selisa rollins mentor: dr. everett shock school of earth and space exploration

11
Selisa Rollins Mentor: Dr. Everett Shock School of Earth and Space Exploration Transport of Elements in the Yellowstone Hydrothermal System

Upload: coyne

Post on 19-Mar-2016

68 views

Category:

Documents


12 download

DESCRIPTION

Transport of Elements in the Yellowstone Hydrothermal System. Selisa Rollins Mentor: Dr. Everett Shock School of Earth and Space Exploration. Silica on Mars. Silica deposits dug up by the Spirit. Evidence of past microbial life. Hydrothermal vents are probable cause of silica enrichment. - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: Selisa Rollins Mentor: Dr. Everett Shock School of Earth and Space Exploration

Selisa RollinsMentor: Dr. Everett Shock

School of Earth and Space Exploration

Transport of Elements in the Yellowstone Hydrothermal

System

Page 2: Selisa Rollins Mentor: Dr. Everett Shock School of Earth and Space Exploration

Silica on Mars• Silica deposits dug

up by the Spirit.– Evidence of past

microbial life.• Hydrothermal

vents are probable cause of silica enrichment.

Figure 1 [1]

Page 3: Selisa Rollins Mentor: Dr. Everett Shock School of Earth and Space Exploration

Why Yellowstone?• Hydrothermal Systems:

– Excellent locations for abundant nutrient supply.

– Affect how rocks are altered.– Harbor life and determine which

microorganisms live where. – Concentrations of SiO2 are detected in

some areas.

Page 4: Selisa Rollins Mentor: Dr. Everett Shock School of Earth and Space Exploration

Hot Spring Locations and Other Present Elements

• Locations:– GOPA– Lower Geyser Basin– Sylvan Spring– Washburn

• Elements:– Antimony (Sb)– Arsenic (As)– Boron (B)– Molybdenum (Mo)– Tungsten (W)

Page 5: Selisa Rollins Mentor: Dr. Everett Shock School of Earth and Space Exploration

Strong CorrelationsSylvan Spring

0.0E+00

5.0E-06

1.0E-05

1.5E-05

2.0E-05

2.5E-05

3.0E-05

3.5E-05

4.0E-05

4.5E-05

5.0E-05

0.0E+00 2.0E-04 4.0E-04 6.0E-04 8.0E-04 1.0E-03

B (M)

As

(M)

200420052006

Page 6: Selisa Rollins Mentor: Dr. Everett Shock School of Earth and Space Exploration

Poor CorrelationsLGB

0.0E+00

5.0E-06

1.0E-05

1.5E-05

2.0E-05

2.5E-05

3.0E-05

3.5E-05

4.0E-05

4.5E-05

5.0E-05

0.0E+00 2.0E-04 4.0E-04 6.0E-04 8.0E-04 1.0E-03

B (M)

As

(M)

200420052006

Page 7: Selisa Rollins Mentor: Dr. Everett Shock School of Earth and Space Exploration

Complex CorrelationsGOPA

0.0E+00

5.0E-06

1.0E-05

1.5E-05

2.0E-05

2.5E-05

3.0E-05

3.5E-05

4.0E-05

4.5E-05

5.0E-05

0.0E+00 2.0E-04 4.0E-04 6.0E-04 8.0E-04 1.0E-03

B (M)

As

(M)

200420052006

Page 8: Selisa Rollins Mentor: Dr. Everett Shock School of Earth and Space Exploration

Observations and Summary• Molybdenum Concentrations:

– Higher at GOPA– Lower at LGB and Sylvan Springs

• Arsenic Concentrations– Lower at GOPA– Higher at LGB and Sylvan Springs

• Basic solutions present at lower elevations.• Acidic solutions present at higher

elevations.  

Page 9: Selisa Rollins Mentor: Dr. Everett Shock School of Earth and Space Exploration

Acknowledgements• Dr. Everett Shock• GEOPIG Lab:

– Tracy Lund– Jeff Havig– Mateo Hernandez– Panjai Prapaipong

Page 10: Selisa Rollins Mentor: Dr. Everett Shock School of Earth and Space Exploration

References• [1] Astronomy Now Online:

http://www.astronomynow.com/080522Spiritfindshotspring-likedepositsonMars.html

• [2] Squyres S W; Arvidson R E; Ruff S. Detection of silica-rich deposits on Mars. Science (New York, N.Y.) 2008; 320(5879): 1063-7.

Page 11: Selisa Rollins Mentor: Dr. Everett Shock School of Earth and Space Exploration

Questions?