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Sparks WB, Parenteau MN, Blankenship RE, Germer TA, Patty CHL, Bott KM, Telesco CM, Meadows VS. Spectropolarimetry of Primitive Phototrophs as Global Surface Biosignatures. Astrobiology 2021; 21:219-234. [PMID: 33216615 PMCID: PMC7876348 DOI: 10.1089/ast.2020.2272] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Download PDF] [Figures] [Subscribe] [Scholar Register] [Received: 04/06/2020] [Accepted: 10/12/2020] [Indexed: 06/11/2023]
Abstract
Photosynthesis is an ancient metabolic process that began on early Earth and offers plentiful energy to organisms that can utilize it such that that they achieve global significance. The potential exists for similar processes to operate on habitable exoplanets and result in observable biosignatures. Before the advent of oxygenic photosynthesis, the most primitive phototrophs, anoxygenic phototrophs, dominated surface environments on the planet. Here, we characterize surface polarization biosignatures associated with a diverse sample of anoxygenic phototrophs and cyanobacteria, examining both pure cultures and microbial communities from the natural environment. Polarimetry is a tool that can be used to measure the chiral signature of biomolecules. Chirality is considered a universal, agnostic biosignature that is independent of a planet's biochemistry, receiving considerable interest as a target biosignature for life-detection missions. In contrast to preliminary indications from earlier work, we show that there is a diversity of distinctive circular polarization signatures, including the magnitude of the polarization, associated with the variety of chiral photosynthetic pigments and pigment complexes of anoxygenic and oxygenic phototrophs. We also show that the apparent death and release of pigments from one of the phototrophs is accompanied by an elevation of the reflectance polarization signal by an order of magnitude, which may be significant for remotely detectable environmental signatures. This work and others suggest that circular polarization signals up to ∼1% may occur, significantly stronger than previously anticipated circular polarization levels. We conclude that global surface polarization biosignatures may arise from anoxygenic and oxygenic phototrophs, which have dominated nearly 80% of the history of our rocky, inhabited planet.
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Affiliation(s)
- William B. Sparks
- SETI Institute, Mountain View, California, USA
- Space Telescope Science Institute, Baltimore, Maryland, USA
| | - Mary Niki Parenteau
- Virtual Planetary Laboratory, University of Washington, Seattle, Washington, USA
- NASA Ames Research Center, Moffett Field, California, USA
| | - Robert E. Blankenship
- Virtual Planetary Laboratory, University of Washington, Seattle, Washington, USA
- Department of Biology, Washington University in St. Louis, St. Louis, Missouri, USA
- Department of Chemistry, Washington University in St. Louis, St. Louis, Missouri, USA
| | - Thomas A. Germer
- National Institute of Standards and Technology, Gaithersburg, Maryland, USA
| | - Christian Herman Lucas Patty
- Institute of Plant Biology, Hungarian Academy of Sciences, Szeged, Hungary
- Space Research and Planetary Sciences, University of Bern, Bern, Switzerland
| | - Kimberly M. Bott
- Virtual Planetary Laboratory, University of Washington, Seattle, Washington, USA
- Department of Earth and Planetary Sciences, University of California, Riverside, Riverside, California, USA
| | - Charles M. Telesco
- Department of Astronomy, University of Florida, Gainesville, Florida, USA
| | - Victoria S. Meadows
- Virtual Planetary Laboratory, University of Washington, Seattle, Washington, USA
- Department of Astronomy, University of Washington, Seattle, Washington, USA
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Sparks WB, Germer TA, Sparks RM. Classical polarimetry with a twist: a compact, geometric approach. Publ Astron Soc Pac 2019; 131:10.1088/1538-3873/ab1933. [PMID: 31579323 PMCID: PMC6774357 DOI: 10.1088/1538-3873/ab1933] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/10/2023]
Abstract
We present an approach to classical polarimetry that requires no moving parts, is compact and robust, and that encodes the complete polarization information on a single data frame, accomplished by replacing the rotation of components such as wave plates with position along a spatial axis. We demonstrate the concept with a polarimeter having a quarter wave plate whose fast axis direction changes with location along one axis of a 2D data frame in conjunction with a fixed-direction polarization analyzer, analogous to a classical rotating quarter wave plate polarimeter. The full set of Stokes parameters is obtained, with maximal sensitivity to circular polarization Stokes V if a quarter wave retarder is used. Linear and circular polarization terms are encoded with spatial carrier frequencies that differ by a factor two, which minimizes cross-talk. Other rotating component polarimeters lend themselves to the approach. Since the polarization modulation spatial frequencies do not change greatly, if at all, with wavelength such devices are close to achromatic, simplifying instrument design. Since the polarimetric information is acquired in a single observation, rapidly varying, transient and moving targets are accessible, loss of precision due to sequential data acquisition is avoided, and moving parts are not required.
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Affiliation(s)
- William B. Sparks
- SETI Institute, 189 Bernardo Avenue, Suite 200, Mountain View, CA 94043
| | - Thomas A. Germer
- National Institute of Standards and Technology, 100 Bureau Drive, Gaithersburg, MD 20899
| | - Rebecca M. Sparks
- Irvine Nature Center, 11201 Garrison Forest Road, Owings Mills, MD 21117
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Patty CHL, Luo DA, Snik F, Ariese F, Buma WJ, Ten Kate IL, van Spanning RJM, Sparks WB, Germer TA, Garab G, Kudenov MW. Imaging linear and circular polarization features in leaves with complete Mueller matrix polarimetry. Biochim Biophys Acta Gen Subj 2018. [PMID: 29526506 DOI: 10.1016/j.bbagen.2018.03.005] [Citation(s) in RCA: 31] [Impact Index Per Article: 5.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/17/2022]
Abstract
Spectropolarimetry of intact plant leaves allows to probe the molecular architecture of vegetation photosynthesis in a non-invasive and non-destructive way and, as such, can offer a wealth of physiological information. In addition to the molecular signals due to the photosynthetic machinery, the cell structure and its arrangement within a leaf can create and modify polarization signals. Using Mueller matrix polarimetry with rotating retarder modulation, we have visualized spatial variations in polarization in transmission around the chlorophyll a absorbance band from 650 nm to 710 nm. We show linear and circular polarization measurements of maple leaves and cultivated maize leaves and discuss the corresponding Mueller matrices and the Mueller matrix decompositions, which show distinct features in diattenuation, polarizance, retardance and depolarization. Importantly, while normal leaf tissue shows a typical split signal with both a negative and a positive peak in the induced fractional circular polarization and circular dichroism, the signals close to the veins only display a negative band. The results are similar to the negative band as reported earlier for single macrodomains. We discuss the possible role of the chloroplast orientation around the veins as a cause of this phenomenon. Systematic artefacts are ruled out as three independent measurements by different instruments gave similar results. These results provide better insight into circular polarization measurements on whole leaves and options for vegetation remote sensing using circular polarization.
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Affiliation(s)
- C H Lucas Patty
- Molecular Cell Physiology, VU Amsterdam, De Boelelaan 1108, 1081 HZ Amsterdam, The Netherlands.
| | - David A Luo
- Optical Sensing Lab, Department of Electrical and Computer Engineering, North Carolina State University, Raleigh, NC 27695, USA
| | - Frans Snik
- Leiden Observatory, Leiden University, P.O. Box 9513, Leiden 2300 RA, The Netherlands
| | - Freek Ariese
- LaserLaB, VU Amsterdam, De Boelelaan 1083, Amsterdam 1081 HV, The Netherlands
| | - Wybren Jan Buma
- HIMS, Photonics Group, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, The Netherlands
| | - Inge Loes Ten Kate
- Department of Earth Sciences, Utrecht University, Budapestlaan 4, Utrecht 3584 CD, The Netherlands
| | - Rob J M van Spanning
- Systems Bioinformatics, VU Amsterdam, De Boelelaan 1108, Amsterdam 1081 HZ, The Netherlands
| | - William B Sparks
- Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
| | - Thomas A Germer
- Senior Science Division, National Institute of Standards and Technology, 100 Bureau Drive, Gaithersburg, MD 20899, USA
| | - Győző Garab
- Institute of Plant Biology, Biological Research Centre, Hungarian Academy of Sciences, P.O. Box 521, Szeged H-6701, Hungary; Department of Physics, Faculty of Science, University of Ostrava, Chittussiho 10, Slezská Ostrava, Czech Republic
| | - Michael W Kudenov
- Optical Sensing Lab, Department of Electrical and Computer Engineering, North Carolina State University, Raleigh, NC 27695, USA
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Meyer ET, Georganopoulos M, Sparks WB, Perlman E, van der Marel RP, Anderson J, Sohn ST, Biretta J, Norman C, Chiaberge M. A kiloparsec-scale internal shock collision in the jet of a nearby radio galaxy. Nature 2015; 521:495-7. [PMID: 26017450 DOI: 10.1038/nature14481] [Citation(s) in RCA: 18] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/25/2014] [Accepted: 03/31/2015] [Indexed: 11/09/2022]
Abstract
Jets of highly energized plasma with relativistic velocities are associated with black holes ranging in mass from a few times that of the Sun to the billion-solar-mass black holes at the centres of galaxies. A popular but unconfirmed hypothesis to explain how the plasma is energized is the 'internal shock model', in which the relativistic flow is unsteady. Faster components in the jet catch up to and collide with slower ones, leading to internal shocks that accelerate particles and generate magnetic fields. This mechanism can explain the variable, high-energy emission from a diverse set of objects, with the best indirect evidence being the unseen fast relativistic flow inferred to energize slower components in X-ray binary jets. Mapping of the kinematic profiles in resolved jets has revealed precessing and helical patterns in X-ray binaries, apparent superluminal motions, and the ejection of knots (bright components) from standing shocks in the jets of active galaxies. Observations revealing the structure and evolution of an internal shock in action have, however, remained elusive, hindering measurement of the physical parameters and ultimate efficiency of the mechanism. Here we report observations of a collision between two knots in the jet of nearby radio galaxy 3C 264. A bright knot with an apparent speed of (7.0 ± 0.8)c, where c is the speed of light in a vacuum, is in the incipient stages of a collision with a slower-moving knot of speed (1.8 ± 0.5)c just downstream, resulting in brightening of both knots--as seen in the most recent epoch of imaging.
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Affiliation(s)
- Eileen T Meyer
- 1] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218, USA [2] University of Maryland Baltimore County, 1000 Hilltop Circle, Baltimore, Maryland 21250, USA
| | - Markos Georganopoulos
- 1] University of Maryland Baltimore County, 1000 Hilltop Circle, Baltimore, Maryland 21250, USA [2] NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - William B Sparks
- Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218, USA
| | - Eric Perlman
- Florida Institute of Technology, 150 West University Boulevard, Melbourne, Florida 32901, USA
| | | | - Jay Anderson
- Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218, USA
| | - Sangmo Tony Sohn
- Johns Hopkins University, 3400 North Charles Street, Baltimore, Maryland 21218, USA
| | - John Biretta
- Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218, USA
| | - Colin Norman
- 1] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218, USA [2] Johns Hopkins University, 3400 North Charles Street, Baltimore, Maryland 21218, USA
| | - Marco Chiaberge
- 1] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218, USA [2] Johns Hopkins University, 3400 North Charles Street, Baltimore, Maryland 21218, USA [3] Istituto Nazionale Astrofisica, Istituto di Radio Astronomia, Via Piero Gobetti 101, I-40129 Bologna, Italy
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Abstract
It is thought that the chiral molecules of living material can induce circular polarization in light at levels much higher than expected from abiotic processes. We therefore obtained high quality imaging circular polarimetry of the martian surface during the favorable opposition of 2003 to seek evidence of anomalous optical activity. We used two narrow-band filters covering 43% of the martian surface, 15% of it in-depth. With polarization noise levels <0.1% (4.3 upper limits 0.2-0.3%) and spatial resolution 210 km, we did not find any regions of circular polarization. When data were averaged over the observed face of the planet, we did see a small non-zero circular polarization 0.02%, which may be due to effects associated with the opposition configuration though it is at the limit of the instrumental capability. Our observations covered only a small fraction of parameter space, so although we obtained a null result, we cannot exclude the presence of optical activity at other wavelengths, in other locations, or at higher spatial resolution.
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Miley GK, Overzier RA, Tsvetanov ZI, Bouwens RJ, Benítez N, Blakeslee JP, Ford HC, Illingworth GD, Postman M, Rosati P, Clampin M, Hartig GF, Zirm AW, Röttgering HJA, Venemans BP, Ardila DR, Bartko F, Broadhurst TJ, Brown RA, Burrows CJ, Cheng ES, Cross NJG, De Breuck C, Feldman PD, Franx M, Golimowski DA, Gronwall C, Infante L, Martel AR, Menanteau F, Meurer GR, Sirianni M, Kimble RA, Krist JE, Sparks WB, Tran HD, White RL, Zheng W. A large population of ‘Lyman-break’ galaxies in a protocluster at redshift z ≈ 4.1. Nature 2004; 427:47-50. [PMID: 14702079 DOI: 10.1038/nature02125] [Citation(s) in RCA: 99] [Impact Index Per Article: 5.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/15/2003] [Accepted: 10/09/2003] [Indexed: 11/08/2022]
Abstract
The most massive galaxies and the richest clusters are believed to have emerged from regions with the largest enhancements of mass density relative to the surrounding space. Distant radio galaxies may pinpoint the locations of the ancestors of rich clusters, because they are massive systems associated with 'overdensities' of galaxies that are bright in the Lyman-alpha line of hydrogen. A powerful technique for detecting high-redshift galaxies is to search for the characteristic 'Lyman break' feature in the galaxy colour, at wavelengths just shortwards of Lyalpha, which is due to absorption of radiation from the galaxy by the intervening intergalactic medium. Here we report multicolour imaging of the most distant candidate protocluster, TN J1338-1942 at a redshift z approximately 4.1. We find a large number of objects with the characteristic colours of galaxies at that redshift, and we show that this excess is concentrated around the targeted dominant radio galaxy. Our data therefore indicate that TN J1338-1942 is indeed the most distant cluster progenitor of a rich local cluster, and that galaxy clusters began forming when the Universe was only ten per cent of its present age.
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Affiliation(s)
- George K Miley
- Leiden Observatory, University of Leiden, PO Box 9513, Leiden, 2300 RA, The Netherlands.
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Bond HE, Henden A, Levay ZG, Panagia N, Sparks WB, Starrfield S, Wagner RM, Corradi RLM, Munari U. An energetic stellar outburst accompanied by circumstellar light echoes. Nature 2003; 422:405-8. [PMID: 12660776 DOI: 10.1038/nature01508] [Citation(s) in RCA: 179] [Impact Index Per Article: 8.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/26/2002] [Accepted: 02/18/2003] [Indexed: 11/09/2022]
Abstract
Some classes of stars, including novae and supernovae, undergo explosive outbursts that eject stellar material into space. In 2002, the previously unknown variable star V838 Monocerotis brightened suddenly by a factor of approximately 10(4). Unlike a supernova or nova, it did not explosively eject its outer layers; rather, it simply expanded to become a cool supergiant with a moderate-velocity stellar wind. Superluminal light echoes were discovered as light from the outburst propagated into the surrounding, pre-existing circumstellar dust. Here we report high-resolution imaging and polarimetry of those light echoes, which allow us to set direct geometric distance limits to the object. At a distance of >6 kpc, V838 Mon at its maximum brightness was temporarily the brightest star in the Milky Way. The presence of the circumstellar dust implies that previous eruptions have occurred, and spectra show it to be a binary system. When combined with the high luminosity and unusual outburst behaviour, these characteristics indicate that V838 Mon represents a hitherto unknown type of stellar outburst, for which we have no completely satisfactory physical explanation.
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Affiliation(s)
- Howard E Bond
- Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218, USA.
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