scholarly journals Aqueous Alteration on Asteroids Simplifies Soluble Organic Matter Mixtures

2021 ◽  
Vol 920 (2) ◽  
pp. L39
Author(s):  
Junko Isa ◽  
François-régis Orthous-Daunay ◽  
Pierre Beck ◽  
Christopher D. K. Herd ◽  
Veronique Vuitton ◽  
...  
Keyword(s):  
Organic Matter ◽  
Soluble Organic Matter ◽  
Aqueous Alteration

scholarly journals Exploring the link between molecular cloud ices and chondritic organic matter in laboratory

2021 ◽  
Vol 12 (1) ◽  
Author(s):  
G. Danger ◽  
V. Vinogradoff ◽  
M. Matzka ◽  
J-C. Viennet ◽  
L. Remusat ◽  
...  
Keyword(s):  
Organic Matter ◽  
Molecular Clouds ◽  
Solar Nebula ◽  
High Resolution Mass Spectrometry ◽  
Soluble Organic Matter ◽  
Aqueous Alteration ◽  
Murchison Meteorite ◽  
Disk Material ◽  
C And N ◽  
Molecular Compounds

AbstractCarbonaceous meteorites are fragments of asteroids rich in organic material. In the forming solar nebula, parent bodies may have accreted organic materials resulting from the evolution of icy grains observed in dense molecular clouds. The major issues of this scenario are the secondary processes having occurred on asteroids, which may have modified the accreted matter. Here, we explore the evolution of organic analogs of protostellar/protoplanetary disk material once accreted and submitted to aqueous alteration at 150 °C. The evolution of molecular compounds during up to 100 days is monitored by high resolution mass spectrometry. We report significant evolution of the molecular families, with the decreases of H/C and N/C ratios. We find that the post-aqueous products share compositional similarities with the soluble organic matter of the Murchison meteorite. These results give a comprehensive scenario of the possible link between carbonaceous meteorites and ices of dense molecular clouds.

Pilot-plant experiments for improvement of polluted canal/klong water by rock-bed filtration

1997 ◽  
Vol 35 (8) ◽  
pp. 83-90
Author(s):  
Shigeo Fujii ◽  
Chiaki Niwa ◽  
Mitsuo Mouri ◽  
Ranjna Jindal
Keyword(s):  
Organic Matter ◽  
Pilot Plant ◽  
Horizontal Flow ◽  
Removal Mechanism ◽  
Soluble Organic Matter ◽  
Filter Media ◽  
Canal Water ◽  
Rock Bed ◽  
One Year ◽  
Filtration Technique

Applicability of the rock-bed filtration technique was investigated through pilot-plant experiments in Bangkok, Thailand. Polluted canal water was used as horizontal flow influent to two reactor channels filled with rocks. During one year operation, HRT, filter media, and aeration mode, were changed in several runs. The results showed that 1) the rock-bed filtration with aeration and the HRT more than 6 h can successfully improve polluted klong water by reducing the pollutants (e.g. 60-120mg/L of SS to 20-40 mg/L and 15-30 mg/L of BOD to 5-20 mg/L); 2) main removal mechanism seems to be the sedimentation resulting from the settleability enhanced by aeration, and the biofilm attached onto rocks also works in the reduction of soluble organic matter; 3) a combination of three rock sizes arranged in descending order showed best results; 4) longer HRT (13 h) produces better effluent but is not so effective if it exceeds 9 hours; 5) 60-70% of sediment IL was decomposed in a year, and porosity in rock beds reduced approximately 16%.

Mobility of soil water-soluble organic matter during rice cultivation

2012 ◽  
Vol 38 (1) ◽  
pp. 40-42 ◽  
Author(s):  
O. A. Gutorova ◽  
A. Kh. Sheudzhen ◽  
A. G. Ladatko
Keyword(s):  
Organic Matter ◽  
Soil Water ◽  
Rice Cultivation ◽  
Water Soluble ◽  
Soluble Organic Matter

scholarly journals Synthesis of 13C-enriched amino acids with 13C-depleted insoluble organic matter in a formose-type reaction in the early solar system

2021 ◽  
Vol 7 (18) ◽  
pp. eabd3575
Author(s):  
Yoshihiro Furukawa ◽  
Yoshinari Iwasa ◽  
Yoshito Chikaraishi
Keyword(s):  
Aqueous Solution ◽  
Organic Matter ◽  
Solar System ◽  
Acid Synthesis ◽  
Soluble Organic Matter ◽  
Early Solar System ◽  
Cold Region ◽  
Amino Acid Synthesis ◽  
Type Reaction ◽  
Insoluble Organic Matter

Solvent-soluble organic matter (SOM) in meteorites, which includes life’s building molecules, is suspected to originate from the cold region of the early solar system, on the basis of 13C enrichment in the molecules. Here, we demonstrate that the isotopic characteristics are reproducible in amino acid synthesis associated with a formose-type reaction in a heated aqueous solution. Both thermochemically driven formose-type reaction and photochemically driven formose-type reaction likely occurred in asteroids and ice-dust grains in the early solar system. Thus, the present results suggest that the formation of 13C-enriched SOM was not specific to the cold outer protosolar disk or the molecular cloud but occurred more widely in the early solar system.

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