Literature DB >> 17407409

Spectral signatures of photosynthesis. I. Review of Earth organisms.

Nancy Y Kiang1, Janet Siefert, Robert E Blankenship.   

Abstract

Why do plants reflect in the green and have a "red edge" in the red, and should extrasolar photosynthesis be the same? We provide (1) a brief review of how photosynthesis works, (2) an overview of the diversity of photosynthetic organisms, their light harvesting systems, and environmental ranges, (3) a synthesis of photosynthetic surface spectral signatures, and (4) evolutionary rationales for photosynthetic surface reflectance spectra with regard to utilization of photon energy and the planetary light environment. We found the "near-infrared (NIR) end" of the red edge to trend from blue-shifted to reddest for (in order) snow algae, temperate algae, lichens, mosses, aquatic plants, and finally terrestrial vascular plants. The red edge is weak or sloping in lichens. Purple bacteria exhibit possibly a sloping edge in the NIR. More studies are needed on pigment-protein complexes, membrane composition, and measurements of bacteria before firm conclusions can be drawn about the role of the NIR reflectance. Pigment absorbance features are strongly correlated with features of atmospheric spectral transmittance: P680 in Photosystem II with the peak surface incident photon flux density at approximately 685 nm, just before an oxygen band at 687.5 nm; the NIR end of the red edge with water absorbance bands and the oxygen A-band at 761 nm; and bacteriochlorophyll reaction center wavelengths with local maxima in atmospheric and water transmittance spectra. Given the surface incident photon flux density spectrum and resonance transfer in light harvesting, we propose some rules with regard to where photosynthetic pigments will peak in absorbance: (1) the wavelength of peak incident photon flux; (2) the longest available wavelength for core antenna or reaction center pigments; and (3) the shortest wavelengths within an atmospheric window for accessory pigments. That plants absorb less green light may not be an inefficient legacy of evolutionary history, but may actually satisfy the above criteria.

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Year:  2007        PMID: 17407409     DOI: 10.1089/ast.2006.0105

Source DB:  PubMed          Journal:  Astrobiology        ISSN: 1557-8070            Impact factor:   4.335


  43 in total

Review 1.  Energy conversion in natural and artificial photosynthesis.

Authors:  Iain McConnell; Gonghu Li; Gary W Brudvig
Journal:  Chem Biol       Date:  2010-05-28

2.  Photochemical performance of the acidophilic red alga Cyanidium sp. in a pH gradient.

Authors:  Jana Kvíderová
Journal:  Orig Life Evol Biosph       Date:  2012-06-02       Impact factor: 1.950

3.  Detection of circular polarization in light scattered from photosynthetic microbes.

Authors:  William B Sparks; James Hough; Thomas A Germer; Feng Chen; Shiladitya DasSarma; Priya DasSarma; Frank T Robb; Nadine Manset; Ludmilla Kolokolova; Neill Reid; F Duccio Macchetto; William Martin
Journal:  Proc Natl Acad Sci U S A       Date:  2009-04-28       Impact factor: 11.205

4.  Govindjee at 80: more than 50 years of free energy for photosynthesis.

Authors:  Julian J Eaton-Rye
Journal:  Photosynth Res       Date:  2013-10-10       Impact factor: 3.573

5.  Bioconjugatable, PEGylated Hydroporphyrins for Photochemistry and Photomedicine. Narrow-Band, Red-Emitting Chlorins.

Authors:  Mengran Liu; Chih-Yuan Chen; Amit Kumar Mandal; Vanampally Chandrashaker; Rosemary B Evans-Storms; J Bruce Pitner; David F Bocian; Dewey Holten; Jonathan S Lindsey
Journal:  New J Chem       Date:  2016-07-21       Impact factor: 3.591

6.  What governs the reaction center excitation wavelength of photosystems I and II?

Authors:  Ron Milo
Journal:  Photosynth Res       Date:  2009-07-08       Impact factor: 3.573

7.  The Significance of Microbe-Mineral-Biomarker Interactions in the Detection of Life on Mars and Beyond.

Authors:  Wilfred F M Röling; Joost W Aerts; C H Lucas Patty; Inge Loes ten Kate; Pascale Ehrenfreund; Susana O L Direito
Journal:  Astrobiology       Date:  2015-06       Impact factor: 4.335

8.  Nonphotosynthetic pigments as potential biosignatures.

Authors:  Edward W Schwieterman; Charles S Cockell; Victoria S Meadows
Journal:  Astrobiology       Date:  2015-05-05       Impact factor: 4.335

Review 9.  Exoplanet Biosignatures: Future Directions.

Authors:  Sara I Walker; William Bains; Leroy Cronin; Shiladitya DasSarma; Sebastian Danielache; Shawn Domagal-Goldman; Betul Kacar; Nancy Y Kiang; Adrian Lenardic; Christopher T Reinhard; William Moore; Edward W Schwieterman; Evgenya L Shkolnik; Harrison B Smith
Journal:  Astrobiology       Date:  2018-06       Impact factor: 4.335

Review 10.  On the free energy that drove primordial anabolism.

Authors:  Michael Kaufmann
Journal:  Int J Mol Sci       Date:  2009-04-22       Impact factor: 6.208

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