STRATIGRAPHY, HYDROTHERMAL ALTERATION AND PALEO-THERMAL ...theargeo.org › presentations ›...

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• Geologist Xavier Musonye •2 ND October 2016 Addis Ababa, Ethiopia STRATIGRAPHY, HYDROTHERMAL ALTERATION AND PALEO-THERMAL HISTORY OF THE OLKARIA - DOMES GEOTHERMAL FIELD, KENYA Proceedings, 6 th African Rift Geothermal Conference, Addis Ababa, Ethiopia, 31 st 8 th November 2016

Transcript of STRATIGRAPHY, HYDROTHERMAL ALTERATION AND PALEO-THERMAL ...theargeo.org › presentations ›...

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•Geologist

Xavier Musonye

•2ND October 2016

Addis Ababa, Ethiopia

STRATIGRAPHY, HYDROTHERMAL ALTERATION AND PALEO-THERMAL HISTORY OF THE OLKARIA

- DOMES GEOTHERMAL FIELD, KENYA

Proceedings, 6th African Rift Geothermal Conference,

Addis Ababa, Ethiopia, 31st – 8th November 2016

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Conclusions and recommendations

Results

Objectives of the study

Introduction

OUTLINE

Methodology

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INTRODUCTION Location map

• Located in southern

central sector of Kenyan

rift

• Other volcanic centres

also located within axial of

rift

• Olkaria, Eburru and

Menengai at production

stage

• Study focuses on Olkaria-

Domes (OW-911A, OW-

912B, OW-916 and OW-

914A)

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Olkaria geothermal field

• Surface geology

comprise of ash deposits,

pumice lapilli, pyroclasts

and comenditic lava

• Sub-surface geology

comprise of basalt,

rhyolite, tuff, trachyte,

dykes and intrusives

• Divided into seven field

• Total installed capacity of

677 MWe

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OBJECTIVES

• To review and compare stratigraphy and

hydrothermal alteration minerals

• Compare the paleo-thermal trends in the study area

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METHODOLOGY

• Samples collected at 2 m interval during drilling

• 1200-1400 samples collected in each well

• Analytical methods include:

i. Binocular microscope analysis

ii. Petrographic microscope analysis

iii.X-ray diffractometer analysis

iv.Fluid inclusion analysis

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RESULTS

Stratigraphy

• Pyroclastics 0-100 m

• Rhyolite 100-500 m

• Basalt 500-1000 m

• Trachyte 500-3000

• Tuff

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Occurrence and distribution of common alteration minerals

• Minerals found:- zeolites,

calcite, pyrite, chalcedony,

opal, quartz, epidote,

prehnite, wollastonite,

actinolite, sphene,

haematite and clays

• Low temp zeolites found

at shallow depth

• High temp minerals found

in abundance in OW-916

and OW-914A compared

to OW-912B and OW-

911A

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Paleo-thermal reconstruction

Well OW-916

• Homogenisation temp

range between 275 °C

and 305 °C- average of

282 °C

• Formation temp is 276 °C

• Formation temp,

alteration mineral temp

and fluid inclusion lie in

the same path

• System has maintained

more or less steady state

of equilibrium Mwangi (2012)

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Well OW-914A

• Homogenisation temp

range between 250 °C

and 290 °C- average of

255 °C

• Alteration mineral temp

and fluid inclusion lie in

the same path

• System has maintained

more or less steady

state of equilibrium

Musonye (2012)

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Well OW-911A

• Homogenisation temp

range between 195 °C

and 286 °C- average of

220 °C

• Formation temp is 220

°C

• Formation temp,

alteration mineral temp

and fluid inclusion lie in

the same path

• System has maintained

more or less steady

state of equilibrium Njathi, (2012)

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Well OW-912B

• Homogenisation temp

at 756 m is between

160 °C and 200 °C-

average of 175 °C

• At 1456 m is between

250 °C and 300 °C-

average of 260 °C

• Formation temp is 280

°C

• Formation temp,

alteration mineral temp

and fluid inclusion lie in

the same path Ronoh, (2012)

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CONCLUSIONS AND RECOMMENDATIONS

Conclusion

• The stratigraphy comprises of five lithological units;

pyroclastics, rhyolite, tuff, basalt and trachyte.

• High temp alteration minerals are noted at shallower

depth at the region of wells OW-916 and OW-914A.

• Well OW-912B recorded the greatest depth at which

high temperature alteration mineral were observed

• Area around wells OW-916 and OW-914A has the heat

closer to the surface

• Temp curves shows that the system has maintained a

steady state of thermal equilibrium over time

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Recommendations

• More fluid inclusion studies need to be done in wells

drilled in Domes area in order to get a detailed picture of

the temperature variation in the whole of the Domes field

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THANKS