| 1. |
- Fray, Nicolas, et al.
(författare)
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High-molecular-weight organic matter in the particles of comet 67P/Churyumov–Gerasimenko
- 2016
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Ingår i: Nature. - : Nature Publishing Group. - 0028-0836 .- 1476-4687. ; 538:7623, s. 72-74
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Tidskriftsartikel (refereegranskat)abstract
- The presence of solid carbonaceous matter in cometary dust was established by the detection of elements such as carbon, hydrogen, oxygen and nitrogen in particles from comet 1P/Halley1, 2. Such matter is generally thought to have originated in the interstellar medium3, but it might have formed in the solar nebula—the cloud of gas and dust that was left over after the Sun formed4. This solid carbonaceous material cannot be observed from Earth, so it has eluded unambiguous characterization5. Many gaseous organic molecules, however, have been observed6, 7, 8, 9; they come mostly from the sublimation of ices at the surface or in the subsurface of cometary nuclei8. These ices could have been formed from material inherited from the interstellar medium that suffered little processing in the solar nebula10. Here we report the in situ detection of solid organic matter in the dust particles emitted by comet 67P/Churyumov–Gerasimenko; the carbon in this organic material is bound in very large macromolecular compounds, analogous to the insoluble organic matter found in the carbonaceous chondrite meteorites11, 12. The organic matter in meteorites might have formed in the interstellar medium and/or the solar nebula, but was almost certainly modified in the meteorites’ parent bodies11. We conclude that the observed cometary carbonaceous solid matter could have the same origin as the meteoritic insoluble organic matter, but suffered less modification before and/or after being incorporated into the comet.
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| 2. |
- Janhunen, Pekka, et al.
(författare)
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Biological Feedbacks as Cause and Demise of Neoproterozoic Icehouse : Astrobiological Prospects for Faster Evolution and Importance of Cold Conditions
- 2007
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Ingår i: PLOS ONE. - : Public Library of Science (PLoS). - 1932-6203. ; 2:2, s. e214-
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Tidskriftsartikel (refereegranskat)abstract
- Several severe glaciations occurred during the Neoproterozoic eon, and especially near its end in the Cryogenian period (630-850 Ma). While the glacial periods themselves were probably related to the continental positions being appropriate for glaciation, the general coldness of the Neoproterozoic and Cryogenian as a whole lacks specific explanation. The Cryogenian was immediately followed by the Ediacaran biota and Cambrian Metazoan, thus understanding the climate-biosphere interactions around the Cryogenian period is central to understanding the development of complex multicellular life in general. Here we present a feedback mechanism between growth of eukaryotic algal phytoplankton and climate which explains how the Earth system gradually entered the Cryogenian icehouse from the warm Mesoproterozoic greenhouse. The more abrupt termination of the Cryogenian is explained by the increase in gaseous carbon release caused by the more complex planktonic and benthic foodwebs and enhanced by a diversification of metazoan zooplankton and benthic animals. The increased ecosystem complexity caused a decrease in organic carbon burial rate, breaking the algal-climatic feedback loop of the earlier Neoproterozoic eon. Prior to the Neoproterozoic eon, eukaryotic evolution took place in a slow timescale regulated by interior cooling of the Earth and solar brightening. Evolution could have proceeded faster had these geophysical processes been faster. Thus, complex life could theoretically also be found around stars that are more massive than the Sun and have main sequence life shorter than 10 Ga. We also suggest that snow and glaciers are, in a statistical sense, important markers for conditions that may possibly promote the development of complex life on extrasolar planets.
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| 3. |
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| 4. |
- Eriksson, Mats, et al.
(författare)
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On the use of MnO2 cartridges for the plutonium determination in seawater
- 2019
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Ingår i: Journal of Environmental Radioactivity. - : ELSEVIER SCI LTD. - 0265-931X .- 1879-1700. ; 204, s. 66-75
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Tidskriftsartikel (refereegranskat)abstract
- To analyze plutonium (Pu) in open ocean waters can be challenging due to the low seawater concentrations. In this study we compared two techniques for Pu determination, one in-situ MnO2 cartridge system and the more commonly used MnO2 precipitation technique. During the pre-pilot GEOTRACES cruise ANT XXX-1 (2005) we tested MnO2 cartridges for the pre-concentration of Pu from seawater at 19 sampling stations on a transect in the southeastern Atlantic Ocean between Vigo (Spain) and Cape Town (South Africa). Our in-situ sampling setup consisted of one particle cartridge followed by three MnO2 cartridges in a series. Through the system we pumped between 956 and 2700 I of surface seawater with a flow rate between 1.6 and 5.21/min. We found that the adsorption efficiency of a single MnO2 cartridge to adsorb Pu was rather constant and on average a 58 +/- 7%. The adsorption efficiency was also found to be independent of seawater: temperature in the range of 18.3-29.2 degrees C, salinity range 34.2-37.1 parts per thousand, and conductivity in the range of 46.8-58.4 mS/cm. In parallel with the in-situ sampling, discrete surface water samples between 259 and 281 I were taken and Pu was pre-concentrated using the MnO2 precipitation method. We find a good agreement between the Pu concentrations determined with the two different techniques. The in-situ pre-concentration technique requires more radiochemical work in the laboratory but has the advantage that large seawater volumes can be sampled without the necessity for radiochemical processing on-board the ship. The much larger volumes sampled with the in-situ technique compared with the precipitation technique, enables accurate determination of Pu-isotopic ratios with a low relative standard deviation. We have shown in this study that in-situ MnO2 cartridge technique can be used in a reliable way for the determination of dissolved Pu seawater concentration in open ocean waters.
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| 5. |
- Tammi, Markku, et al.
(författare)
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EGF regulates HAS-2 expression, controls epidermal thickness and stimulates keratinocyte migration
- 2002
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Ingår i: Hyaluronan, Vol 1: Chemical, Biochemical and Biological Aspects. - Great Britain : Woodhead Publishing Limited. - 1855735709 ; , s. 561-570
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Konferensbidrag (refereegranskat)abstract
- High concentrations of hyaluronan reside in the small space between the vital kertinocyte layers of human and animal epidermis and influence keratinocyte interactions, including growth, mobility and differentiation. We have previously found that the content of epidermal hyaluronan in human skin organ cultures is decreased and increased by cortisol and retinoic acid, and associated with enhanced and retarded terminal differentiation, respectively. To further substantiate this idea, we incubated epidermal keratinocytes with epidermal growth factor (EGF), and found a marked increase in hyaluronan synthesis which correlated with faster migration in an in vitro wounding assay of keratinocyte monolayers. EGF increased hyaluronan also in stratified, differentiated organotypic cultures, and increased the height of vital epidermis and reduced the thickness of the cornified layers, findings in line with an inhibition of terminal differentiation of keratinocytes. The stimulation of hyaluronan synthesis by EGF was due to upregulation of hyaluronan synthase 2 (HAS2) but not HAS1 or HAS3. A part of the EGF influence on the structure of epidermis, and on skin wound healing, is thus mediated through its control of HAS2 expression.
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