75th meteoritical society meeting, cairns, 14 august 2012

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75th Meteoritical Society Meeting, Cairns, 14 August 2012 Northwest Africa 5738 An Extraordinarily Evolved Eucrite P. H. Warren 1 , J. Isa 1 , N. Gessler 2 , I. Ahn 3 and B-G. Choi 4 1, UCLA 2, Duke University 3, Korea Polar Research Inst. 4, Seoul National University

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Northwest Africa 5738 An Extraordinarily Evolved Eucrite P. H. Warren 1 , J. Isa 1 , N. Gessler 2 , I. Ahn 3 and B-G. Choi 4 1, UCLA 2, Duke University 3, Korea Polar Research Inst. 4, Seoul National University. - PowerPoint PPT Presentation

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Page 1: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

75th Meteoritical Society Meeting, Cairns, 14 August 2012

Northwest Africa 5738An Extraordinarily Evolved

Eucrite

P. H. Warren1, J. Isa1, N. Gessler2, I. Ahn3 and B-G. Choi4

1, UCLA 2, Duke University 3, Korea Polar Research Inst. 4, Seoul National University

Page 2: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

NWA 573822 stones found in 2009, total 2.2 kg

Page 3: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

ARTIFACT0.5 mm

NWA 5738

backscattered electron image

Page 4: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

PYROXENE COMPOSITIONS

0 10 20 30 40 50 60 70 80 90 100

50

40

30

20

10

En Fs

Di HdNWA 5738

Cumulate eucrites Moama Serra de Magé Nagaria Moore County Pomozdino

Noncumulate eucrites Y-791195 Juvinas Haraiya Nuevo Laredo

NLHJY

PMCN

SMM

Page 5: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

Mayne et al. (2009)cu

mul

ates

NWA 4523 (3 different clasts)

NWA 5738 primary plag.

Page 6: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

20

30

40

50

60

70

80

90

100

110

0 1 2 3 4 5 6bulk Na (mg/g)

bulk

Mg

(mg/

g) noncumulate cumulate

NWA 5738

Ibitira

E U C R I T E S

Page 7: 75th Meteoritical Society Meeting, Cairns, 14 August 2012
Page 8: 75th Meteoritical Society Meeting, Cairns, 14 August 2012
Page 9: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

brach

NWA 5738

Base diagrams: Mittlefehldt et al. (2008)

Analysis of bulk NWA 5738 by CO2 laser-fluorination at KOPRI (avg. of 2 similar analyses):

δ18O = 3.589‰, δ17O = 1.617‰Δ17O = ‒0.271‰

Page 10: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

NWA 5738

Base diagram: Scott et al. (2009)

Page 11: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

Base diagram: Compositions of metals from HED impact-melt breccias (within howardites; Lorentz et al., 2007)

NWA 573810 separate grains

Page 12: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

166000

168000

170000

172000

174000

176000

178000

795 800 805 810 815 820 825energy (keV)

coun

ts

Page 13: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

0

2000000

4000000

6000000

8000000

10000000

12000000

14000000

870 875 880 885 890 895 900 905energy (keV)

coun

ts

Page 14: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

10

100

Sr Ba La Ce Nd Sm Eu Tb Dy Ho Yb Lu Hf Ta Th U

REE

sam

ple/

CI c

hond

rites

(wt.

ratio

)

30NWA 5738

BouvanteStannern Trend

Juvinas'Main Group'

(literature averages)

warm-desert alteration

Page 15: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

Earth’s Continental Crustas represented by shale composites

Page 16: 75th Meteoritical Society Meeting, Cairns, 14 August 2012
Page 17: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

10

100

Sr Ba La Ce Nd Sm Eu Tb Dy Ho Yb Lu Hf Ta Th U

REE

sam

ple/

CI c

hond

rites

(wt.

ratio

)

30NWA 5738

BouvanteStannern Trend

Juvinas'Main Group'

(literature averages)

warm-desert alteration

Page 18: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

18

22

26

30

34

38

0 1 2 3 4 5bulk Sm (µg/g)

bulk

Sc

(µg/

g)

noncumulate cumulate

Kapoeta clast F4

NWA5738

E U C R I T E S

Nuevo Laredo trend

Stannerntrend

NWA 5738

Page 19: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

18

22

26

30

34

38

0 1 2 3 4bulk Yb (µg/g)

bulk

Sc

(µg/

g)

noncumulate cumulate

Kapoeta clast F4

NWA5738

E U C R I T E S

Stannerntrend

Nuevo Laredo trend

Page 20: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

0.0

1.0

2.0

3.0

4.0

5.0

30 40 50 60 70bulk Mg/(Mg+Fe), mol%

bulk

Sm

, µg/

g noncumulate cumulate

Kapoeta clast F4NWA5738 E U C R I T E S

Nuevo L. trend

Stannerntrend

Page 21: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

Barrat et al. (2011)BSE images of NWA 049

Page 22: 75th Meteoritical Society Meeting, Cairns, 14 August 2012
Page 23: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

SECONDARY MINERAL ASSEMBLAGES IN EUCRITESThermalmetamorphism? Fe-px Fe-ol Ca-plag Silica Chromite Troilite Zircon Apatite references

NWA 1000 Ext. low Yes Yes - - - - - - Warren

NWA 2061 Ext. low Yes Yes Yes - - - - - Barrat

NWA 5073 Ext. low Yes Yes Yes - Yes Yes - Yes Roszjar

Y-75011 Ext. low Yes Yes Yes - - - - - Barrat

Y-82202 Ext. low Yes Yes Yes - - - - - Barrat

NWA 049 Low Yes Yes Yes - - - - - Barrat

Pasamonte Low Yes Yes - - - - - - McCallum, Herd, Barrat

NWA 5738 Normal - Yes Yes Yes Yes Yes Yes? - THIS WORK

Sioux County Normal* Yes Yes Yes Yes - - - - Barrat*

Serra de Magé High (cumulate) - - - Yes - - - - Treiman

* "Despite a careful search, Fe enrichments along cracks in pyroxenes from equilibrated eucrites have not yet been observed ." Polymict breccia Sioux County is the one exception .

Page 24: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

p y r o x e n eC

a –

p l a

g

Fe–olivines

Fe–olivines

Page 25: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

p y r o x e n e

C a – p l a g

Fe–olivines

Page 26: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

p y r o x e n eC a – p l a g

chromite

C a – p l a g

Page 27: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

p y r o x e n eC a – p l a g

F e – o l i v i n e

Page 28: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

p y r o x e n e

p r i m a r y p l a g

C a – p l a g

F e – o l i v i n

e

Page 29: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

0 10 20 30 40 50 60 70 80 90 100

50

40

Ab An

primary

secondary

Or Or

20

10

30

NWA 5738

PLAGIOCLASECOMPOSITIONS

cf. Barrat et al. (2011)

Page 30: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

C a – p l a g + s i l i c a

p y r o x e n e

C a – p l a g

Page 31: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

p y r o x e n e

F e S

C a – p l a g + s i l i c a

Page 32: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

p y r o x e n e

F a – r i c h o

l i v

i n e s s

chromite

Page 33: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

p y r o x e n e

C a – p l a g ?

z i r c o n

Page 34: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

SECONDARY MINERAL ASSEMBLAGES IN EUCRITESThermalmetamorphism? Fe-px Fe-ol Ca-plag Silica Chromite Troilite Zircon Apatite references

NWA 1000 Ext. low Yes Yes - - - - - - Warren

NWA 2061 Ext. low Yes Yes Yes - - - - - Barrat

NWA 5073 Ext. low Yes Yes Yes - Yes Yes - Yes Roszjar

Y-75011 Ext. low Yes Yes Yes - - - - - Barrat

Y-82202 Ext. low Yes Yes Yes - - - - - Barrat

NWA 049 Low Yes Yes Yes - - - - - Barrat

Pasamonte Low Yes Yes - - - - - - McCallum, Herd, Barrat

NWA 5738 Normal - Yes Yes Yes Yes Yes Yes? - THIS WORK

Sioux County Normal* Yes Yes Yes Yes - - - - Barrat*

Serra de Magé High (cumulate) - - - Yes - - - - Treiman

* "Despite a careful search, Fe enrichments along cracks in pyroxenes from equilibrated eucrites have not yet been observed ." Polymict breccia Sioux County is the one exception .

Page 35: 75th Meteoritical Society Meeting, Cairns, 14 August 2012

C O N C L U S I O N SNWA 5738 is an extraordinary eucriteIts oxygen isotopes have a low, NWA-1240-like Δ17OIts primary plagioclase is extremely sodic (average An74)

The bulk composition is commensurately Na-rich also exceptionally rich in incompatible trace elements despite moderate Sc and mg ratio

... extends the Stannern trendNWA 5738 shows extensive development of secondary mineralogy: Unprecedented combination of Fe-olivine, Ca-plagioclase (etc.)

with silicain a normally equilibrated eucrite

Secondary veining probably developed when fluid (aqueous?) percolated through the rock after it had undergone some brecciation and cooling. Precipitation of new phases occurred preferentially in cracks in pyroxene, possibly b/c pyroxene provided a more reactive substrate.