The Habitability of Proxima Centauri b: Environmental States and Observational Discriminants.

Proxima Centauri b provides an unprecedented opportunity to understand the evolution and nature of terrestrial planets orbiting M dwarfs. Although Proxima Cen b orbits within its star's habitable zone, multiple plausible evolutionary paths could have generated different environments that may or may not be habitable. Here, we use 1-D coupled climate-photochemical models to generate self-consistent atmospheres for several evolutionary scenarios, including high-O2, high-CO2, and more Earth-like atmospheres, with both oxic and anoxic compositions. We show that these modeled environments can be habitable or uninhabitable at Proxima Cen b's position in the habitable zone. We use radiative transfer models to generate synthetic spectra and thermal phase curves for these simulated environments, and use instrument models to explore our ability to discriminate between possible planetary states. These results are applicable not only to Proxima Cen b but to other terrestrial planets orbiting M dwarfs. Thermal phase curves may provide the first constraint on the existence of an atmosphere. We find that James Webb Space Telescope (JWST) observations longward of 10 µm could characterize atmospheric heat transport and molecular composition. Detection of ocean glint is unlikely with JWST but may be within the reach of larger-aperture telescopes. Direct imaging spectra may detect O4 absorption, which is diagnostic of massive water loss and O2 retention, rather than a photosynthetic biosphere. Similarly, strong CO2 and CO bands at wavelengths shortward of 2.5 µm would indicate a CO2-dominated atmosphere. If the planet is habitable and volatile-rich, direct imaging will be the best means of detecting habitability. Earth-like planets with microbial biospheres may be identified by the presence of CH4-which has a longer atmospheric lifetime under Proxima Centauri's incident UV-and either photosynthetically produced O2 or a hydrocarbon haze layer. Key Words: Planetary habitability and biosignatures-Planetary atmospheres-Exoplanets-Spectroscopic biosignatures-Planetary science-Proxima Centauri b. Astrobiology 18, 133-189.

Novel method for determining hydrogel and silicone hydrogel contact lens transmission curves and their spatially specific ultraviolet radiation protection factors.

PURPOSE: Anterior ocular tissues exposed to high levels of toxic ultraviolet (UV) radiation may undergo physiologic changes leading to diseases that can alter the ocular surface, particularly in the stem cell-rich limbal region. UV radiation-blocking hydrogel contact lenses provide protection across the ocular surface, which varies according to the lens thickness. METHODS: A novel fiber optic spectrophotometer front-end system has been developed to measure lens transmission curves at test points across lens surfaces to determine optical properties based on the Beer-Lambert law. Factors determining the transmission curves include the hydrogel lens used, its refractive index, whether a UV radiation-blocking dopant is incorporated, the water content, and the thickness of the lens. Test lenses of equal power were placed over a detecting fiber optic and illuminated by a deuterium source, and transmission spectra were recorded. The small optical sampling size allowed the spectral transmission profile to be determined across the lens surface, and comparisons were made with different lenses. RESULTS: Transmission curves across the lenses showed greater UV radiation-blocking capacity at the thicker peripheral region, with the 50% cutoff wavelength moving toward the visible spectrum by 10 nm from the center to the periphery. In addition, the ability to determine the spatially specific absorption coefficient and the related UV radiation protection factor was demonstrated. CONCLUSIONS: The system measures spatial variation in lens transmission and comparing different lens types while overcoming many of the handling limitations of cuvette-based spectrophotometer methods. The data show good agreement with published transmission curves and allow intralens and interlens comparisons.