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The Habitability of Proxima Centauri b: Environmental States and Observational DiscriminantsProxima 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 mm 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 mm 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.
Document ID
20180003054
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Meadows, Victoria S.
(Washington Univ. Seattle, WA, United States)
Arney, Giada N.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Schwieterman, Edward W.
(Washington Univ. Seattle, WA, United States)
Lustig-Yaeger, Jacob
(Washington Univ. Seattle, WA, United States)
Lincowski, Andrew P.
(Washington Univ. Seattle, WA, United States)
Robinson, Tyler
(California Univ. Santa Cruz, CA, United States)
Domagal-Goldman, Shawn D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Deitrick, Russell
(Washington Univ. Seattle, WA, United States)
Barnes, Rory K.
(Washington Univ. Seattle, WA, United States)
Fleming, David P.
(Washington Univ. Seattle, WA, United States)
Luger, Rodrigo
(Washington Univ. Seattle, WA, United States)
Driscoll, Peter E.
(Carnegie Institution for Science Washington, DC, United States)
Quinn, Thomas R.
(Washington Univ. Seattle, WA, United States)
Crisp, David
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
May 25, 2018
Publication Date
February 1, 2018
Publication Information
Publication: Astrobiology
Publisher: Mary Ann Liebert
Volume: 18
Issue: 2
ISSN: 1531-1074
e-ISSN: 1557-8070
Subject Category
Geosciences (General)
Lunar And Planetary Science And Exploration
Report/Patent Number
GSFC-E-DAA-TN53800
Funding Number(s)
CONTRACT_GRANT: NSF IGERT DGE-1258485
CONTRACT_GRANT: NNA13AA93A
CONTRACT_GRANT: NNH12ZDA002C
CONTRACT_GRANT: 80KSC017C0007
Distribution Limits
Public
Copyright
Other

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