lpsc 2016-presentation

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New Experimental Evidence of Silicate Formation with Meteorite Like Oxygen Isotopes on a Dust Surface Analog S ubrata Chakraborty Haiyang Kehoe and M. H. Thiemens University of California, San Diego Department of Chemistry and Biochemistry, 9500 Gilman Drive, La Jolla, CA 92093-0356

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Page 1: Lpsc 2016-presentation

New Experimental Evidence of Silicate Formation with Meteorite Like Oxygen Isotopes on a Dust Surface Analog

Subrata ChakrabortyHaiyang Kehoe and M. H. Thiemens

University of California, San DiegoDepartment of Chemistry and Biochemistry, 9500 Gilman Drive, La Jolla, CA 92093-0356

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•Dust particles are obiquitous throughout the universe•Dying stars are the ‘dust factories’ •Constitutes ~1 mass % in the ISM•As high as 10 % in planetary nebula•Dust particles are mainly of two types: carbonaceous and silicates•Long lifetime journey– stellar region through diffuse, dense or molecular clouds to the new born star or its planetary system •Significantly processed during this journey

Background

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Rational

Condensation of oxides in gas phase were theoretically calculated

Ferrarotti and Gail, AA, 2002Mg + H2O → MgO(s) + H2Fe + H2O → FeO(s) + H22Fe + 3H2O → Fe2O3(s) + 3H23Fe + 4H2O → Fe3O4(s) + 4H2

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Rational

Oxidation Reaction on the surface of an existing oxide: SiO, FeO, Al2O3 etc….

With absorbed water molecule Specifically in colder environments

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Experimental

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Experimental

Sample: Si, SiO, Al2O3…..

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Experimental

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Experimental

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Experimental

Four different sets of experiments:1.SiO vapor deposit + H2O2 vapor deposit2.SiO vapor deposit + H2O vapor deposit3.(Al2O3 + Si) vapor deposit + H2O vapor

deposit4.(Al2O3 + SiO) vapor deposit + H2O vapor

deposit

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1 mm

1.SiO Vapor Deposit + H2O2@ 150 K

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1.SiO Vapor Deposit + H2O2

Collection Plate

Side Wall- Foil

Collection Plate- Foil

Element

Atomic (%)

Si 44.2O 55.8

SiOx (<2)

Element

Atomic (%)

Si 38.9O 61.1

Element

Atomic (%)

Si 34.9O 65.1

SiO2

SiO2

@ 150 K

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SiO2

1.SiO Vapor Deposit + H2O2@ 150 K

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2. SiO Vapor Deposit + H2O @ 150 K

2 mm

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Element

Atomic (%)

Si 45.5O 54.5

Stoichiometry: SiO1.2

2. SiO Vapor Deposit + H2O @ 150 K

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Element

Atomic (%)

Si 41.8O 58.2

Stoichiometry: SiO1.4

2. SiO Vapor Deposit + H2O @ 150 K

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2. SiO Vapor Deposit + H2O @ 150 K

Oxygen Isotopes

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2. SiO Vapor Deposit + H2OTime Progression

27 Hrs

19 Hrs

5 Hrs

2.5 Hrs

1 Hr

@ 150 K

@ 300 K

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3. (Al2O3 + Si) Vapor Deposit + H2O @150 K

2 mm

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3. (Al2O3 + Si) Vapor Deposit + H2O @150 K

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3. (Al2O3 + Si) Vapor Deposit + H2O @150 K

Page 21: Lpsc 2016-presentation

3. (Al2O3 + Si) Vapor Deposit + H2O @150 K

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3. (Al2O3 + Si) Vapor Deposit + H2O @150 K

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3. (Al2O3 + Si) Vapor Deposit + H2O @150 K

Element

Atomic (%)

Si 63.8Al 9.4O 26.8

Stoichiometry: AlSi6.7O2.9

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4. (Al2O3 + SiO) Vapor Deposit + H2O @150 K

2 mm

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4. (Al2O3 + SiO) Vapor Deposit + H2O @150 K

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4. (Al2O3 + SiO) Vapor Deposit + H2O @150 K

Page 27: Lpsc 2016-presentation

4. (Al2O3 + SiO) Vapor Deposit + H2O @150 K

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4. (Al2O3 + SiO) Vapor Deposit + H2O @150 K

Element

Atomic (%)

Si 38.6Al 16.9O 44.5

Stoichiometry: AlSi2.3O2.6

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4. (Al2O3 + SiO) Vapor deposit + H2O vapor deposit

Element

Atomic (%)

Si 42.3Al 13.3O 44.4

~ 10 micron particle

Stoichiometry: AlSi3.2O3.3

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Mechanism

Duley and Millar, 1978….. Model (theoretical) for the reaction of +ve ions

with –ve charged species on oxide grain surfaces

Recombination of gas phase ions with surface O- and OH-

Explains selective depletion of Al, Ca, Cr, Ti, Mn etc…..

Page 31: Lpsc 2016-presentation

MechanismDuley and Millar, 1978….. Model (theoretical) for the reaction of +ve ions

with –ve charged species on oxide grain surfaces

Recombination of gas phase ions with surface O- and OH-

Explains selective depletion of Al, Ca, Cr, Ti, Mn etc…..Other way round….

Reaction of adsorbed species (H2O) with the host species (Si, Al etc…)

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Bikondoa et al., Nature 2006

MechanismSteps: Water adsorbs into O vacancies Dissociates into OH and H

fragments. The OH fragment is pinned at the

position of the O vacancy The H fragment attaches to

another oxygen from the bridging-O rows forming a second OH groupHypothesis:XO + OH → (XOOH)* → XOO + H

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Mechanism

Based on Marcus, 2004

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ComparisonGas Phase Reactions

Chakraborty et al., Science, 2013

Group-2H2 + O → OH + HSiO + OH → SiO2 + HOH + OH → H2O + HOH + O2 → HO2 + O SiO + HO2 → SiO2 + OH

Group 1SiO (g) + O2 → SiO2 + OSiO (g) + O → SiO2

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ComparisonGas Phase Reactions

Chakraborty et al., Science, 2013

Group 1SiO (g) + O2 → SiO2 + OSiO (g) + O → SiO2

Group-2H2 + O → OH + HSiO + OH → SiO2 + HOH + OH → H2O + HOH + O2 → HO2 + O SiO + HO2 → SiO2 + OH

Surface Reactions

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ConclusionsSurface assisted oxidation reation is a

possible mechanismEffective in the dark and cold molecular

clouds and colder parts of the solar nebula

Observed: Growth of new particles through reactions

Observed: Mass-independent oxygen isotopic compositions in the newly formed SiOx particles

Multicle element oxide grains do form in this process

Need more studies in this direction

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Page 38: Lpsc 2016-presentation

3. (Al2O3 + Si) Vapor Deposit + H2O @150 K