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PHOTON AND WATER MEDIATED SULFUR OXIDE AND ACID CHEMISTRY IN THE ATMOSPHERE OF VENUS Jay A. Kroll , Veronica Vaida Department of Chemistry and Biochemistry University of Colorado - Boulder June 20, 2014 Photo Credit: J. Gabás Esteban

PHOTON AND WATER MEDIATED SULFUR OXIDE AND ACID CHEMISTRY IN THE ATMOSPHERE OF VENUS Jay A. Kroll, Veronica Vaida Department of Chemistry and Biochemistry

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PHOTON AND WATER MEDIATED SULFUR OXIDE AND ACID CHEMISTRY IN

THE ATMOSPHERE OF VENUS

Jay A. Kroll, Veronica Vaida Department of Chemistry and Biochemistry

University of Colorado - BoulderJune 20, 2014

Photo Credit: J. Gabás Esteban

• Sulfur compounds have been observed on a number of planetary bodies.

Background/Motivation

Photo credit: ESA

Venus Earth Mars

Io EuropaCallisto

Background/Motivation• Sulfur compounds have

been observed on a number of planetary bodies.

• Venus– Sulfuric acid clouds 50-70 km

http://nssdc.gsfc.nasa.gov/image/planetary/venus/pvo_uv_790226.jpg

Background/Motivation

Belyaev et al. Icarus, Volume 217, Issue 2, 2012, 740 - 751

Mixing Ratio (ppmv)

Altit

ude

(km

)

SO2

SO

• Sulfur compounds have been observed on a number of planetary bodies.

• Venus– Sulfuric acid clouds 50-70 km

– Increase in SO2 at 90 km

– Exceeds model predictions by orders of magnitude

Background/Motivation

Belyaev et al. Icarus, Volume 217, Issue 2, 2012, 740 - 751

Mixing Ratio (ppmv)

Altit

ude

(km

)

SO2

SO

• Sulfur compounds have been observed on a number of planetary bodies.

• Venus– Sulfuric acid clouds 50-70 km

– Increase in SO2 at 90 km

– Exceeds model predictions by orders of magnitude

– Requires a chemical source of SO2 in the middle atmosphere

• UV photolysis of H2SO4

UV Photolysis?

H2SO4 + UV SO3+H2O SO3 + UV SO2+O

• UV photolysis of H2SO4

UV Photolysis?

H2SO4 + UV SO3+H2O SO3 + UV SO2+O

Lane and Kjaergaard, J Phys. Chem A. 2008, 112, 4958-4964

180 nmSulfuric Acid Cross Section

• UV photolysis of H2SO4

UV Photolysis?

H2SO4 + UV SO3+H2O SO3 + UV SO2+O

Lane and Kjaergaard, J Phys. Chem A. 2008, 112, 4958-4964

180 nmSulfuric Acid Cross Section Spectral Actinic Flux of Venus

Zhang et al. Icarus, Volume 217, Issue 2, 2012, 714 - 739

58 km 70 km112 km

Red Light Photolysis

V=0

V=1

V=2

V=3

V=4

V=5

V=6

4v9

5v9

O-H Stretch

Feierabend et al., Chemical Physics Letters, 2006, 420, 438 - 442

Credit: Zeb Kramer

38.5 kcal/mol

47.2 kcal/mol

Feierabend et al., Chemical Physics Letters, 2006, 420, 438 - 442

Red Light Photolysis

Credit: Zeb Kramer

38.5 kcal/mol

47.2 kcal/mol

Feierabend et al., Chemical Physics Letters, 2006, 420, 438 - 442

Red Light Photolysis

Explains SO2 vertical profile on Earth

Does It Explain SO2 on Venus?

Zhang et al. Icarus, Volume 217, Issue 2, 2012, 714 - 739

•Include UV Cross Section•Debate on Effect of Water Clustering•Lab Measurements of J values are needed

Sulfuric Acid Cross Section

Sulfurous Acid

Voegele et al. (2002) “About the Stability of Sulfurous Acid and its dimer,” Chem. Eur. J. 8, 24, 5644-5651.

H2SO3 + n H2O SO2 + (n+1)H2O

New UV Spectrometer

iHR550 Spectrometer

with UV Sensitized CCD

Energetiq Laser Driven Light

Source

Glass Cell with Quartz Windows

Iris

First Test - June 2nd

+

First Test - June 2nd

+

H2O?

Recent ResultsPure SO2

Recent ResultsPure SO2 Pure Water

Recent ResultsPure SO2 Pure Water

SO2 + Water (varied)

Recent ResultsPure SO2 Pure Water

SO2 + Water (varied) Water + SO2 (varied)

Recent Results

Recent Results

Cell WindowpH~3

Clean WindowpH~7

Future Work

CRD

Nd:YAG

Dye Laser

SO2 + H2O + H2SO3H2O

Xe Arc Lamp

Future Work

CEAS

Red Photochemical

Lamp

SO3 + H2OH2SO4 +H2O

SO2 + H2OH2SO3 + H2O

Energetiq LDLS

J

J

Future Work- Experiments

Dye Laser

Nd:YAG

Energetiq LDLS

CEAS

CRD

AcknowledgementsVaida Group Members– Allison Harris, Rebecca Rapf, Russell Perkins

Steve Brown – NOAA

NSF Grant Number CHE1306386

Contact: [email protected]