Graduate student Jeff Bowman examines "frost flowers", microbially-enriched ice crystals on the Arctic sea ice.
Graduate student David Smith with Professor Peter Ward on James Ross Island, Antarctica, searching for fossils that hold clues to ancient climate and extinction patterns on Earth.
UWAB graduate students Megan Smith and Elena Amador sample waters from the highly acidic Rio Tinto in Spain looking for an analog to early Martian environments.
Postdoc and UWAB Alum William Brazelton (PhD, ’10), high in Newfoundland’s Gros Morne National Park, searches for microbial life fueled by serpentinization.

Welcome to Astrobiology at the University of Washington

UWAB Headlines


Collisions Could Reveal "Invisible Gas" In Exoplanets

UWAB graduate student Edward Schwieterman, professor Victoria Meadows, and researchers Tyler Robinson, Amit Misra, and Shawn Domagal-Goldman have demonstrated that the collisional absorption signature of nitrogen gas can be detected in Earth’s disk-averaged spectrum and have modeled how it would appear on Earth-like exoplanets. Usually, nitrogen is considered an “invisible gas” because it lacks normal spectral features.  Detection of nitrogen would provide a means to characterize the bulk atmosphere of potentially habitable exoplanets and constrain the likelihood of oxygen production by non-living processes. The paper has been published in The Astrophysical Journal here.   MORE>


Atmospheric signs of volcanic activity could aid search for life

UW Astrobiology graduate students Amit Misra, Josh Krissansen-Totton, Matt Koehler and Steve Sholes have collaborated on an interdisciplinary paper on how to detect geological activity on extrasolar planets by looking for volcanically-induced transient sulfate aerosols in the planet's atmosphere. MORE>


Beyond Human: Animals, Aliens, and Artificial Intelligence!

UWAB and Museology graduate student, Wolf Clifton, has launched his Masters project which is an online exhibit titled "Beyond Human: Animals, Aliens, and Artificial Intelligence!" MORE>


Searching for Alien Biosignatures: Non-Photosynthetic Organisms May Produce Novel Signatures of Life on Exoplanets

UWAB graduate student Edward Schwieterman, professor Victoria Meadows, and professor Charles Cockell at the UK Centre for Astrobiology present an interdisciplinary study of the possibility non-photosynthetic organisms may create signs of life on Earth-like exoplanets. These organisms contain pigments that reflect light differently than water, rocks, or photosynthetic organisms like land plants, producing spectral signatures that could indicate the presence of life. The paper resulted from an Astrobiology Program research rotation and was published in the May issue of Astrobiology. MORE>


Stars May Change Mini-Neptunes into Habitable Planets

UWAB graduate student Rodrigo Luger, professors Rory Barnes and Victoria Meadows, and collaborators have found that some terrestrial planets in the habitable zones of low mass stars could be the evaporated cores of small Neptune-like planets. While these planets are likely to be very different from Earth in composition, they should have abundant surface water, one of the principal ingredients for habitability. The paper was published in the January issue of Astrobiology. MORE>


New Venus Studies Probe the Dynamic Atmosphere Below the Clouds and Reveal the Complexities of Hazy Worlds

UWAB graduate student, Giada Arney, and VPL colleagues, present the first maps of cloud opacity, droplet sulfuric acid percentage, and trace gases in the Venus lower atmosphere.  Unexpected temporal and spatial variations of several species may be related to rainout processes, and variable hemispherical dichotomies suggest that the Venusian troposphere is just as dynamic as higher layers of the atmosphere.  There may be many Venus-like exoplanets, and understanding the planet next door is the first step to understanding these other worlds. MORE>


UWAB Autumn 2014 Newsletter Released!

For up-to-date news about what's going on with UW Astrobiology, check out the latest issue of our newsletter! MORE>


Too Hot To Handle: Planets in the Habitable Zones of Low Mass Stars May Be Roasted Early On

UWAB graduate student Rodrigo Luger and Professor Rory Barnes have shown that many terrestrial planets in the habitable zones of low mass (M dwarf) stars could have experienced extreme stellar heating for up to 1 billion years after planet formation. This heating arises because M dwarfs evolve differently than the Sun -- they contract and cool for a much longer period of time. As they cool, the habitable zone moves in and so planets we find in the habitable zone today may have spent up to 1 billion years in a Venus-like state. During this period, destruction of water by UV radiation and hydrogen escape to space could ultimately build up massive abiotic oxygen atmospheres. MORE>