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X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon...

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X-ray Expeditions into Geosciences and Mining Geosciences Applications of EDS and µ-XRF Bruker Nano GmbH, Berlin Webinar, April25 th , 2012 Innovation with Integrity
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Page 1: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

X-ray Expeditions into Geosciences and Mining Geosciences Applications of EDS and µ-XRF Bruker Nano GmbH, Berlin Webinar, April25th, 2012

Innovation with Integrity

Page 2: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

Webinar Overview

Part I

Advanced EDS analysis options for geoscience applications using SDD on SEM

Part II

Geological applications of the M4 TORNADO µ-XRF spectrometer

Page 3: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

Advanced EDS Analysis Options for Geoscience Applications using SDD

Dr. Tobias Salge, EDS Application Scientist, Bruker Nano GmbH, Berlin

Page 4: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 4

State-of-the-art XFlash® silicon drift detectors (SDD)

• Energy resolution 121 eV (FWHM Mn Kα)

• Best energy resolution range up to 100 kcps

• Multi detector option

QUANTAX EDS system for SEM, EPMA and TEM

Page 5: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 5

Overview

• Fast, high resolution mapping Display of small features

• Spectrum imaging Improved element identification Quantitative analysis of REE by peak deconvolution Modal analysis

• Computer-controlled SEM High resolution at the macroscale Particle search using feature analysis

• Application examples Earth and planetary samples Core samples of impactites at the K-Pg boundary Mining samples focussing on REE, iron oxides

Page 6: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 6

OPD leg 207 (4000 km from crater)

Chicxulub impact structure • ~Ø 180 km, ~65 Ma • Target rock:

silicate basement, 3 km sediments

• Release of SOx, CO2, H2O

K-Pg boundary Asteroid impact and mass extinction

Image of NASA Worldwind

Chicxulub crater

Yax-1 UNAM-7

Page 7: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 7

Schulte et al. 2009

Thin section

K-Pg transition at OPD leg 207 2 cm ejecta spherule deposit

Page 8: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 8

Schulte et al. 2010, Science, 327, 1214-1218

Dolomite spherule with layered clay shell indicates impact-induced mechanical and thermal stress.

ODP leg 207, High-resolution map 4072x3072 pixel, 30 min, 500 kcps

Page 9: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 9

Spectrum Imaging HyperMap

Page 10: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 10

Spectrum Imaging HyperMap

Page 11: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 11

Spectrum Imaging HyperMap

Page 12: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 12

• Synthetic spectrum of highest count level found in each spectrum channel

• Detection of trace elements present in one pixel

MaxPixSpec reveals the presence of Th, La, Ce, …

Granite 200 µm

Element Identification Maximum Pixel Spectrum vs. Sum Spectrum

Page 13: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 13

Ce

Monazite (La, Ce, Nd, Pr…)PO4

MaxPixSpec reveals the presence of Th, La, Ce, …

200 µm

wt.%

Element Identification Maximum Pixel Spectrum vs. Sum Spectrum

• Synthetic spectrum of highest count level found in each spectrum channel

• Detection of elements present in a few pixels only

Granite

Page 14: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 14

How far can we take peak deconvolution? Diagenetic monazite concretion

Page 15: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 15

Peak intensity map

Intensity map and area spectra display zonation.

Area spectra

La Gd 300 µm

How far can we take peak deconvolution? Diagenetic monazite concretion

Page 16: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 16

Peak intensity map

Overlapping element lines lead to wrong display of element distribution.

Gd 300 µm

How far can we take peak deconvolution? Diagenetic monazite concretion

Area spectra

Page 17: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 17

>5.1

4.7

3.5

2.4

1.2

0.0

wt.% Quantitative map Deconvolution result

• Overlapping peaks can be deconvolved • Quantitative map displays correct element distribution

Gd 300 µm

How far can we take peak deconvolution? Diagenetic monazite concretion

Page 18: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 18

• Concentration of Gd, Sm, Nd within the core • Sequential incorporation of LREE • La dominating the outermost rim

Line scan (wt.%) extracted from quantitative map:

How far can we take peak deconvolution? Diagenetic monazite concretion

Page 19: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 19

Salge et al. 2007

BSE

Microcrystalline breccia matrix Core: UNAM-7 381.4 m

Modal analysis Chemical phase mapping UNAM-7

Matrix

Matrix

Matrix

1 cm

Anh

80 µm

Page 20: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 20

80 µm Salge et al. 2008

Autophase result

Modal analysis Chemical phase mapping

Core: UNAM-7 381.4 m

UNAM-7

Matrix

Matrix

Matrix

1 cm

Anh

Page 21: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 21

80 µm

Modal content

Phase Area fraction (%)

Anhydrite 51.8

Dolomite 30.6

Calcite 14.9

K-feldspar 1.0

Celestine 0.7

Na-feldspar 0.5

Modal analysis Chemical phase mapping

Core: UNAM-7 381.4 m

Salge et al. 2008

UNAM-7

Matrix

Matrix

Matrix

1 cm

Anh

Page 22: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 22

Computer-controlled SEM Jobs – StageControl

Page 23: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 23

Yax-1 core: Unit 5 861.72m

Composite of 276 maps • 2 µm pixel resolution • 11,906 x 11,595 pixel • ICR: 450,000 cps • 20 kV, 18 nA, 18 h

(4 min per single map) 5 mm

Matrix Melt rock 1 cm

High resolution at the macroscale 140 megapixel map

Yax-1

Nelson et al. (in press, available online at GCA)

Page 24: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 24

5 mm

Matrix Melt rock

Next image

Yax-1 core: Unit 5 861.72m

Composite of 276 maps • 2 µm pixel resolution • 11,906 x 11,595 pixel • ICR: 450,000 cps • 20 kV, 18 nA, 18 h

(4 min per single map)

1 cm

High resolution at the macroscale 140 megapixel map

Yax-1

Nelson et al. (in press, available online at GCA)

Page 25: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 25

1 mm

• Crystallized impact melt material with hydrothermal overprint.

• Multiple fracturing events due to interaction of hot fluids with solidified melts.

Impact melt Matrix

Impact melt

Matrix

K-metasomatism Multiple fracturing events

Yax-1

Page 26: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 26

Particle detection and classification Feature analysis

1. Particle detection

2. Chemistry: Chemical classification

3. Review: Reclassification

Page 27: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27

Particle detection and classification Feature analysis

Morphological classification dialog: Binarization

27.04.2012

Page 28: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

28

Particle detection and classification Feature analysis

2. Chemical classification

27.04.2012

Page 29: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 29

Descrimination of calcite and flourite Feature analysis

Class Count Area fraction (%) Fluorite CaF2 130 9.2 Ca-carbonate CaCO3 4 2.3 Unclassified 482 68.5 All 616 100

20 kV, 60 kcps, 0.5 s

Composite of 14 BSE images

Page 30: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012

Altered laterite Classification of monazite and pyrochlore

Bariopyrochlore Ba0.3Sr0.2Ca0.1Nb1.8Ti0.2O5.6(H2O)0.8

Plumbopyrochlore Pb0.8Y0.2U0.1Ca0.1Nb1.4Si0.2Fe2+0.2Ta0.1O6.2(OH)0.5

Zirconolite Ca0.8Ce0.2ZrTi1.5Fe2+0.3Nb0.1Al0.1O7

Hollandite Ba0.8Pb0.2Na0.1Mn4+

6.1Fe3+1.3Mn2+

0.5Al0.2Si0.1O16

Composite of 64 BSE images

30

Page 31: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012

Pyrochlore Deconvolution of overlapping peaks

2.90 3.00 3.10 3.20 3.30 3.40 3.50 3.60 3.703.80keV

0.0

0.5

1.0

1.5

2.0

2.5

3.0

3.5

4.0

cps/eV

Ca

U

Th

1.80 2.00 2.20 2.40 2.60keV

0

20

40

60

80

100

120

cps/eV

Sr Pb Zr

Nb Ta

4.2 4.4 4.6 4.8 5.0 5.2 5.4 5.6 5.8 6.0 6.2 6.4 6.6keV

0

2

4

6

8

10

12

14

16

18

20

22

24 cps/eV

Ti

Ba

Ce

Fe

Pyrochlore spectrum XFlash® 5030, 20 kV, 90-120 kcps, 3 s

31

Page 32: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 32

Classification Standardless quantification

Class Count Monazite Nd>8 wt.% 123 Monazite La>18 wt.% 551 Monazite 669 Baryte 32 Hollandite 22 Plumbopyrochlore 15 Bariopyrochlore 20

Zirconolite 2 Unclassified 43 All 1477

Page 33: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 33

Classification of monazite Composition

• An exchange of neodynium with lanthanum is present.

Ce versus Nd

0,00,0

3,0

1,2

5,9

2,5

8,9

3,7

11,8

4,9

14,8

6,2

17,8

7,4

20,7

8,7

23,7

9,9

26,6

11,1

29,6

12,4

Ce

Nd

Ce versus Nd 12.4

11.1

9.9

8.7

7.4

6.2

4.9

3.7

2.5

1.2

0.0

Nd

(wt.

%)

0.0 3.0 5.9 8.9 11.8

14.8 17.8 20.7 13.7 29.6

Ce (wt.%) 26.6

La versus Nd La versus Nd

0,00,0

2,3

1,2

4,5

2,5

6,8

3,7

9,0

4,9

11,3

6,2

13,5

7,4

15,8

8,7

18,0

9,9

20,3

11,1

22,5

12,4

La

Nd

0.0 2.3 4.5 6.8 9.0 11.3 13.5 15.8 18.0 22.5

La (wt.%)

12.4

11.1

9.9

8.7

7.4

6.2

4.9

3.7

2.5

1.2

0.0

Nd

(wt.

%)

20.3

La versus Nd

Page 34: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

La-Monazite Monazite Nd-Monazite

Page 35: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 35

Iron oxides Fast quantification using a standard

Haematite Fe2O3

N=10 Expected (at.-%)

Mean (at.-%)

s (±at.-%)

O 60.0 60.0 0.5 Fe 40.0 40.0 0.5 Magnetite Fe3O4

N=10

Expected (at.-%)

Mean (at.-%)

s (±at.-%)

O 57.1 56.9 1.0 Fe 42.9 43.1 1.0

EDX detector: XFlash® 5040 QUAD HV: 15 kV Current: 142.6 nA

Haematite Fe2O3 and Magnetite Fe3O4 • Standard-based quantification is

required to obtain highest accuracy.

• Haematite was used for reference.

• Using high count rates, iron oxides can be discriminated in a short time.

Count rate (In/Out): 900/675 kcps Time reference/sample: 120/30 ms Counts per spectrum: 20000 – 25000

Page 36: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 36

BSE image of iron ore pellet Area spectra

Spectrum imaging of iron oxides Advanced analysis options

Silicate

Haematite Magnetite

Page 37: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 37

Autophase result

Spectrum Imaging of Iron Oxides Autophase

Magnetite / Haematite = 9.4

Class Area fraction (%) Magnetite 86.3 Haematite 9.2 Silicate 3.3 Unassigned 1.2 Total 100.0

Page 38: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 38

Magnetite

Classification of iron oxides Feature analysis

Haematite

Ti-Haematite Ti-Magnetite

BSE image of iron ore pellet 15 kV, ~450 kcps, 0.5 s

Page 39: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 39

Quantification with hybrid method Standardless with reference for Fe and O

Magnetite / Haematite = 9.6 (Autophase 9.4)

Class Count Area fraction (%) Ti-Magnetite 2 0,1 Magnetite 540 79,7 Ti-Haematite 2 0,1 Haematite 57 8,3 Quartz 3 0,6 Olivine 11 1,6 Na-feldspar 4 5,6 Alumosilicate 3 0,1 Calcium pyroxene 1 0,1 Apatite 2 2,1 Calcium carbonate 2 0,3 Unclassified 26 1,4 All 653 100,0

Page 40: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 40

Summary

• State-of-the-art XFlash® SDD technology enables fast mapping

• Spectrum imaging significantly enhances EDS analysis

• Deconvolution is an important tool for element identification and quantification

• Computer-controlled acquisition provides high resolution at the macroscale

• Feature analysis combines morphological and chemical classification

• Hybrid method combines standardless and standard-based quantification

Page 41: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

Geological Applications of the M4 TORNADO µ-XRF Spectrometer

Dr. Roald Tagle, µ-XRF Application Scientist, Bruker Nano GmbH, Berlin

Page 42: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

A technological alliance From electron to X-ray excitation

µ-XRF ARTAX EDS QUANTAX

High speed µ-XRF spectrometer

27.04.2012 42

Page 43: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 43

The M4 TORNADO Spatially resolved µ-X-ray spectroscopy

Page 44: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 44

The M4 TORNADO Focusing X-rays with a polycapillary lens

10 mm

23 µm for 17,5 keV

Poly-capillary lens collects large angle of tube radiation and concentrates it into a small spot on the sample

Focusing X-rays

Page 45: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

45

The M4 TORNADO Instrument specifications

SDD 30 mm2, <145 eV FWHM

Key Features

• High brilliance X-ray source with small spot

• Video microscope for sample positioning with 10X and 100X magnification

• SDD technology offering high count rate capability in combination with optimum energy resolution

• Large vacuum chamber, 20 mbar in 120 s

• Powerful high speed servo motors, for samples up to 5 kg

27.04.2012

Page 46: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 46

Comparison µ-XRF & electron excitation High sensitivity for heavy elements

• Spectra of NIST 612 with approx. 500 ppm of more than 20 elements, EPMA (blue) and µ-XRF (red)

• Different excitation probability, therefore higher sensitivity for heavy elements

Page 47: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

47

Features and applications examples of the M4 Tornado in geology

• Qualitative and quantitative analyses of large samples, up to 30 X 15 cm and 5 kg, without previous preparation

Element distribution in sediments (K/Pg-boundary)

Documenting thin sections (large area scan)

Composition of the unique Dermbach meteorite

(HyperMap quantification)

• Quantitative analysis for mayor and trace elements, down to the low ppm range

Composition of volcanic glasses

27.04.2012

Page 48: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

27.04.2012 48

Raton Basin continental K/Pg sites

Chicxulub impact structure • ~Ø 180 km, ~65 Ma • Target rock:

silicate basement, 3 km sediments

K-Pg boundary Asteroid impact and mass extinction

Image of NASA Worldwind

Chicxulub crater

Yax-1 UNAM-7

Page 49: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

Scan of the Cretaceous / Paleogene boundary in Raton Basin US

Optimized for trace elements Overview measurement

5 mm

Ca Al Cr Cr Cr/Si Zr/Si Ni/Si

Pg K

27.04.2012 49

Page 50: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

Scanning thin sections

Conditions: 35 keV 800 µA, 5 ms per pixel 100 µm step size

Document thin sections or samples in a short time e.g. ~ 30 minutes per section up to 18 at the same time!

Results can be saved in independent files.

27.04.2012 50

Page 51: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

Independently saved section results

27.04.2012 51

Page 52: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

Qualitative and quantitative analysis of the unique Dermbach iron meteorite

The HyperMap feature allows an optimal “data mining”! Not only compositional overview for recognition of characteristic areas but also quantification of selected regions

The Dermbach meteorite was found in Germany in 1924.The Fe-Ni phase contains one of the highest Ni-concentrations described in literature

Bartoschewitz et al (2012). LPSC. Abs 1292

Conditions: 50 keV 200 µA, 5 ms per pixel 60 µm step size 974 x 883 Pixel 2 h measuring time

27.04.2012 52

Page 53: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

Results • The high Ni concentrations were

confirmed. A strong fractionation of the Fe-Ni-metal with a low-Ni rim could be found in the sample

• The Ni increase correlates with the Cu increase in the Fe-Ni metal

Qualitative and quantitative analysis of the unique Dermbach iron meteorite

Fe Co Ni Cu Ni-low 1 70.2 1.11 28.5 0.22 Ni-low 2 65.0 1.08 33.6 0.29 Ni-high 1 58.8 0.96 40.4 0.44 Ni-high 2 55.8 0.95 42.7 0.48

27.04.2012 53

Page 54: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

Quantitative analysis of major and trace elements in volcanic glass

The quantification was performed using the M4 standardless quantification routine. 35 kV, 750 µA, 60 s Al/Ti/Cu-filter

Ga ~20 ppm Sr from 30 to 120 ppm

27.04.2012 54

Page 55: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

Summary

• Unique speed and performance in the determination of the element distribution in large sample with measurement times per pixel of 0.3 ms and up to 4 Million pixels in a single HyperMap

• High spatial resolution down to 25 µm X-ray spot size, motors steps of 4 µm

• Optimal for the analysis of inhomogeneous samples, due to better identification of the representative location of interest

• Non-destructive, fast analysis of large samples without preparation, including solid, powder or liquid samples

• Qualitative and quantitative analysis of all elements from Na upwards, due to vacuum chamber, detection limit for heavy trace elements in the low ppm range

• Standardless Fundamental Parameter quantification with type calibration option

• Powerful software with multiple tools for optimal data mining

27.04.2012 55

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Geozentrum Nordbayern P. Schulte

Museum of Natural History, HU Berlin

D. Stöffler, P. Claeys, L. Hecht

Universidad Nacional Autónoma

de México J. Urrutia- Fucugauchi

Institute of Meteoritics, University of New Mexico H. Newsom

Institute for Planetology,

WWU Münster A. Deutsch

Natural History Museum London

A. Kearsley

International Continental Scientific

Drilling Program

Ocean Drilling Program

Page 57: X-ray Expeditions into Geosciences and Mining · 27.04.2012 4 State-of-the-art XFlash® silicon drift detectors (SDD) •Energy resolution 121 eV (FWHM Mn Kα) •Best energy resolution

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