GERM Reservoir Database
Development and Maintenance by the EarthRef.org Database Team

GERM Database Search Results        
Reservoir Z Element Value Median SD Low High N Unit Info Reference Source(s)
Earth 13 Al 1.8           ppm Model composition of the Earth as first noted by Ganapathy & Anders 1974.  The values are notably less for the 'cosmic' elements than that of the chondrites and eucrites which of course is to be expected, and enriched in the more terrestrial elements. Morgan et al. 1978 Ganapathy & Anders 1974
Earth 20 Ca 1.9           ppm Model composition of the Earth as first noted by Ganapathy & Anders 1974.  The values are notably less for the 'cosmic' elements than that of the chondrites and eucrites which of course is to be expected, and enriched in the more terrestrial elements. Morgan et al. 1978 Ganapathy & Anders 1974
Earth 26 Fe 35.9           ppm Model composition of the Earth as first noted by Ganapathy & Anders 1974.  The values are notably less for the 'cosmic' elements than that of the chondrites and eucrites which of course is to be expected, and enriched in the more terrestrial elements. Total Fe from FeO + Fe. Morgan et al. 1978 Ganapathy & Anders 1974
Earth 19 K 0.02           ppm Model composition of the Earth as first noted by Ganapathy & Anders 1974.  The values are notably less for the 'cosmic' elements than that of the chondrites and eucrites which of course is to be expected, and enriched in the more terrestrial elements. Morgan et al. 1978 Ganapathy & Anders 1974
Earth 12 Mg 13.2           ppm Model composition of the Earth as first noted by Ganapathy & Anders 1974.  The values are notably less for the 'cosmic' elements than that of the chondrites and eucrites which of course is to be expected, and enriched in the more terrestrial elements. Morgan et al. 1978 Ganapathy & Anders 1974
Earth 25 Mn 0.06           ppm Model composition of the Earth as first noted by Ganapathy & Anders 1974.  The values are notably less for the 'cosmic' elements than that of the chondrites and eucrites which of course is to be expected, and enriched in the more terrestrial elements. Morgan et al. 1978 Ganapathy & Anders 1974
Earth 11 Na 0.16           ppm Model composition of the Earth as first noted by Ganapathy & Anders 1974.  The values are notably less for the 'cosmic' elements than that of the chondrites and eucrites which of course is to be expected, and enriched in the more terrestrial elements. Morgan et al. 1978 Ganapathy & Anders 1974
Earth 28 Ni 2           ppm Model composition of the Earth as first noted by Ganapathy & Anders 1974.  The values are notably less for the 'cosmic' elements than that of the chondrites and eucrites which of course is to be expected, and enriched in the more terrestrial elements. Morgan et al. 1978 Ganapathy & Anders 1974
Earth 14 Si 14.3           ppm Model composition of the Earth as first noted by Ganapathy & Anders 1974.  The values are notably less for the 'cosmic' elements than that of the chondrites and eucrites which of course is to be expected, and enriched in the more terrestrial elements. Morgan et al. 1978 Ganapathy & Anders 1974
Earth 22 Ti 0.1           ppm Model composition of the Earth as first noted by Ganapathy & Anders 1974.  The values are notably less for the 'cosmic' elements than that of the chondrites and eucrites which of course is to be expected, and enriched in the more terrestrial elements. Morgan et al. 1978 Ganapathy & Anders 1974
Eucrites 13 Al 1.2           ppm Model composition of the Eucrite Parent body as found in this study (Morgan et al. 1978). These are basically just single element compositions of eucrites, which will be compared to other models that correlate to the values of Eucrites yet are representaive of similar yet different groups of material from the solar system. Morgan et al. 1978
Eucrites 20 Ca 1.3           ppm Model composition of the Eucrite Parent body as found in this study (Morgan et al. 1978). These are basically just single element compositions of eucrites, which will be compared to other models that correlate to the values of Eucrites yet are representaive of similar yet different groups of material from the solar system. Morgan et al. 1978
Eucrites 26 Fe 29.2           ppm Model composition of the Eucrite Parent body as found in this study (Morgan et al. 1978). These are basically just single element compositions of eucrites, which will be compared to other models that correlate to the values of Eucrites yet are representaive of similar yet different groups of material from the solar system. Total Fe from FeO + Fe. Morgan et al. 1978
Eucrites 19 K 0.003           ppm Model composition of the Eucrite Parent body as found in this study (Morgan et al. 1978). These are basically just single element compositions of eucrites, which will be compared to other models that correlate to the values of Eucrites yet are representaive of similar yet different groups of material from the solar system. Morgan et al. 1978
Eucrites 12 Mg 15           ppm Model composition of the Eucrite Parent body as found in this study (Morgan et al. 1978). These are basically just single element compositions of eucrites, which will be compared to other models that correlate to the values of Eucrites yet are representaive of similar yet different groups of material from the solar system. Morgan et al. 1978
Eucrites 25 Mn 0.01           ppm Model composition of the Eucrite Parent body as found in this study (Morgan et al. 1978). These are basically just single element compositions of eucrites, which will be compared to other models that correlate to the values of Eucrites yet are representaive of similar yet different groups of material from the solar system. Morgan et al. 1978
Eucrites 11 Na 0.03           ppm Model composition of the Eucrite Parent body as found in this study (Morgan et al. 1978). These are basically just single element compositions of eucrites, which will be compared to other models that correlate to the values of Eucrites yet are representaive of similar yet different groups of material from the solar system. Morgan et al. 1978
Eucrites 28 Ni 1.7           ppm Model composition of the Eucrite Parent body as found in this study (Morgan et al. 1978). These are basically just single element compositions of eucrites, which will be compared to other models that correlate to the values of Eucrites yet are representaive of similar yet different groups of material from the solar system. Morgan et al. 1978
Eucrites 14 Si 16.4           ppm Model composition of the Eucrite Parent body as found in this study (Morgan et al. 1978). These are basically just single element compositions of eucrites, which will be compared to other models that correlate to the values of Eucrites yet are representaive of similar yet different groups of material from the solar system. Morgan et al. 1978
Eucrites 22 Ti 0.07           ppm Model composition of the Eucrite Parent body as found in this study (Morgan et al. 1978). These are basically just single element compositions of eucrites, which will be compared to other models that correlate to the values of Eucrites yet are representaive of similar yet different groups of material from the solar system. Morgan et al. 1978
H Ordinary Chondrites 13 Al 1.2           ppm Model composition of H-Chondrites as found by Mason 1965.  These values correlate to those found by Morgan et al. 1978 for the Eucrite parent body, which is the norm for these types of materials (chondrites). The match is not perfect however, seeing that the H-chondrites are obviously more abundant in the involatile elements and metals due to their cosmic origins. Morgan et al. 1978 Mason 1965
H Ordinary Chondrites 20 Ca 1.3           ppm Model composition of H-Chondrites as found by Mason 1965.  These values correlate to those found by Morgan et al. 1978 for the Eucrite parent body, which is the norm for these types of materials (chondrites). The match is not perfect however, seeing that the H-chondrites are obviously more abundant in the involatile elements and metals due to their cosmic origins. Morgan et al. 1978 Mason 1965
H Ordinary Chondrites 26 Fe 27.8           ppm Model composition of H-Chondrites as found by Mason 1965.  These values correlate to those found by Morgan et al. 1978 for the Eucrite parent body, which is the norm for these types of materials (chondrites). The match is not perfect however, seeing that the H-chondrites are obviously more abundant in the involatile elements and metals due to their cosmic origins.Total Fe from FeO+ Fe. Morgan et al. 1978 Mason 1965
H Ordinary Chondrites 19 K 0.08           ppm Model composition of H-Chondrites as found by Mason 1965.  These values correlate to those found by Morgan et al. 1978 for the Eucrite parent body, which is the norm for these types of materials (chondrites). The match is not perfect however, seeing that the H-chondrites are obviously more abundant in the involatile elements and metals due to their cosmic origins. Morgan et al. 1978 Mason 1965
H Ordinary Chondrites 12 Mg 14.3           ppm Model composition of H-Chondrites as found by Mason 1965.  These values correlate to those found by Morgan et al. 1978 for the Eucrite parent body, which is the norm for these types of materials (chondrites). The match is not perfect however, seeing that the H-chondrites are obviously more abundant in the involatile elements and metals due to their cosmic origins. Morgan et al. 1978 Mason 1965
H Ordinary Chondrites 25 Mn 0.23           ppm Model composition of H-Chondrites as found by Mason 1965.  These values correlate to those found by Morgan et al. 1978 for the Eucrite parent body, which is the norm for these types of materials (chondrites). The match is not perfect however, seeing that the H-chondrites are obviously more abundant in the involatile elements and metals due to their cosmic origins. Morgan et al. 1978 Mason 1965
H Ordinary Chondrites 11 Na 0.64           ppm Model composition of H-Chondrites as found by Mason 1965.  These values correlate to those found by Morgan et al. 1978 for the Eucrite parent body, which is the norm for these types of materials (chondrites). The match is not perfect however, seeing that the H-chondrites are obviously more abundant in the involatile elements and metals due to their cosmic origins. Morgan et al. 1978 Mason 1965
H Ordinary Chondrites 28 Ni 1.6           ppm Model composition of H-Chondrites as found by Mason 1965.  These values correlate to those found by Morgan et al. 1978 for the Eucrite parent body, which is the norm for these types of materials (chondrites). The match is not perfect however, seeing that the H-chondrites are obviously more abundant in the involatile elements and metals due to their cosmic origins. Morgan et al. 1978 Mason 1965
H Ordinary Chondrites 14 Si 17.1           ppm Model composition of H-Chondrites as found by Mason 1965.  These values correlate to those found by Morgan et al. 1978 for the Eucrite parent body, which is the norm for these types of materials (chondrites). The match is not perfect however, seeing that the H-chondrites are obviously more abundant in the involatile elements and metals due to their cosmic origins. Morgan et al. 1978 Mason 1965
H Ordinary Chondrites 22 Ti 0.06           ppm Model composition of H-Chondrites as found by Mason 1965.  These values correlate to those found by Morgan et al. 1978 for the Eucrite parent body, which is the norm for these types of materials (chondrites). The match is not perfect however, seeing that the H-chondrites are obviously more abundant in the involatile elements and metals due to their cosmic origins. Morgan et al. 1978 Mason 1965
Igneous Rocks 47 Ag 3.2           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 13 Al 8.3           wt% Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Schmitt et al. 1972
Igneous Rocks 79 Au 0.23           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 83 Bi 0.36           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 35 Br 14           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 48 Cd 7.1           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 58 Ce 3.1           ppm Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Wanke & Palme 1974
Igneous Rocks 27 Co 3           ppm Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Schmitt et al. 1972
Igneous Rocks 24 Cr 1930           ppm Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Schmitt et al. 1972
Igneous Rocks 55 Cs 0.7           ppb Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Tera et al. 1970
Igneous Rocks 55 Cs 0.7           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 63 Eu 0.6           ppm Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Schnetzler & Philpotts 1969
Jerome 1970
Igneous Rocks 26 Fe 8.9           wt% Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Schmitt et al. 1972
Igneous Rocks 32 Ge 7.3           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 72 Hf 0.61           ppm Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Jerome 1970
Igneous Rocks 71 Lu 0.2           ppm Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Jerome 1970
Igneous Rocks 11 Na 3070           ppm Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Schmitt et al. 1972
Igneous Rocks 11 Na 2770           ppm Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Tera et al. 1970
Igneous Rocks 28 Ni 3.5           ppm Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 76 Os 3           ppt Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 76 Os 400           ppt Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Morgan 1965
Igneous Rocks 46 Pd 0.4           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 37 Rb 50           ppb Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Tera et al. 1970
Igneous Rocks 37 Rb 30           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 75 Re 60           ppt Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Morgan 1965
Igneous Rocks 75 Re 2.2           ppt Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 51 Sb 1.1           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 21 Sc 24           ppm Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Schmitt et al. 1972
Igneous Rocks 34 Se 500           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 62 Sm 0.9           ppm Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Schnetzler & Philpotts 1969
Jerome 1970
Igneous Rocks 52 Te 4.1           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 52 Te 150           ppb Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Clark Jr. et al. 1967
Igneous Rocks 81 Tl 0.08           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 92 U 48           ppb Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Igneous Rocks 92 U 14           ppb Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Reed & Jovanovic 1969
Igneous Rocks 92 U 25           ppb Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Fisher 1969
Igneous Rocks 92 U 20           ppb Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Morgan & Lovering 1973
Igneous Rocks 92 U 45           ppb Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Clark Jr. et al. 1967
Igneous Rocks 70 Yb 1.1           ppm Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Schnetzler & Philpotts 1969
Igneous Rocks 70 Yb 1           ppm Element abundances of Moore County eucrites as found by various other sources.  These values are used for comparison to values obtained in this study (Morgan et al. 1978) according to some form of Neutron Activation Analysis. Morgan et al. 1978 Jerome 1970
Igneous Rocks 30 Zn 1.2           ppm Major, minor and trace element abundances of eucrites from Moore County which much like the Serra de Mage is cumulate and unbrecciated. However, Moore County eucrites have less plagioclase than Serra de Mage and the plagioclase that it does have is much less calcic.  According to Hess and Henderson 1949 this eucrite resembles a terrestrial norite in bulk composition. Moore County Morgan et al. 1978
Juvinas Eucrite 47 Ag 21           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Laul et al. 1972
Juvinas Eucrite 47 Ag 100           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 13 Al 6.8           wt% Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Schmitt et al. 1972
Juvinas Eucrite 13 Al 7.1           wt% Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Juvinas Eucrite 79 Au 7.9           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Juvinas Eucrite 79 Au 7.1           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 79 Au 3.8           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Laul et al. 1972
Juvinas Eucrite 83 Bi 5           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Laul et al. 1972
Juvinas Eucrite 83 Bi 3.5           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 35 Br 160           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 35 Br 146           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Laul et al. 1972
Juvinas Eucrite 48 Cd 65           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Morgan & Lovering 1973
Juvinas Eucrite 48 Cd 29           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 58 Ce 7.1           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Schnetzler & Philpotts 1969
Juvinas Eucrite 27 Co 5.8           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Juvinas Eucrite 27 Co 4           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Schmitt et al. 1972
Juvinas Eucrite 24 Cr 2100           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Schmitt et al. 1972
Wanke et al. 1972
Juvinas Eucrite 55 Cs 8.2           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Laul et al. 1972
Juvinas Eucrite 55 Cs 5.7           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Tera et al. 1970
Juvinas Eucrite 55 Cs 5           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 63 Eu 0.7           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Schnetzler & Philpotts 1969
Juvinas Eucrite 63 Eu 0.6           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Jerome 1970
Juvinas Eucrite 26 Fe 14.5           wt% Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Juvinas Eucrite 26 Fe 12.4           wt% Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Schmitt et al. 1972
Juvinas Eucrite 32 Ge 60           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Juvinas Eucrite 32 Ge 4           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 72 Hf 1.3           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Jerome 1970
Juvinas Eucrite 77 Ir 27000           ppt Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Juvinas Eucrite 77 Ir 28           ppt Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 71 Lu 0.28           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Jerome 1970
Juvinas Eucrite 11 Na 3350           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Tera et al. 1970
Juvinas Eucrite 11 Na 2300           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Schmitt et al. 1972
Wanke et al. 1972
Juvinas Eucrite 28 Ni 1.1           ppm Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 76 Os 18           ppt Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 46 Pd 0.4           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 46 Pd 1           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Juvinas Eucrite 37 Rb 167           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Tera et al. 1970
Juvinas Eucrite 37 Rb 250           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 75 Re 9.7           ppt Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 51 Sb 42           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 21 Sc 29           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Schmitt et al. 1972
Wanke et al. 1972
Juvinas Eucrite 34 Se 77           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 14 Si 23           wt% Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Juvinas Eucrite 62 Sm 1.9           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Schnetzler & Philpotts 1969
Juvinas Eucrite 62 Sm 1.7           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Jerome 1970
Juvinas Eucrite 62 Sm 1.5           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Juvinas Eucrite 65 Tb 0.6           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Juvinas Eucrite 52 Te 10.3           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 52 Te 290           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Clark Jr. et al. 1967
Juvinas Eucrite 81 Tl 0.75           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Laul et al. 1972
Juvinas Eucrite 81 Tl 1.1           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 92 U 57           ppb Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 92 U 200           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Clark Jr. et al. 1967
Juvinas Eucrite 92 U 99           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Morgan & Lovering 1973
Juvinas Eucrite 92 U 89           ppb Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Juvinas Eucrite 70 Yb 1.7           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Schnetzler & Philpotts 1969
Jerome 1970
Juvinas Eucrite 30 Zn 2.5           ppm Major, minor and trace element abundances of the Juvinas eucrite, which is a typical brecciated sample.  Juvinas was analyzed according to various types of Neutron Activation Analysis and it was found to be compositionally similar to Ibitira eucrite. Other characteristics that define Juvinas are its mineral assemblages and oriented textures with lithic clasts several centimeters wide, and positive Eu anomalies which resembles rocks from a layered igneous intrusion.  Morgan et al. 1978
Juvinas Eucrite 30 Zn 1.1           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Wanke et al. 1972
Juvinas Eucrite 30 Zn 2.5           ppm Element concentrations for Juvinas eucrite as analyzed by various different sources.  This particular sample has been studied quite a bit, so relevant data to compare to values found by this study (Morgan et al. 1978) are in great abundance. Morgan et al. 1978 Laul et al. 1972
Moon 13 Al 5.8           ppm Model major element composition of the Moon as first noted by Ganapathy and Anders 1974. The moon is notably depleted in the alkali elements which could have been an effect of the high temperature of chondrule formation.  Morgan et al. 1978 Ganapathy & Anders 1974
Moon 20 Ca 6.4           ppm Model major element composition of the Moon as first noted by Ganapathy and Anders 1974. The moon is notably depleted in the alkali elements which could have been an effect of the high temperature of chondrule formation.  Morgan et al. 1978 Ganapathy & Anders 1974
Moon 26 Fe 9           ppm Model major element composition of the Moon as first noted by Ganapathy and Anders 1974. The moon is notably depleted in the alkali elements which could have been an effect of the high temperature of chondrule formation.  Total Fe from FeO + Fe. Morgan et al. 1978 Ganapathy & Anders 1974
Moon 19 K 0.01           ppm Model major element composition of the Moon as first noted by Ganapathy and Anders 1974. The moon is notably depleted in the alkali elements which could have been an effect of the high temperature of chondrule formation.  Morgan et al. 1978 Ganapathy & Anders 1974
Moon 12 Mg 17.4           ppm Model major element composition of the Moon as first noted by Ganapathy and Anders 1974. The moon is notably depleted in the alkali elements which could have been an effect of the high temperature of chondrule formation.  Morgan et al. 1978 Ganapathy & Anders 1974
Moon 25 Mn 0.03           ppm Model major element composition of the Moon as first noted by Ganapathy and Anders 1974. The moon is notably depleted in the alkali elements which could have been an effect of the high temperature of chondrule formation.  Morgan et al. 1978 Ganapathy & Anders 1974
Moon 11 Na 0.09           ppm Model major element composition of the Moon as first noted by Ganapathy and Anders 1974. The moon is notably depleted in the alkali elements which could have been an effect of the high temperature of chondrule formation.  Morgan et al. 1978 Ganapathy & Anders 1974
Moon 28 Ni 0.5           ppm Model major element composition of the Moon as first noted by Ganapathy and Anders 1974. The moon is notably depleted in the alkali elements which could have been an effect of the high temperature of chondrule formation.  Morgan et al. 1978 Ganapathy & Anders 1974
Moon 14 Si 18.6           ppm Model major element composition of the Moon as first noted by Ganapathy and Anders 1974. The moon is notably depleted in the alkali elements which could have been an effect of the high temperature of chondrule formation.  Morgan et al. 1978 Ganapathy & Anders 1974
Moon 22 Ti 0.34           ppm Model major element composition of the Moon as first noted by Ganapathy and Anders 1974. The moon is notably depleted in the alkali elements which could have been an effect of the high temperature of chondrule formation.  Morgan et al. 1978 Ganapathy & Anders 1974
North American Shale Composite (NASC) 47 Ag 14.2           ppb Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 13 Al 6.7           wt% Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 79 Au 0.95           ppb Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 79 Au 3.2           ppm Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 83 Bi 6.6           ppb Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 35 Br 70           ppb Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 48 Cd 30           ppb Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 58 Ce 10.8           ppm Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 27 Co 7.6           ppm Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 27 Co 14.3           ppm Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 24 Cr 2500           ppm Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 24 Cr 2100           ppm Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 55 Cs 8.5           ppb Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 63 Eu 0.7           ppm Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 63 Eu 0.7           ppm Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 26 Fe 12.9           wt% Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 26 Fe 14.1           wt% Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 32 Ge 3.5           ppb Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 72 Hf 1.1           ppm Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 77 Ir 3.9           ppt Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 71 Lu 0.42           ppm Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 71 Lu 0.37           ppm Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 11 Na 1440           ppm Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 11 Na 1370           ppm Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 28 Ni 6           ppm Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 37 Rb 125           ppb Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 75 Re 2           ppt Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 51 Sb 7.3           ppb Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 21 Sc 31.5           ppm Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 21 Sc 30           ppm Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 34 Se 80           ppb Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 14 Si 22.9           wt% Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 62 Sm 2.3           ppm Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 62 Sm 1.8           ppm Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 65 Tb 0.5           ppm Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 52 Te 0.5           ppb Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 81 Tl 0.41           ppb Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 92 U 81           ppb Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 92 U 104           ppb Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 70 Yb 1.8           ppm Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 70 Yb 1.9           ppm Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
North American Shale Composite (NASC) 30 Zn 2.7           ppm Element concentrations of the Ibitira eucrite as found by Wanke et al. 1974 which in this case is the only other source that has comparative data on this sample. Morgan et al. 1978 Wanke & Palme 1974
North American Shale Composite (NASC) 30 Zn 1.6           ppm Major, minor and trace element concentrations of eucrites from Ibitira which is a vesicular unbrecciated eucrite sample. The vesicular nature of Ibitira is possibly due to the fact that it crystallzed at a low pressure relative to other eucrites. This sample has been analyzed according to Neutron Activation using a single chip of the Ibitira sample.  Morgan et al. 1978
Sera de Mage Eucrite 47 Ag 3.3           ppb Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Laul et al. 1972
Sera de Mage Eucrite 47 Ag 1           ppb Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 13 Al 9.2           wt% Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 79 Au 1.8           ppb Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Laul et al. 1972
Sera de Mage Eucrite 79 Au 0.14           ppb Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 83 Bi 2.4           ppb Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Laul et al. 1972
Sera de Mage Eucrite 83 Bi 0.18           ppb Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 35 Br 45           ppb Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Laul et al. 1972
Sera de Mage Eucrite 35 Br 15           ppb Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 48 Cd 10           ppb Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 48 Cd 5.3           ppb Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Laul et al. 1972
Sera de Mage Eucrite 58 Ce 1.2           ppm Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Schnetzler & Philpotts 1969
Sera de Mage Eucrite 27 Co 10           ppm Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Schmitt et al. 1972
Sera de Mage Eucrite 27 Co 4.8           ppm Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 24 Cr 1740           ppm Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Schmitt et al. 1972
Sera de Mage Eucrite 24 Cr 2200           ppm Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 55 Cs 2.1           ppb Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Laul et al. 1972
Sera de Mage Eucrite 55 Cs 1           ppb Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 63 Eu 0.5           ppm Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 63 Eu 0.3           ppm Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Schnetzler & Philpotts 1969
Sera de Mage Eucrite 26 Fe 9.9           wt% Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 26 Fe 7.1           wt% Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Schmitt et al. 1972
Sera de Mage Eucrite 32 Ge 3.2           ppb Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 77 Ir 2.2           ppt Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 71 Lu 0.06           ppm Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 11 Na 3380           ppm Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Schmitt et al. 1972
Sera de Mage Eucrite 11 Na 2370           ppm Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 28 Ni 1           ppm Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 37 Rb 50           ppb Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 75 Re 0.8           ppt Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 51 Sb 0.7           ppb Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 21 Sc 14           ppm Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Schmitt et al. 1972
Sera de Mage Eucrite 21 Sc 19.2           ppm Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 34 Se 78           ppb Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Laul et al. 1972
Sera de Mage Eucrite 34 Se 105           ppb Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 14 Si 21.5           wt% Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 62 Sm 0.3           ppm Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 62 Sm 0.33           ppm Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Schnetzler & Philpotts 1969
Sera de Mage Eucrite 52 Te 1           ppb Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 81 Tl 0.03           ppb Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 81 Tl 0.12           ppb Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Laul et al. 1972
Sera de Mage Eucrite 92 U 16           ppb Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Morgan & Lovering 1973
Sera de Mage Eucrite 92 U 8.2           ppb Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
Sera de Mage Eucrite 70 Yb 0.37           ppm Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Schnetzler & Philpotts 1969
Sera de Mage Eucrite 30 Zn 0.78           ppm Element abundances of the Serra de Mage eucrite as analyzed by various different sources.  These values are placed against the values found in this study (Morgan et al. 1978) according to INAA. Morgan et al. 1978 Laul et al. 1972
Sera de Mage Eucrite 30 Zn 0.64           ppm Major, minor and trace element abundances as found in Eucrites from Serra de Mage (Brazil).  Sample analyzed by INAA at University of Oregon. Serra de Mage has a relatively high, but variable, plagioclase content as compared to other Eucrites.  The calcic nature of this plagioclase makes Serra de Mage perhaps the best meteoric analogue to lunar anorthosites and ancient terrestrial calcic anorthosites. Morgan et al. 1978
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