Photos and highlights from the Oct-Nov 2018 expedition to better understand ways to search for life beyond Earth.
This illustration shows a simulated view of NASA's Interior Exploration using Seismic Investigations, Geodesy and Heat Transport (InSight) lander firing retrorockets to slow down as it descends toward the surface of Mars. Credits: NASA/JPL-Caltech
NASA’s Mars Interior Exploration using Seismic Investigations, Geodesy and Heat Transport (InSight) lander is scheduled to touch down on the Red Planet at approximately 3 p.m. EST Nov. 26, and viewers everywhere can watch coverage of the event live on NASA Television, the agency’s website and social media platforms.
Launched on May 5, InSight marks NASA’s first Mars landing since the Curiosity rover in 2012. The landing will kick off a two-year mission in which InSight will become the first spacecraft to study Mars’ deep interior. Its data also will help scientists understand the formation of all rocky worlds, including our own.
Read the press release from NASA.
For more on InSight and its connection to astrobiology, visit the Astrobiology at NASA website.
Source: [NASA]November 26, 2018 • Written by: NASA • Report issue
The Andes field expedition team's camp at night. Right in the center of the star trail, the two Magellanic Clouds give visions of alien worlds. Photo credit: Victor Robles, Campoalto and the SETI Institute NAI Team.
Nathalie Cabrol, Director of the Carl Sagan Center for the Study of Life in the Universe, led the SETI Institute NAI team on its 2018 field expedition to the Andes:
“This year, between October 17-November 20, 2018, my team and I are returning to the Chilean High Andes,” said Nathalie. “There we will continue the development of new planetary exploration strategies, instruments, and systems, that in the near future will dramatically change the way we search for life beyond Earth. Our project is supported by the NASA Astrobiology Institute and helps prepare missions such as Mars 2020 and ExoMars that will soon seek traces of ancient biosignatures on the Red Planet.”
While the team is in Chile, Nathalie has posted updates when she is able to be in an area with an Internet connection. The photos are amazing!
Source: [SETI Institute]November 20, 2018 • Written by: SETI Institute • Report issue
To better support the broad, interdisciplinary field of astrobiology – the study of the origin, evolution, distribution, and future of life in the universe – NASA is announcing a new programmatic infrastructure for the Astrobiology Program. Source: NASA Astrobiology
To better support the broad, interdisciplinary field of astrobiology – the study of the origin, evolution, distribution, and future of life in the universe – NASA is announcing a new programmatic infrastructure for the Astrobiology Program.
By the end of 2019, the Astrobiology Program will establish several virtual collaboration structures called “research coordination networks” (RCNs) that will replace the Program’s virtual institute, the NASA Astrobiology Institute (NAI). With this shift, NASA’s overall investment in the Astrobiology Program is not changing. Astrobiology is an important part of NASA’s portfolio and Congress formally added Astrobiology as one of NASA’s ...
Source: [NASA Astrobiology Program]November 01, 2018 • Written by: NASA Astrobiology • Report issue
With the October issue of the NASA Astrobiology Institute (NAI) Newsletter, we are merging the content of the NAI Newsletter with the International Astrobiology Newsletter (IAN), https://ian.arc.nasa.gov. IAN has been hosted by the NAI for many years as a service to the international astrobiology community, a community which itself has provided the newsletter’s content. Because there existed numerous sites that report on the science of astrobiology, IAN focused on activities such as astrobiology conferences and conference sessions, workshops and educational events, career opportunities, and proposal calls. This and future issues of the NAI Newsletter will incorporate content from IAN, providing a more comprehensive update on activities in the growing field of astrobiology.October 30, 2018 • Posted by: Miki Huynh • Report issue
Astrobiology has a long tradition in Europe, which manifested itself in the foundation of the Centro de Astrobiologia in 1999 (CAB) and the launch of the European Astrobiology Network Association (EANA) in 2001. CAB has organized, in collaboration with the NASA Astrobiology Institute (NAI), sixteen “International Summer Schools in Astrobiology,” and EANA holds annual workshops in the field attended by astrobiologists from all over the world. Since this date, many national astrobiology societies and a regional astrobiology network (the Nordic Network of Astrobiology, which has organised a multitude of astrobiology events) in Europe, have been created. Despite recommendations of the ...
Source: [European Astrobiology Institute]October 29, 2018 • Written by: Wolf Geppert • Report issue
Habitable exoplanets where life uses the purple-pigmented compound retinal to provide metabolic energy from sunlight could provide a remote biosignature when viewed spectroscopically. Image credit: NASA/Ames/JPL–Caltech.
Early life-forms on Earth may have been able to generate metabolic energy from sunlight using a purple-pigmented molecule called retinal that possibly predates the evolution of chlorophyll and photosynthesis. If retinal has evolved on other worlds, it could create a a distinctive biosignature as it absorbs green light in the same way that vegetation on Earth absorbs red and blue light.
Earth’s atmosphere has not always contained significant amounts of oxygen. For the first two billion years of our planet’s history, the atmosphere was rich in carbon dioxide and methane, but around 2.4 billion years ago something ...
Source: [Astrobiology Magazine (astrobio.net)]October 25, 2018 • Written by: Keith Cooper • Report issue
Application Deadline: December 3, 2018
The Astrobiology Early Career Collaboration Awards offer research-related travel support for undergraduate, graduate students, postdocs, and junior scientists. Applicants are encouraged to use these resources to circulate among two or more laboratories supported by the NASA Astrobiology Program (Exobiology and Evolutionary Biology, the NAI, Planetary Science and Technology Through Analog Research, MatiSSE, PICASSO and the Habitable Worlds), however any travel that is critical for the applicant’s research will be considered. Travelers must be formally affiliated with a U.S. institution. Requests are limited to $5,000.
More information is available at: https://nai.nasa ...
Source: [ECCA]October 24, 2018 • Posted by: Miki Huynh • Report issue
Left: Example of a black smoker hydrothermal vent in the Atlantic Ocean (Source: Wikimedia Commons). Right A-D: Photos showing how hydrothermal mineral samples are turned into electrode ink that can be painted onto a fuel cell electrode assembly.
Seafloor hydrothermal vents are natural geo-electro-chemical systems that behave in some ways like fuel cells. They produce redox gradients that can help to support life with geochemical energy. Such vents are also thought to exist on other worlds such as Europa or Enceladus, and may provide habitable environments where life could emerge even in the absence of sunlight.
A research team led by Dr. Laurie Barge a member of the NASA Astrobiology Institute (NAI)’s Jet Propulsion Laboratory Icy World team, in collaboration with the SETI Institute node of the NAI, has used fuel cell experimental techniques to simulate the ...
Source: [Astrobiology (via SETI and JPL)]October 22, 2018 • Posted by: Miki Huynh • Report issue
The Search for Life Near and Far
Deadline Extended: November 6, 2018 11:59PM ET
AbSciCon 2019 is the next conference in a series organized by the astrobiology community. This year’s theme is Understanding and Enabling the Search for Life on Worlds Near and Far. Future missions and observations will aim to further our understanding of diverse planetary environments while fundamental research on the origin and evolution of life on Earth drives our understanding of how life may operate elsewhere.
Session proposal topics are encouraged to span a broad array of topics with strong interdisciplinary themes that address new ...
Source: [AbSciCon]October 15, 2018 • Posted by: Miki Huynh • Report issue
On October 10, 2018, the committee appointed by the National Academies of Sciences, Engineering, and Medicine presented recommendations for a research strategy and direction in the study of astrobiology to NASA and the scientific community.
A recording of the livestream can be viewed at: https://livestream.com/NASEM/AstrobioScience.
The report can be downloaded at https://www.nap.edu/astrobioscience.
Source: [NASEM]October 10, 2018 • Posted by: Miki Huynh • Report issue
Left: Dr. Jennifer Glass holds a piece of stromatolitic ironstone. Research conducted in her lab at Georgia Tech points to the way in which nitrous oxide may have helped warm early Earth. Photo credit: Georgia Tech / A. Carter. Right: Banded iron formations in Karijini National Park, Australia. These sediments, once ancient seafloor, are red because iron rusted out of solution as oxygen built up in the water. The same dissolved iron facilitated production of nitrous oxide. Photo credit: Georgia Tech / J. Glass
Carbon dioxide and methane get partial credit for keeping the early Earth ice-free, but established research suggests that those gases were not always sufficiently abundant to warm the globe on their own. A new view on ocean chemistry during Earth’s Proterozoic Eon, about 2.5-0.5 billion years ago, point to a possible way that nitrous oxide, also known as laughing gas, could have filled the “greenhouse gap.” Results published by scientists at Georgia Tech who are members of the Alternative Earths team, the NASA Astrobiology Institute team based at the University of California, Riverside, demonstrate a potential mechanism ...September 21, 2018 • Posted by: Miki Huynh • Report issue
A sample of a thermal map of an exoplanet (left) and the corresponding position on an orbital diagram (right). Source: A.D.Adams/NASA Ames Research Center.
Members of the NASA Astrobiology Institute based at NASA Ames Research Center team have published a paper describing a thermal model applied to light curves of planet-bearing stars. The model accurately reproduces much of the large-scale data of existing full-orbit photometry captured by the Spitzer Space Telescope, including the timescale of heating/cooling, the time positions of minimum and maximum flux, and depths of transits and secondary eclipses.
“Reassessing Exoplanet Light Curves with a Thermal Model” is published in the Astronomical Journal.September 07, 2018 • Posted by: Miki Huynh • Report issue
NASA Astrobiology Institute (NAI) Georgia Tech team postdoctoral fellow Kennda Lynch and several astrobiologists are featured in the Netflix series Explained episode 9, “Extraterrestrial Life,” which digs into the probabilities of finding life in the universe. The episode was released on July 4, 2018.
A preview with clips of interviews was tweeted by Vox.
Source: [Netflix]August 31, 2018 • Posted by: Miki Huynh • Report issue
An article in Science describes the research of evolutionary biologists, including Matt Herron and Will Ratcliff, members of the NASA Astrobiology Institute’s Georgia Tech team, in examining the mechanisms that enabled the transition from single cells to multicellular life. Across a variety of organisms, the researchers found that a series of small genetic steps may have been responsible for the shift to multicellularity.
The story includes this video highlighting the work happening at their lab.
Source: [Science]August 27, 2018 • Posted by: Miki Huynh • Report issue
Terry Isson and Noah Planavsky provide a new framework for global climate regulation to explain Earth's warmer past climate. Image source: NASA
Scientists with the NASA Astrobiology Institute team based at UC Riverside have published a new paper providing explanation for why Earth’s early climate was more stable and warmer than it is today.
Excerpted from the story by Jim Shelton at YaleNews:
When life first evolved more than 3.5 billion years ago, Earth’s surface environment looked very different. The sun was much weaker, but Earth remained warm enough to keep liquid water at the surface. The researchers said this suggests that much higher carbon dioxide levels would have been needed to keep early Earth warm enough. But how ...
Source: [Nature (via UC Riverside)]August 17, 2018 • Written by: YaleNews • Report issue
- December 15 - Application Deadline: Bateman Postdoctoral Fellowship, Yale University
- December 20 - Application Deadline: Open Position in Planetary Geology
- December 23 - Application Deadline: Postdoctoral Research in Microbial Nitrogen Cycling
- December 31 - Abstract submission deadline for Workshop on In Situ Exploration of the Ice Giants
- December 31 - Early Registration Deadline for Mars Extant Life: What's Next?
- December 31 - Application Deadline: Emergence of Metabolism and Mineral-Organic Chemistry on Early Earth and Ocean Worlds
- December 31 - Application Deadline: Assistant Professor
- December 31 - Application Deadline: NASA SMD Seeks Volunteer Reviewers
- December 31 - Application Deadline: Research Fellow - Microbiome Research
- January 1 - Application Deadline: Grad Student/Postdoc Opportunities in Planetary Surface Processes at UT Austin
- January 4 - Application Deadline: Ph.D. Graduate Positions at Universidad de Atacama
- January 5 - Application Deadline: Research Associate in Planetary Science at CU Boulder
- January 5 - Application Deadline: M.S./Ph.D. positions for Fall 2019
- January 7 - CALL FOR SESSIONS: 2019 NAM for Royal Astronomical Society 2019 National Astronomy Meeting
- January 7 - Application Deadline: Assistant Professor Position, Department of Astronomy, New Mexico State University
- January 8 - Application Deadline: Graduate and Postdoctoral Opportunities in Planetary Surface Processes at Stanford University
- January 15 - Application Deadline: Director, University of Texas Institute for Geophysics
- January 15 - Application Deadline: Research Opportunities at the University of Hawaii: Fluid Migration in Titan's Ice Shell