|   Home   |   Troposphere   |   Mesosphere   |   Fieldwork   |   Laboratory   |   Modelling   |   Mars   |   Members   |

Meteor Smoke
> Mesosphere
> Laboratory
> Modelling

Iodine Particles

Calcium Chemistry

Magnesium Chemistry

UHVV ice study

Silicon Particles

Publications

Links

Field Campaign Photos

Contact Us

Laboratory studies of meteoric smoke particle (MSP) analogues

Figure 4 shows Transmission electron microscopy (TEM) images of micron-size particle aggregates produced from three distinct chemical systems of relevance to the Earth's upper atmosphere. Clearly, despite having different compositions (as identified from x-ray analysis), the particles share certain features i.e. the aggregates are comprised of large numbers of smaller particles and they have extended, fractal-like morphologies [Saunders and Plane, 2006a]. These observations hint at a likely common particle growth mechanism for such Fe-containing aerosol systems (see modelling section).


Figure 4 TEM images of fractal particle aggregates of laboratory generated meteoric smoke mimics with compositions identified as (i) Fe2O3, (ii) FeOOH and (iii) Fe2SiO4 - Figure taken with permission from Saunders and Plane, 2006a.


For each system, the particles were generated by the photo-oxidation of precursor gases in a laminar flow reactor; iron pentacarbonyl [Fe(CO)5] for the production of gas-phase Fe atoms and tetraethyl orthosilicate [TEOS] for the production of Si atoms and / or SiO molecules. Subsequent gas-phase oxidation and polymerisation reactions then lead to condensable species which undergo homogeneous nucleation to the aerosol phase (see Figure 5).


Figure 5 Possible gas-phase reaction pathways leading to the formation of meteoric smoke mimics with end compositions as identified in TEM analysis. Proposed polymerisation reactions leading to structural re-arrangement in the solid-phase to form the minerals hematite (Fe2O3), goethite (FeOOH) and fayalite (Fe2SiO4) are indicated by dashed arrows - Figure taken with permission from Saunders and Plane, 2006a.


Particle sampling onto TEM grids allowed for subsequent imaging and analysis as described above. Time-resolved particle size distributions were measured using a scanning mobility particle sizer (SMPS) instrument. Also, generated particles were passed into a multi-pass (White) absorption cell and the particle light extinction spectra recorded [Saunders and Plane, 2006c].

 

 

Leverhulme Trust Award 2011

 

We have recently received funding from the Leverhulme Trust for a 3 year project – ‘Lab-on-a-chip synthesis of cosmic dust analogues’.

 

The objective of the project is to efficiently synthesise (at low cost) and study the properties of nanoparticles with realistic composition (metal oxides, carbonates and silicates) and size (< 100 nm) as analogues for cosmic dust particles formed in the atmospheres of the inner planets Earth, Venus and Mars, of Titan and also in the interstellar medium (ISM).

 

The diagram below indicates the three main experimental phases required to meet the project objectives. The first phase involves the novel application of the microfluidics or Lab-on-a-chip (LOC) technique. This will provide a miniaturised ‘bottom-up’ pathway to the controlled formation of monodisperse nanofluids – solutions of the target nanoparticles. Phase two is the dip-coating of the nanofluids followed by evaporation and drying stages to form thin nanolayered substrates. The final phase is the Knudsen cell study of relevant vapour uptake/interactions with the nanolayered substrates to elucidate critical parameters such as uptake coefficient (γ), and to characterise resulting surface modifications.

 

Leverhulme_schematic.png

 

Target vapour-particle interactions include H2SO4 (Earth/Venus), CO2 (Mars) and organics (Titan). In addition we plan to study the catalysis of CO2 formation from CO and O2, of relevance to the atmosphere of Venus and the catalytic role of nanoparticles in the formation of species including H2, H2O and CO in the ISM.

 

We also plan to use the nanolayered substrates for FT-IR determination of the refractive indices of the target nanoparticles.

 

References

Saunders, R.W., and J.M.C. Plane (2006a) Inorganic aerosol formation and growth in the Earth's lower and upper atmosphere. J. Phys. IV France, 139, 243.
Saunders, R.W., and J.M.C. Plane (2006c) A laboratory study of meteor smoke analogues: composition, optical properties and growth kinetics. J. Atmos. Solar-Terr. Phys., vol 68, page 2182.

For information related to this project
Go to > Mesospheric importance > Modelling work