SwRI scientists created a new model for impact-generated outgassing on the early Earth. A large impact creates a transient high temperature atmosphere. Within a thousand years, the atmosphere condenses, while deep-seated, impact-generated melt spreads across the surface. The model shows how pools of lava could release gases and create a greenhouse effect that warmed the planet.
In the first billion years of Earth’s history, the planet was bombarded by primordial asteroids, while a faint Sun provided much less heat. A Southwest Research Institute-led team posits that this tumultuous beginning may have ultimately fostered life on Earth, particularly in terms of sustaining liquid water.
“The early impacts caused temporary, localized destruction and hostile conditions for life. But at the same time, they had a long-term beneficial effect in stabilizing surface temperatures and delivering key elements for life as we know it,” said Dr. Simone Marchi, a senior research scientist at SwRI’s Planetary Science Directorate in ...
Source: [Southwest Research Institute]June 23, 2016 / Written by: Southwest Research Institute
A bacterial colony showing individual cells undergoing transposable element events, resulting in blue fluorescence. Images are shown at (a) t = 0, (b) t = 40 min, and (c) t = 60 min, with arrows indicating newly occurring events in each image. Image courtesy of T.E. Kuhlman, University of Illinois at Urbana-Champaign, reproduced with permission from Proceedings of the National Academy of Sciences USA.
“Jumping genes” are ubiquitous. Every domain of life hosts these sequences of DNA that can “jump” from one position to another along a chromosome; in fact, nearly half the human genome is made up of jumping genes. Depending on their specific excision and insertion points, jumping genes can interrupt or trigger gene expression, driving genetic mutation and contributing to cell diversification. Since their discovery in the 1940s, researchers have been able to study the behavior of these jumping genes, generally known as transposons or transposable elements (TE), primarily through indirect methods that infer individual activity from bulk results. However, such ...June 20, 2016 / Written by: Siv Schwink
Propylene oxide was detected, primarily with the NSF's Green Bank Telescope, near the center of our Galaxy in Sagittarius (Sgr) B2, a massive star-forming region. Credit: B. Saxton, NRAO/AUI/NSF from data provided by N.E. Kassim, Naval Research Laboratory
A team of scientists using highly sensitive radio telescopes have discovered the first complex organic chiral molecule in interstellar space. The molecule, propylene oxide (CH3CHOCH2), was found near the center of our Galaxy in an enormous star-forming cloud of dust and gas known as Sagittarius B2 (Sgr B2).
The research was undertaken primarily with the National Science Foundation’s Green Bank Telescope (GBT) in West Virginia as part of the Prebiotic Interstellar Molecular Survey. Additional supporting observations were taken with the Parkes radio telescope in Australia.
“This is the first molecule detected in interstellar space that has the ...
Source: [National Radio Astronomy Observatory]June 17, 2016 / Written by: National Radio Astronomy Observatory
The NASA Postdoctoral Program (NPP) offers U.S. and international scientists the opportunity to conduct important research while contributing to NASA’s scientific goals. Applications are now being accepted for postdoctoral fellows to engage in research with NASA’s Nexus for Exoplanet System Science (NExSS) advisors.
NExSS is a NASA research coordination network dedicated to the study of planetary habitability. The goals of NExSS are to investigate the diversity of exoplanets and to learn how their history, geology, and climate interact to create the conditions for life (https://nexss.info/). NExSS investigators also strive to put planets into an architectural ...
The pre-workshop online activities for the NExSS Exoplanet Biosignatures Workshop Without Walls will commence on June 13! We are pleased to let you know that 3 pairs of meetings will be timed to engage participants across the globe.
These pre-workshop activities will be community work sessions to review the State of the Science of remotely detectable biosignatures. The results will be summarized at the 3-day in-person workshop in July, where they will facilitate discussions for Advancing the Science and Technology for exoplanet biosignatures.
State of the Science Review
The length of each meeting will be 75 minutes.
Meeting 1: Topic ...
This artist's conception symbolically represents complex organic molecules, known as polycyclic aromatic hydrocarbons, seen in the early universe. These large molecules, comprised of carbon and hydrogen, are among the building blocks of life.
The molecules shown, called quinones, are potentially significant for the “origin of life” or the habitability of planets.
One of the lava flows analyzed in the study, from the shore of Australia’s Beasley River. Gas bubbles that formed as the lava cooled, 2.7 billion years ago, have since filled with calcite and other minerals. The bubbles now look like white spots. Researchers compared bubble sizes from the top and bottom of the lava flows to measure the ancient air pressure.
The layers on this 2.7 billion-year-old rock, a stromatolite from Western Australia, show evidence of single-celled, photosynthetic life on the shore of a large lake. The new result suggests that this microbial life thrived despite a thin atmosphere.
Source: [University of Washington]June 07, 2016 / Written by: Hannah Hickey
Mahoney Lake in British Columbia.
Metagenomic sequencing has provided new information about understudied populations of microorganisms that inhabit Mahoney Lake in British Columbia at depths where light does not reach. Mahoney Lake is an extreme meromictic system, meaning that the lake contains layers of water that do not mix. There is a great deal of information concerning microorganisms that live in sunlit portions of Mahoney Lake, and similar anoxic systems that contain high levels of sulfate and sulfide in the water column. However, less is known about communities living at depths below the photic zone.
The new study provides insight into the the types of ...
Source: [Frontiers in Microbiology]June 02, 2016 / Written by: Aaron Gronstal
Early Career Seminar: Chemical Gardens, Chimneys, and Fuel Cells: Simulating Prebiotic Chemistry in Hydrothermal Vents on Ocean Worlds
On Wednesday, June 1, 2016 at 11AM PDT, Laura Barge, NASA Jet Propulsion Laboratory, will be presenting the next early career seminar, Early Career Seminar: Chemical Gardens, Chimneys, and Fuel Cells: Simulating Prebiotic Chemistry in Hydrothermal Vents on Ocean Worlds.
Abstract: Planetary water-rock interfaces generate energy in the form of redox, pH, and thermal gradients, particularly in hydrothermal systems where the reducing, heated vent fluid feeds back into the more oxidizing ocean. Alkaline vents produced by serpentinization have been proposed as a possible location for the emergence of life on the early Earth due to various factors, including the mineral ...May 31, 2016 / Written by: Julie Fletcher
Lead author, Changyi Zhang, collecting samples in September 2014 at a hot spring in Yellowstone National Park.
Scientists from Carl R. Woese Institute for Genomic Biology have identified a new genetic marker (the apt gene) in a species of archaea named Sulfolobus islandicus. S. islandicus is a hyperthermophilic member of the phylum Crenarchaeota, and can be found in environments like volcanic springs with temperatures up to 91°C. Currently, S. islandicus is rapidly developing as a model for studying archaeal biology as well as linking novel biology to evolutionary ecology using functional population genomics.
Previously, only one similar genetic marker (the pyrEF gene) was known for Sulfolobus species. However, the majority of Sulfolobus mutants that have been ...
Source: [Applied and Environmental Microbiology]May 26, 2016 / Written by: Aaron Gronstal
Scanning electron micrographs of anaerobic Fe(II)-oxidizing cultures. From: Schadler et al. (2009) Formation of Cell-Iron-Mineral Aggregates by Phototrophic and Nitrate-Reducing Anaerobic Fe(II)-Oxidizing Bacteria, Geomicrobiology Journal.
A new study provides insight into a well-recognized chemolithotrophic pathway that can be used by microorganisms inhabiting anoxic sediments. Researchers used an enrichment culture of chemolithoautotrophic organisms from freshwater sediments (dubbed Culture KS) as a model system to study the pathway: nitrate-dependent ferrous iron [Fe(II)] oxidation (NDFO).
Previous efforts to isolate the organism responsible for the oxidation of iron [Fe(II)] in Culture KS had proven unsuccessful. In the new study, researchers used metagenomic analysis to better understand the roles of different bacteria in Culture KS. Using this method, they were able to identify the primary Fe(II)-oxidizer ...
Source: [Applied Environmental Microbiology]
The colored rings signify the different sectors where geoscientists work. The wedges, in turn, represent the fields where geoscientists are employed and include different examples of occupations. Where the wedges intersect with the rings indicates that those fields are included in those sectors. Image credit: Illustrator: Kathleen Cantner. Content: Heather Houlton & Abigail Seadler
The American Geosciences Institute (AGI) developed an infographic as a part of their Preparing Our Workforce (POW) Initiative to help students entering the workforce redefine what it means to have a career in geoscience. Having a successful geoscience career is not solely about mastering the technical fields of study. Students must seamlessly integrate their interests and competencies to build a professional portfolio that bolsters their career. Recognizing the importance of emphasizing the transferability of skills across different fields is imperative to students’ employability as geoscientists.
Source: [American Geosciences Institute ]May 18, 2016 / Written by: Julie Fletcher
A new study explores how properties of organization and cognition in the human brain could be universal. Researchers focused on semantics, or ‘meaning expressed through language,’ and developed an empirical measure of how semantics might reflect cultural, historical, and environmental backgrounds. The results highlight a universal structure underlying the sampled vocabulary across different language groups and largely independent of geography or environment.
Schematic of a bipartite semantic network constructed through translation (first layer to second layer) and back-translation (second layer to third layer) for MOON and SUN in two American languages: Coast Tsimshian (red) and Lakhota (blue).
Source: [PNAS]May 16, 2016 / Written by: Aaron Gronstal
In situ macro and mesostructure of Barstow Formation tufa. Image credit: Ibarra and Corsetti
The processes that govern the formation of stromatolites—structures that may represent macroscopic manifestation of microbial processes and a clear target for astrobiological investigation—occur at various scales (local versus regional), yet determining their relative importance remains a challenge, particularly for ancient deposits and/or if similar deposits are discovered elsewhere in the Solar System.
A new paper builds upon the traditional multiscale level approach of investigation (micro-, meso-, macro-, mega-) by including a lateral comparative investigational component of fine- to large-scale features to determine the relative significance of local and/or nonlocal controls on stromatolite morphology, and in the ...
Source: [Astrobiology]May 11, 2016 / Written by: Julie Fletcher
Our sun has a temperature of about 5800K. For stars cooler than our sun (M dwarfs at 3000-4000K) the habitable zone is closer in. For hotter stars (A dwarfs at 10,000K) the region is much farther out.
Researchers have provided new estimates for the inner edge of the habitable zone for synchronously rotating terrestrial planets around late-K and M-dwarf stars. Using a 3-D Earth-analog global climate model (GCM), the team has shed new light on the relationship between the rotational rates of planets and habitability around these types of stars. The results indicate that rotation rates for planets at the inner edge of the habitable zone become faster and that the inner edge is farther away from the host star than indicated in previous GCM studies.
The paper, “The inner edge of the habitable zone for synchronously ...
Source: [Earth and Planetary Astrophysics]May 09, 2016 / Written by: Aaron Gronstal
- March 30 - Application Deadline: Europlanet 2020 Infrastructures
- March 31 - Early Bird Registration Deadline for Robotic Telescopes Student Research and Education Conference
- March 31 - Abstract Submission Deadline for Small Satellites for Space Research (COSPAR 2017)
- March 31 - Travel Grant Application Deadline for Small Satellites for Space Research (COSPAR 2017)
- March 31 - Abstract Submission Deadline for Kepler & K2 Science Conference IV: Legacy & Scion
- March 31 - Application Deadline: NASA Space Technology Mission Directorate Early Career Faculty (ECF)
- March 31 - Application Deadline: ROSES 2016 Fellowships for Early Career Researchers
- April 1 - Abstract Submission Deadline for The 4th International Conference of Geobiology — Rocks, life and climate
- April 1 - Deadline for Merit and Need-Based Student and Early-Career Grants for Goldschmidt 2017
- April 1 - Abstract Submission Deadline for Goldschmidt 2017
- April 1 - Application Deadline: NASA Astrobiology Early Career Collaboration Award
- April 3 - Financial Assistance Deadline for NASA's 29th Annual Planetary Science Summer Seminar
- April 3 - Application Deadline for NASA's 29th Annual Planetary Science Summer Seminar
- April 3 - Abstract Submission Deadline for Robotic Telescopes Student Research and Education Conference
- April 4 - Indication of Interest Deadline for The Fifth International Planetary Dunes Workshop: From the Bottom of the Oceans to the Outer Limits of the Solar System
- April 4 - Registration Deadline for Radio Exploration of Planetary Habitability
- April 6 - Abstract Submission Deadline for Molecules in space: Linking the interstellar medium to (exo)planets
- April 11 - Abstract Submission Deadline for The XVIIIth International Conference on the Origin of Life
- NAI 2014 Annual Science Report