Exoplanet discovery has made remarkable progress, with the first rocky planets having been detected in the central star's liquid water habitable zone. The remote sensing techniques used to characterize such planets for potential...
moreExoplanet discovery has made remarkable progress, with the first rocky planets having been detected in the central star's liquid water habitable zone. The remote sensing techniques used to characterize such planets for potential habitability and life rely solely on our understanding of life on Earth. The vegetation red edge from terrestrial land plants is often used as a direct signature of life, but it occupies only a small niche in the environmental parameter space that binds life on present-day Earth and has been widespread for only about 460 My. To more fully exploit the diversity of the one example of life known, we measured the spectral characteristics of 137 microorganisms containing a range of pigments, including ones isolated from Earth's most extreme environments. Our database covers the visible and near-infrared to the short-wavelength infrared (0.35–2.5 μm) portions of the electromagnetic spectrum and is made freely available from biosignatures. astro.cornell.edu. Our results show how the reflectance properties are dominated by the absorption of light by pigments in the visible portion and by strong absorptions by the cellular water of hydration in the infrared (up to 2.5 μm) portion of the spectrum. Our spectral library provides a broader and more realistic guide based on Earth life for the search for surface features of extraterrestrial life. The library, when used as inputs for modeling disk-integrated spectra of exoplanets, in preparation for the next generation of space-and ground-based instruments, will increase the chances of detecting life. biosignatures | spectral library | reflectivity | extremophiles | pigments I n the last decade, the field of exoplanet research has transi-tioned rapidly from detection to detection and characterization , with the first rocky exoplanets detected in the central star's liquid water habitable zone. Much of the excitement of this research in both the astrobiology community and the general public is motivated by the quest to discover a second genesis of life. The great distances that separate us from even the most nearby stars dictate that all measurements of the exoplanet must be made through remote sensing techniques for the foreseeable future. Thus, it is critical for us to determine the types of bio-signatures that we should be looking for when designing the next generation of ground-and space-based instruments that will observe these planets at high spectral and possibly spatial resolutions. Since the mid-1960s a primary life-searching strategy has been to look for a specific combination of an oxidizing and a reducing gas in the exoplanetary atmosphere, such as the O 2 and CH 4 in our atmosphere, because this is a thermodynamically unstable situation suggesting that an active agent such as life is responsible for the chemical disequilibrium (1, 2). Of particular interest, both from an observational and modeling perspective, is to complement those indirect life detection studies with surface features that are direct properties of the organisms themselves (3). Although there is a considerable knowledge base of the spectral properties of land plants (4, 5), very little information is present in the literature on the reflectance properties of microorganisms. Land plants are widespread on present-day Earth and are easily detected from high-resolution spacecraft observations (6). However, they occupy only a small niche in the environmental parameter space that brackets known terrestrial life. Additionally, land plants have been widespread on Earth for only about 460 My (7), whereas much of the history of life has been dominated by single-celled microbial life. Within the prokaryotic and eukaryotic microbes there is a far greater diversity of pigmentation than in land plants. For this reason, any hypotheses about extraterrestrial life based solely on land plants ignore much of the diversity of known life. To develop a more representative library of terrestrial spectra we produced a digital spectral library that provides high-resolution hemispherical reflectance measurements for 137 phylogenetically diverse microorganisms from the visible and near-infrared (VNIR, 0.35–1.0 μm) to the short-wavelength infrared (SWIR, 1.0–2.5 μm) regions of the electromagnetic spectrum. The library is made available from biosignatures.astro.cornell.edu. One approach when searching for life on exoplanets is to explore the range of pigmentation types that have evolved on this Earth. To examine the widest possible environmental range for life on Earth to inform our search we have chosen to include a diversity of extremophiles, organisms that live and thrive under conditions that make it challenging for a carbon-based organism using water as a solvent to survive (8). At the same time, we are cognizant of the fact that extremophiles are phylogenetically diverse and are unlikely to show spectral signatures not found among other pigmented organisms. Thus, we present reflectance spectra of organisms possessing a wide range of pigmentation but Significance We develop the first catalogue, to our knowledge, of reflectance spectra for a diverse range of pigmented microorganisms, including ones that were isolated from Earth's most extreme environments. This catalogue provides a broad scope of surface signatures for life on exoplanets, which could provide different conditions from those on Earth, allowing, for example, extrem-ophiles on Earth to become the predominant life form. Much of the history of life on Earth has been dominated by microbial life, and it is likely that life on exoplanets evolves through single-celled stages prior to multicellular creatures. Here, we present the first database, to our knowledge, for such surface features in preparation for the next generation of space-and ground-based telescopes that will search for a wide variety of life on exoplanets.