NAI’s team at RPI has been hosting the ExxonMobil Bernard Harris Summer Science Camp for the last several years. Here is a link to the NPR show To the Best of Our Knowledge featuring a digest of last year’s camp in which teams of middle-school students designed missions to search for life on Mars. It includes interviews with students from the winning team and their parents, prefaced by a superb introduction by Dr. Wayne Roberge. The camp is a vital component of the E/PO program of the NY Center for Astrobiology, and this show does an excellent ...February 18, 2014 / Posted by: Daniella Scalice
Photo of RAD flight model in the lab (left) and an artist's impression of the Curiosity rover on Mars. Credit: NASA / JPL
Scientists have published the first thorough analysis of radiation readings from the surface of another planet. Using its Radiation Assessment Detector (RAD), NASA’s Curiosity rover measured radiation exposure during its journey to Mars, and the amount of radiation present at the planet’s surface.
Radiation and its variations impact not only the planning of human and robotic missions, but also the search for extraterrestrial life. Without substantial atmospheric protection, powerful particles entering the air can penetrate ...
A deep-sea hydrothermal vent. Credit: Photo courtesy of Chris Germen, WHOI/NSF, NASA/ROV Jason 2012, at Woods Hole Oceanographic Institution
A new study reports that a protein used in plant photosynthesis could have originated 2.5 billion years ago in methanogenic microbes – long before oxygen levels rose in Earth’s atmosphere. The research was supported in part by the Exobiology and Evolutionary Biology (Exo/Evo) element of the NASA Astrobiology program.
When studying Methanocaldococcus jannaschii, a methanogen that lives in deep-sea hydrothermal vent environments, the team found a protein called thioredoxin. This protein plays a regulatory role in photosynthesis ...February 13, 2014 / Posted by: Aaron Gronstal
The workshop’s primary focus was to focus on the astrobiological potential of icy worlds in the outer solar system, including Europa, Ganymede, Enceladus, Titan, and beyond. Participants discussed future research directions and spacecraft missions that can best assess that potential. The agenda for the workshop was organized around thematic sessions that address the potential habitability of the unique planetary environments of the outer solar system.
Source: [USRA]February 12, 2014 / Posted by: Daniella Scalice
The image to the left shows Jennifer Glass working in a chamber where she can control the oxygen levels to mimic the deep sea environment. On the right is an example of marine gas hydrates on the sea floor. Credit: Rob Felt (left image); US Department of Energy (right image)
On March 3, 2014, Dr. Jennifer Glass of the Georgia Institute of Technology (GA Tech) will present the second in our series of talks from alumni of the NASA Astrobiology NASA Postdoctoral Program (NPP). In her talk, “Microbes, Methane and Metals: Insights From Geochemistry, Omics and Single Cell Imaging,” Glass ...February 11, 2014 / Written by: Aaron Gronstal
Water forms on interplanetary dust particles due to space-weathering from the solar wind. Hydrogen ions in the solar wind react with oxygen atoms in the dust to form tiny water-filled vesicles(blue). Credit: John Bradley, UH SOEST/ LLNL
Could Space Dust have Delivered Life’s Ingredients to Earth?
For the first time, scientists have detected water molecules on the surface of interplanetary dust particles. The water forms in tiny bubbles when solar wind irradiates and damages the dust grains floating through space.
Previous research had shown that space dust also contains organic carbon—another key ingredient for life. Taken together ...
Gemini Planet Imager's first light image of the light scattered by a disk of dust orbiting the young star HR4796A. This narrow ring is thought to be dust from asteroids or comets left behind by planet formation; some scientists have theorized that the sharp edge of the ring is defined by an unseen planet.
After nearly a decade of development, construction and testing, the world’s most advanced instrument for directly imaging and analyzing planets orbiting around other stars, the Gemini Planet Imager, is pointing skyward and collecting light from distant worlds. Read the full story here.
Source: [Lawrence ...February 5, 2014 / Posted by: Daniella Scalice
Voyager Views Titan's Haze. There is a lot of interesting chemistry occurring in Titan's dense atmosphere. Credit: Voyager Project, JPL, NASA
Henderson (Jim) Cleaves of the Carnegie Institution of Washington will present the next talk in the NAI Director’s Seminar Series on February 10 at 11:00 AM PST.
Amino Acid Analysis of Titan Tholins and Comparison With Other Prebiotic Reaction Systems
Titan’s atmospheric chemistry produces a host of discrete organic chemical products. It is likewise well known than Miller-Urey type reactions produce a host of complex discrete organic products. We have examined various complex reaction ...February 4, 2014 / Posted by: Aaron Gronstal
Fossil remains of Ediacara biota. Credit: Courtesy of Marc Laflamme, University of Toronto
A team of researchers, including members of the MIT Node of the NASA Astrobiology Institute (NAI), have revealed new insight into why organisms on the ancient Earth began to grow larger. Life began on our planet as single-cell microorganisms, but today the Earth supports a diverse array of multicellular life. The new study could help explain the advantages that early organisms gained from an increase in size.
The study, published in Current Biology, shows how primitive organisms called Ediacara became larger to help access nutrients in ocean ...February 4, 2014 / Written by: Aaron Gronstal
This equipment is used by Goddard's Astrobiology Analytical Lab to analyze very small samples. On the right is the nanoelectrospray emitter, which gives sample molecules an electric charge and transfers them to the inlet of the mass spectrometer (left), which identifies the molecules by their mass.
NAI-funded astrobiologists at NASA’s Goddard Space Flight Center have successfully completed a proof-of-concept study of a new technique to analyze extremely small samples of material such as from asteroids, comets, and IDPs for the presence of biomolecules such as amino acids, components used to make DNA, and other biologically important molecules like ...February 3, 2014 / Posted by: Daniella Scalice
The original box containing archived spark discharge samples prepared by Stanley Miller in 1958. The label shows Miller’s original writing: p 114 refers to his notebook. Credit: Jeffrey Bada and Robert Benson/Scripps Institution of Oceanography, University of California at San Diego
Back in 1953, Stanley Miller, working at the University of Chicago with Harold Urey, showed how easily one could cook up life’s building blocks by simulating the conditions on early Earth.
But while the success of the Miller-Urey experiment kicked off an entire field of research, Miller had one basic piece of advice for anyone who ...
As we are rapidly approaching the end of the end of this stage of the Astrobiology Strategy planning, we would like to thank everyone that has participated as a presenter or author, commented on a white paper or at a webinar, or even just listened in to one of the presentations. If you have not yet had the opportunity to listen to a particular webinar or comment on a particular white paper, they are all available on the website astrobiologyfuture.org. However, please visit the website soon, as we will be closing the papers to comments on Friday, February 14th ...February 1, 2014 / Posted by: Aaron Gronstal
NGC 7023: The Iris Nebula, Image Credit & Copyright: Jim Misti (acquisition), Robert Gendler (processing)
Astrobiologists at NASA Ames Research Center funded by the NASA Astrobiology Institute have recently published a study on the analysis of Polycyclic Aromatic Hydrocarbons, or PAH’s, in the Iris Nebula. Their analyses of individual PAH spectra have allowed them to see how different types of PAH’s map to different areas of the nebula, and also how PAH behavior changes with respect to changes in the local environment.
Source: [The Astrophysical Journal]January 30, 2014 / Posted by: Daniella Scalice
In the late 1990s, the University of Washington created what was arguably the world’s first graduate program in astrobiology, aimed at preparing scientists to hunt for life away from Earth. In 2001, David Catling became one of the first people brought to the UW specifically to teach astrobiology.
Catling, a UW professor of Earth and space sciences, is the author of Astrobiology: A Very Short Introduction, the 370th offering in the Oxford University Press series of “very short introduction” books by experts in various fields. Catling was commissioned by editors to write the book, which was published in the ...
REDESPA is a new Planetology and Astrobiology network in Spain, led by a Board of 40 experts from different disciplines and from more than a dozen Spanish organizations including the Spanish National Research Council, National Institute of Aerospace Technology, Centro de Astrobiología, National Astronomic Observatory, and Science Museum of Castilla-La Mancha. REDESPA’s mission is to share information and be an open platform about scientific subjects as well as educational, ethical, and societal issues. In the context of REDESPA, we have also launched a specific chapter for young researchers (JIPA: Jóvenes Investigadores en Planetología y Astrobiología). The Membership registration in ...January 27, 2014 / Posted by: Daniella Scalice
- Mar 10 - Director's Seminar: The Formation of Complex Organic Molecules in Star-Forming Regions
- Mar 17-21 - Lunar and Planetary Science Conference
- Mar 17-21 - Search for Life Beyond the Solar System: Exoplanets, Biosignatures & Instruments
- April 1 - Application Deadline for NASA Astrobiology Early Career Collaboration Award