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SUBDUCTION TECTONICS, SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Will Gosnold and Shan de Silva Silva
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SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

Dec 19, 2015

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Page 1: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

SUBDUCTION TECTONICS, SUBDUCTION TECTONICS, MAGMATISM AND SURFACE MAGMATISM AND SURFACE

HEAT FLOW IN THE ANDEAN ARCHEAT FLOW IN THE ANDEAN ARC

Will Gosnold and Shan de SilvaWill Gosnold and Shan de Silva

Page 2: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

Overview

• HFD data

• Data treatment

• Characteristics of each HFD profile

• Tectonic history

• Tectonic models

Page 3: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

The Global Heat Flow Database of the International Heat Flow CommissionClick on the globe to enter

                                                                                                                                           

                                                     Global Heat Flow ( mW m^2) : 0-40 violet, 40-80 blue,

80-120 green, 120-240 yellow, 240+ red

www.heatflow.und.edu

Page 4: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

Continents and Oceans

 Africaxls or ASCII

 Asiaxls or ASCII

Antarctica Australia

xls or ASCII

 North America

xls or ASCIIGlobal in RTF format

Europexls or ASCII

South America

xls or ASCII

  Eastern North Pacific

Western North Pacific

Western South Pacific

 

 Continental Data

xls or ASCII

Eastern South Pacific

 North Atlantic Ocean

xls or ASCII

Indian Ocean

 Mediterranean area seas

Oceanic References

  Marine Data

xls or ASCII

www.heatflow.und.edu

Page 6: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

Residual Heat Flow Density contour map of South America (Hamza et al., 2005)

Page 7: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

Locations of active volcanoes (red triangles) and heat flow sites in South America. Light blue sites are in low-angle subduction area; purple sites are in the high angle subduction area.

Page 8: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.
Page 9: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.
Page 10: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

0

50

100

150

200

250

300

350

400

0 1000 2000 3000 4000 5000 6000

Distance (km)

mW

m-2

Unsmoothed HFD

Smoothed HFD

The data were smoothed using a 10-point running mean of heat flow density vs. distance from the volcanic front.

Page 11: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

Andes heat flow vs. distance

0

20

40

60

80

100

120

140

160

180

0 1000 2000 3000 4000 5000 6000

Distance from coast

In the Andes region of steep subduction, HFD increases sharply to >250 mW m-2 at the volcanic front and the high HFD region extends about 200 km behind the VF. At 300 km behind the VF, HFD has declined to 60 mW m-2. HFD is relatively stable in the back arc basins as well as in Precambrian regions to the east, with values in the range of 60 to 80 mW m-2.

Page 12: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

In the Andes region with sub-horizontal subduction, the transition from magmatic arc to craton is indistinguishable from normal crustal HFD variability due to age and radioactive heat production.

0

10

20

30

40

50

60

70

80

90

100

0 500 1000 1500 2000 2500 3000 3500 4000 4500 5000

Distance (km)

Page 13: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

• The zone of high HFD is about 300 km wide in the steeply subducting section of the Andean arc and <100 km wide in the Cascade arc. HFD variability in the flat subduction zone is indistinguishable from variability due to crustal age and radioactive heat production.

0

50

100

150

200

0 100 200 300 400 500 600

km

mW

m-2

Andes high angle

Andes low angle

Page 14: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.
Page 15: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

Tectonic scheme for Altiplano-Puna Volcanic Complex

• 30 ma - Crustal doubling • 13 ma – Delamination event• 10 ma – Initiation of pulsed emplacement of

upper to mid-crustal magmas which fueled eruption of at least 30,000 km3 of ignimbrites

• 10 ma – emplacement of 1,500 km3

• 8 ma – emplacement of 2,500 km3

• 6 ma – emplacement of 5,400 km3

• 4 ma – emplacement of 10,000 km3

Page 16: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

Sources of anomalously high heat flow

1. Long-period of conductive heating

2. Magmatism in middle and upper crust

Page 17: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

Temperature contours 13 my after delamination.

Magma emplacement in the upper crust is necessary to account for observed heat flow.

0 50000 100000 150000 200000 250000 300000-60000

-40000

-20000

0

0 50000 100000 150000 200000 250000 300000-60000

-40000

-20000

0

meters

meters

meters

meters

Page 18: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

0

200

400

600

800

1000

1200

1400

1600

1800

0 10 20 30 40 50 60 70

Depth (km)

Deg

C

0

10

20

30

40

50

60

70

80

90

mW

m-2

Initial Tz

Tz at present

Initial HFD profile

HFD vs depth at present

Can we detect the delamination event at 13 ma?

Page 19: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

0

200

400

600

800

1000

1200

1400

1600

1800

0 10 20 30 40 50 60 70

Depth (km)

Deg

C

0

10

20

30

40

50

60

70

80

90

mW

m-2

Initial Tz

Tz at present

Initial HFD profile

HFD vs depth at present

Can we detect the delamination event at 13 ma using surface heat flow?

Page 20: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.
Page 21: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

Plate rollback with counter flow at subduction velocity

Plate rollback with counter flow at half subduction velocity

Plate rollback with no counter flow

0 100000 200000 300000 400000 500000 600000

-150000

-100000

-50000

0

Dep

th (

m)

0 100000 200000 300000 400000 500000 600000

-150000

-100000

-50000

0

Dep

th (

m)

0 100000 200000 300000 400000 500000 600000

Distance from trench

-150000

-100000

-50000

0

Dep

th (

m)

Page 22: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

0

200

400

600

800

1000

1200

1400

0 20 40 60 80 100

Depth (km)

Deg C

Initial

8ma

6ma

4ma

Present

Page 23: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.
Page 24: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

Andes Surface HFD and Intrusion Models

Page 25: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

0

100

200

300400

500

600

700

800

0 10 20 30 40 50

Depth (km)

MP

a

Brittle yield stress

Ductile Yield Stress

Pre-eruption

Intrusion 4 Ma

Delamination

Page 26: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

0

20

40

60

80

100

120

140

0 50 100 150 200 250 300 350 400 450

Distance (km)

Cascades HFD profile

Page 27: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

Locations of active volcanoes (red triangles) and HFD sites in South America. Light blue sites are in low-angle subduction area; purple sites are in the high angle subduction area.

Page 28: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

Locations of HFD sites (purple circles) and active Volcanoes (red triangles) in Cascade range.

Page 29: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

0

50

100

150

200

0 1000 2000 3000 4000 5000

km

mW

m-2

Andes high angle

Andes low angle

Cascades

Conclusions

In all cases, the high HFD belt coincides with the zone of active volcanism and the amplitude of the HFD anomaly appears to correlate with the angle of subduction. Variable width of the high HFD zones is interpreted to be related to differences in thickness and composition of the local crust, and to the duration of subduction.

Page 30: SUBDUCTION TECTONICS, MAGMATISM AND SURFACE HEAT FLOW IN THE ANDEAN ARC Will Gosnold and Shan de Silva.

• The sharpness of changes in HFD is due to magma emplacement within the past 4 my.

• The overprint of near surface magmatism masks the thermal effects of delamination.

Special acknowledgement of volcanologist Shanaka deSilva for consultation on volcano-tectonic history.