: A Direct Search for Life As We Know It and Don’t Know It 2:00 PM – 3:00 PM: Afternoon Session 1 (Introduction: Taylor Plattner)
Nadia Szeinbaum: Synthetic microbial consortia to explore cooperation on early Earth
Anthony Burnetti:The dual origins of phototrophy and major evolutionary transitions.
Devon Cole:Stability of atmospheric oxygen levels and ocean ventilation
Philip Szot: Vertical Entry Robot for Navigating Europa (VERNE) Mission and System Design
Loren Dean Williams: Polymers versus Metabolism
Adriana Lozoya Colinas: DNA replication facilitated by a prebiotic solvent
Aaron Pital:Semantic mining of chemical origins from non-chemistry disciplines
5:00-6:00: Networking breakout session
Plenary Speakers
Mariel Borowitz
Assistant Professor, Sam Nunn School of International Affairs, Georgia Institute of Technology
Astrobiology: Science, Technology, Policy, and Politics
Mariel Borowitz is an Assistant Professor in the Sam Nunn School of International Affairs at Georgia Tech. Her research deals with international space policy issues, including international cooperation in Earth observing satellites and satellite data sharing policies. She also focuses on strategy and developments in space security and space situational awareness. Dr. Borowitz earned a PhD in Public Policy at the University of Maryland and a Masters degree in International Science and Technology Policy from the George Washington University. She has a Bachelor of Science degree in Aerospace Engineering from the Massachusetts Institute of Technology. Dr. Borowitz completed a detail as a policy analyst for the Science Mission Directorate at NASA Headquarters in Washington, DC from 2016 to 2018. Her book, “Open Space: The Global Effort for Open Access to Environmental Satellite Data,” was published by MIT Press in 2017.
Christopher E. Carr
Research Scientist, MIT Research Fellow, MGH
A Direct Search for Life As We Know It and Don’t Know It
Christopher E. Carr is an engineer/scientist in Cambridge, Massachusetts, USA. He serves as the Science PI or PI for several life detection instrument and/or astrobiology projects. He is broadly interested in searching for and expanding the presence of life beyond Earth while enabling a sustainable human future. He is currently a Research Scientist at MIT in the Department of Earth, Atmospheric and Planetary Sciences, and a Research Fellow at the Massachusetts General Hospital in the Department of Molecular Biology. He also serves as a Scott M. Johnson Fellow in the U.S. Japan Leadership Program. This summer he will join the Georgia Tech faculty as an Assistant Professor in the Daniel Guggenheim School of Aerospace Engineering, with a secondary appointment in the School of Earth and Atmospheric Sciences.
2020 Exploration and Origins Colloquium:
This interdisciplinary colloquium will highlight space exploration science and origins research going on at the Georgia Institute of Technology, as well as neighboring universities. The goals of the colloquium are to forge relationships between diverse individuals, encourage collaboration and interdisciplinary understanding, and kick-start future fundable projects requiring the skills and expertise of multi-lab teams.
As previously, the colloquium will be roughly split into two sections: Exploration and Origins. While outlines of the two sections are provided below, the scope of abstracts considered will be broad. Past submissions have been from the departments of Earth and Atmospheric Sciences, Chemistry & Biochemistry, Biology, Physics, Mathematics, and multiple engineering departments. We emphasize that all interested parties are welcome regardless of discipline or affiliation.
Exploration: For the Exploration session, we are particularly interested in submissions that deal with any and all aspects of reaching beyond to explore the nature of diverse environments. Examples include space technology development, spacecraft mission design, planetary science modeling, biological or ecological fieldwork and direct observations of extrasolar systems; in short, exploring what is ‘out there’, wherever ‘there’ is.
Origins: Submissions for the Origins session are encouraged to include some aspect of reaching back to understand the nature of the world today. Examples include cosmology and the origins of life itself, the emergence of multicellularity, the evolution of minerals, complex chemistry, atmospheres, and biological molecules or processes, and the formation of planetary systems; basically, how did we get here?
Abstract Pages:
The pages linked here contain a selection of abstracts from our submitting attendees.
The poster boards we will be using have dimensions 36″ by 42″. You may choose to set your poster up in a portrait or landscape orientation.
The organizing committee:
Aaron Pital (Graduate Student, Chemistry and Biochemistry) Chase Chivers (Graduate Student, Earth and Atmospheric Sciences) Christina Buffo (Graduate Student, Chemistry and Biochemistry) Tyler Roche (Graduate Student, Chemistry and Biochemistry) Rebecca Guth-Metzler (Graduate Student, Chemistry and Biochemistry) Taylor Plattner (Graduate Student, Earth and Atmospheric Sciences) Micah Schaible (Postdoctoral Fellow, Chemistry and Biochemistry)
Funding and Support:
We are grateful for the funding and support provided by CSTAR, GT Conference Support, the School of Earth and Environmental Sciences, the School of Chemistry and Biochemistry, and Frank Rosenzweig (NAI, CAN-7)
“Ocean Worlds of the Outer Solar System” Public Lecture and reception Dr. Kevin Hand, NASA JPL Smithgall 117 Lecture Hall, 353 Ferst Drive NW, Atlanta, GA 30313, 6:30pm with reception to follow
Friday, March 29
8:15 AM – 9:00 AM: Coffee and Poster Setup
9:00 AM – 9:10 AM: Welcome notes
Topic: Planetary Science and Exploration
9:10 AM – 10:10 AM: Plenary 1: Paul Steffes, Georgia Institute of Technology, “Radio Science: From Uncovering Jupiter’s Formation to Searching for Intelligent Life in Our Galaxy”
10:10 AM – 10:30 AM: Zach Siebars, “Multi-functional Composites for Space Travel: Design Considerations Using Reduced Graphene Oxides as Additives in Polymers”
10:30 AM – 10:50 AM: Adrian Ildefonso, “Silicon-Germanium Platforms: an Enabling Technology for Next-Generation Space Systems”
10:50 AM – 11:00 AM: Coffee break
11:00 AM – 11:20 AM: William Jun, “Design of an Interplanetary Radionavigation System for Surface Geolocation”
11:20 AM – 11:40 AM: Justin Lawrence, “Developing Ocean World Exploration Strategies and Hardware Below Antarctic Ice Shelves”
11:40 AM – 12:00 PM: Billy Quarles, “Habitability of Exoplanets Around Sunlike Stars”
12:00 PM – 1:00 PM: Lunch, atrium of Krone Engineered Biosystems Building (EBB)
Topic: Life Origins and its Detection
1:00 PM – 2:00 PM: Plenary 2: Sara Walker, Arizona State University
2:00 PM – 2:20 PM: Aaron McKee, “Proto-oligopeptides at Mineral Interfaces: Interactions of Silica and an Expanded Prebiotic Peptide inventory”
2:20 PM – 2:40 PM: Moran Frenkel-Pinter, “Chemical Mutualism of Prebiotic Mixtures of Cationic Depsipeptides and RNA”
2:40 PM – 2:50 PM: Coffee break
2:50 PM – 3:10 PM: Jefferey Skolnick, “Studies on the Origin of Protein Chirality, Biochemical Function, and Strcture”
3:10 PM – 3:30 PM: David Fialho, “Plausible Prebiotic Formation and Supramolecular Assembly of Depsipeptide Nucleic Acid Oligomers”
3:30 PM – 3:50 PM: Nadia Szeinbaum, “A Synthetic Microbial Consortium to Explore Cooperation on Early Earth”
3:50 PM – 4:15 PM: Coffee break
4:15 PM – 7:00 PM: Poster session and Colloquium reception
Building on the success of the 2018 Astrobiology Colloquium, Georgia Tech Astrobiology and ExplOrigins groups are proud to announce the 2019 Exploration and Origins Colloquium, which will take place on March 28-29, 2019. This is the 2nd annual networking event under the theme of exploring the universe and origins of life.
This year the colloquium is split in two sections: the first section is focused on space exploration technology and planetary science, and the second is oriented toward the chemistry and biology of the origins and the search for life. The event will consist of presentations and talks by early career scientists, i.e. graduate and undergraduate students, and post-doctoral fellows, working in the exciting fields of space and planetary science, engineering and astrobiology across Georgia Tech campus and the greater Atlanta. There will also be plenary lectures given by distinguished members of the global astrobiology community. The objective of this interdisciplinary colloquium is to forge connections across the kinds of research at Georgia Tech straddling the boundaries between technology development and hypothesis testing in the search for life’s beginnings and to explore collaborative ideas among participants. Hence, senior researchers and faculty are also highly encouraged to attend.
Plenary Speakers:
Kevin Hand, NASA Jet Propulsion Laboratory
Dr. Kevin Peter Hand is a planetary scientist at NASA’s Jet Propulsion Laboratory in Pasadena, California. His research focuses on the origin, evolution, and distribution of life in the solar system with an emphasis on Jupiter’s moon, Europa. His work involves both theoretical and laboratory research on the physics and chemistry of icy moons in the outer solar system. Hand is the Director of the Ocean Worlds Lab at JPL. He served as co-chair for NASA’s Europa Lander Science Definition team and he is the Project Scientist for the Pre-Phase-A Europa Lander mission. From 2011 to 2016 he served as Deputy Chief Scientist for Solar System Exploration at JPL. He served as a member of the National Academies Committee on Astrobiology and Planetary Sciences. His work has brought him to the Dry Valleys of Antarctica, the sea ice near the North Pole, the depths of the Earth’s oceans, and to the glaciers of Kilimanjaro. Dr. Hand was a scientist onboard James Cameron’s 2012 dive to the bottom of the Mariana Trench, and he was part of a 2003 IMAX expedition to hydrothermal vents in the Atlantic and Pacific oceans. He has made nine dives to the bottom of the ocean. In 2011 he was selected as a National Geographic Explorer. Hand earned his PhD from Stanford University and bachelor’s degrees from Dartmouth College. He was born and raised in Manchester, Vermont.
Sara Walker, Arizona State University
Professor Walker is an astrobiologist and theoretical physicist at Arizona State University, the Deputy Director of the Beyond Center for Fundamental Concepts in Science, and the Associate Director of the ASU-Santa Fe Institute Center for Biosocial Complex Systems. She is also Co-founder of the astrobiology-themed social website SAGANet.org, and a member of the Board of Directors of Blue Marble Space. Her work centers on in the origin of life and how to find life on other worlds. She is most interested in whether or not there are ‘laws of life’ – related to how information structures the physical world – that could universally describe life here on Earth and on other planets. She is active in public engagement in science, with appearances at the World Science Festival and on “Through the Wormhole” and NPR’s Science Friday
Paul Steffes Georgia Institute of Technology
Professor Steffes performed his doctoral research at Stanford University where he concentrated on microwave radio occultation experiments using the Voyager and Mariner spacecraft, with specific interest in microwave absorption in planetary atmospheres. Then, in 1982, he joined the faculty of Georgia Tech and is currently a Professor of Electrical and Computer Engineering. His research focuses on microwave and millimeter-wave remote sensing and radio astronomy and has been sponsored by NASA, the NSF, the SETI Institute and by industry. He has been involved with numerous NASA missions, including Pioneer-Venus, Magellan, the Advanced Communications Technology Satellite (ACTS), the High Resolution Microwave Survey (HRMS), and Juno (Jupiter Polar Orbiter).
Keynote and oral presentations will be in the Children’s Health Care of Atlanta Seminar Room (EBB 1005), Krone Engineered Biosystems Building (EBB), 950 Atlantic Drive, NW, Atlanta. GA 30332.
The poster session and networking event will be in held the 1stand 2nd floor atria of the Molecular Science and Engineering Building (MoSE), 901 Atlantic Drive NW, Atlanta, GA 30318.
We are grateful for funding and support from The Georgia Tech Strategic Plan Action Group (SPAG), the School of Earth and Atmospheric Sciences (EAS), The NSF/NASA Center for Chemical Evolution (CCE), The School of Chemical and Biomolecular Engineering, and the School of Chemistry and Biochemistry.
Georgia Tech Astrobiology is proud to announce that the 2018 Astrobiology Colloquium will take place on March 30th, 2018. This is a new early career event for the Georgia Tech astrobiology community and will consist of presentations and talks by students (both graduate and undergraduate) and post-doctoral fellows working in astrobiology, space science, and engineering across the Georgia Tech campus and greater Atlanta. There will also be plenary lectures given by distinguished members of the global astrobiology community.Our theme, for what we hope is the inauguration of an annual event is: Exploring Life Origins and the Universe: A Networking Event. As such, in addition to our early career speakers, poster presentations, and our plenary lectures, there will be networking and innovation platform activities to forge connections and explore collaborative ideas among participants. Hence, senior researchers and faculty are highly encouraged to attend.
Registration for the 2018 Georgia Tech Astrobiology Colloquium is now closed as the event has reached capacity. However, an overflow space with a direct feed to the conference presentations is available in the Suddath Symposium Room located on the first floor of the Parker H. Petit Institute for Bioengineering and Bioscience Building (IBB). This room will have a view-only feed from the main colloquium in EBB and is open to the entire campus community. Space is limited and first come-first served.
For colloquium updates and notifications please join our mailing list by clicking here
(Please Note: This is an announcement e-mail list only for updates about the colloquium.)
For all other questions, please contact us
Plenary Speakers
Organizing Committee
Faculty Advisors
Martha Grover
Glenn Lightsey
Jennifer Glass
Exploring Life Origins and the Universe: Program
March 30, 2018
8:15-9:00: Coffee and Poster Setup
9:00-9:10: Welcome by Paul M. Goldbart, Dean of Georgia Tech College of Sciences
9:10-10:10: Plenary 1: Ada Yonath, Weizmann Institute, Israel What Was First, the Genetic Code or its Products?
10:10-10:30 Coffee Break and Posters 1
10:30-10:45: Burcar, B.; Lago, J.; Pasek, M.; Menor-Salvan, C.; Hud, N. Phosphorylation in Urea-Rich Eutectic Solvents
10:45-11:00: Taran, O. Iron Sulfide Minerals in Prebiotic Redox Chemistry
11:00-11:15: McKee, A. A Possible Path to Prebiotic Peptides Involving Mineral Substrates and Hydroxy Acid-mediated Amide Bond Formation
11:15-11:30: Fialho, D.; Clarke, K.; Moore, M.; Schuster, G.; Krishnamurthy, R.; Hud, N. Glycosylation of a Model Proto-RNA Nucleobase with non-Ribose Sugars: Implications for the Prebiotic Synthesis of Nucleosides
11:30-11:45: Solano, M.; frenkel-Pinter, M.; Grover, M.; Hud, N Selection and Assembly of Prebiotically Plausible Protopeptides
11:45-12:00: Bray, M.; Bowman, J; Petrov, A.; REddi, R. Iron: Primordial Cofactor for the Translation System
12:00-1:15: Lunch, atrium of the Integrated Biosciences Building (IBB)
1:15-2:15: Plenary 2: Niles Lehman, Portland State University Scrambling to Build the RNA World
2:15-2:35: Coffee Break and Posters 2
2:35-2:50: Márquez-Zacarías, P.; Ratcliff, W. C. How to Describe Exo-Evo? An Organismal Approach to Evolutionary Dynamics
2:50- 3:05: Chen, K.; Rosenzweig, R. F.; Herron, M. D. Genetic Basis Underlying De Novo Origins of Multicellularity in Response to Predation
3:05-3:20: Szeinbaum, N.; Henry, C.; Crowe, S. A.; Stewart, F. J.; DiChristina, T. J.; Reinhard, C. T.; Nunn, B. L.; Glass, J. B. Metaproteomics Reveals a Novel Betaproteobacterium with Roles in Metal and Nitrogen Cycling in the Deep Subsurface
3:20-3:35: Krafft, A.; Colvin, T.; Homar, K.; Lynch, K. L.; Greene, R. Fitzsimmons, R.; Zaharescu, G. D. The Embedded Scientist Program
3:35-3:50: Lourenco, N. E.; Williams, W. L.; Coen, C. t.; Frounchi, M.; Cressler, J. D. MicroNimbus: a Spaceborne mm-Wave Temperature Profilometer for the Earth’s Atmosphere
3:50-4:05: Duca, Z.; Cantrell, T.; Speller, N. C.; Stockton, A. M. Quantitative, Compositional Analysis of Trace Amino Acids in Europa: analogues with a modular μCE-LIF System
4:05-4:55: Transport to Evening Venue
4:55-5:45: Round Table Activities
5:45-6:15 Summary and Wrapup
6:00: Dinner, Ironmonger Brewing, Marietta, GA
7:00: Plenary 3: Shawn Domagal-Goldman, NASA Goddard Space Flight Center LUVOIR: An Astrobiology Mission to Targets Near and Far
