Literature DB >> 30547073

Experimentally determined trace element partition coefficients between hibonite, melilite, spinel, and silicate melts.

D Loroch1, S Klemme1, J Berndt1, A Rohrbach1.   

Abstract

This article provides new data on mineral/melt partitioning in systems relevant to the evolution of chondrites, Calcium Aluminum-Rich Inclusions (CAI) in chondrites and related meteorites. The data set includes experimentally determined mineral/melt partition coefficients between hibonite (CaAl12O19), melilite (Ca2(Al,Mg)2SiO7), spinel (MgAl2O4) and silicate melts for a wide range of trace elements: Sc, Ti, V, Cr, Co, Ni, Cu, Zn, Ga, Ge, Rb, Sr, Y, Zr, Nb, Rh, Cs, Ba, La, Ce, r, Nd, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, Lu, Hf, Ta, W, Pb, Th and U. The experiments were performed at high temperatures (1350 °C < T < 1550 °C) and ambient pressure. The experimental run products were analyzed using electron microprobe (EMPA) and laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS). The partition coefficients for 38 trace elements were calculated from the LA-ICP-MS data.

Entities:  

Year:  2018        PMID: 30547073      PMCID: PMC6282632          DOI: 10.1016/j.dib.2018.10.100

Source DB:  PubMed          Journal:  Data Brief        ISSN: 2352-3409


Specifications table Value of the data The new trace element partition coefficients supplement the existing database of mineral/melt partition coefficients of minerals that are frequently found in Ca- and Al-rich inclusions in chondritic meteorites. The new trace element partition coefficients between hibonite, an class="Chemical">melilite and spinel and silicate melts may be used to test whether these minerals crystallized from or equilibrated with a silicate melt or whether they condensed from a vapor phase. This partition coefficient data set is based on experiments under oxidizing conditions, since preliminary experiments under reducing conditions, which would have been more relevant to solar nebula processes, resulted in crystals which were too small to be analyzed. Our mineral/mineral partition coefficients may be used to test whether hibonite, melilite and spinel are in thermodynamic equilibrium or not.

Data

In this article, we report new experimentally determined trace element partition coefficients between hibonite (CaAl12O19), melilite (Ca2(Al,Mg)2SiO7), spinel (MgAl2O4), and silicate melts at high temperatures (Tables 3 and 4). Data were generated using high temperature experiments, which were characterized using electron microprobe and LA-ICP-MS methods (Table 1, Table 4, Table 5, Table 6).
Table 3

Mineral-melt partition coefficients including the available literature data. The 1σ represents the mean absolute standard error on the average and “n” stands for the number of analyzes that had been incorporated in the calculations for the D-values in the form of “n” of the mineral vs. “n” of the silicate melt.

Hibonite
H1-Ti2-R3
H1-Ti5-R4
H1-Ti5-R5
H2-Ti2-R2
H2-Ti2-R3
D-ValueσnD-ValueσnD-ValueσnD-ValueσnD-Valueσn
Mg1.86±0.215/62.68±0.226/62.98±0.406/60.92±0.116/61.12±0.126/6
Si0.045±0.0045/60.027±0.0035/60.031±0.0036/60.033±0.0036/60.051±0.0046/6
Ca0.29±0.015/60.31±0.016/60.28±0.016/60.34±0.016/60.32±0.016/6
Sc0.18±0.015/60.19±0.016/60.17±0.016/60.20±0.016/60.18±0.016/6
Ti0.91±0.065/60.68±0.036/60.67±0.056/61.08±0.076/61.21±0.056/6
V0.033±0.0025/60.020±0.0016/60.019±0.0016/60.044±0.0026/60.049±0.0026/6
Cr3/05.24±2.302/11/03/02.26±0.583/1
Co1.63±0.055/62.40±0.086/62.30±0.106/60.88±0.036/61.13±0.036/6
Ni1.15±0.185/61.91±0.166/61.65±0.236/60.62±0.116/60.77±0.126/6
Cu0.16±0.015/60.18±0.016/60.18±0.016/60.069±0.0036/60.12±0.016/6
Zn3.37±0.554/53.53±0.636/64.32±1.072/52.21±0.374/62.44±0.355/6
Ga2.56±0.085/61.81±0.056/61.95±0.076/61.66±0.056/62.44±0.076/6
Ge2.99±0.743/32.80±0.564/63.08±0.833/43.76±0.845/33.89±0.926/3
Rb0/60/60/60/60/6
Sr0.49±0.015/60.55±0.016/60.52±0.025/60.52±0.016/60.51±0.016/6
Y0.23±0.015/60.17±0.016/60.16±0.016/60.36±0.016/60.31±0.016/6
Zr0.20±0.015/60.19±0.016/60.16±0.016/60.28±0.016/60.25±0.016/6
Nb0.087±0.0035/60.083±0.0036/60.075±0.0036/60.20±0.016/60.19±0.016/6
Rh19.4±1.55/613.6±1.16/619.8±2.56/60/634.6±3.56/6
Cs0/04.02±2.391/11/00/11/0
Ba0.031±0.0034/60.027±0.0036/60.029±0.0035/60.025±0.0044/60.026±0.0036/6
La7.52±0.195/64.29±0.096/65.17±0.156/67.07±0.176/68.44±0.206/6
Ce4.49±0.115/62.89±0.076/63.05±0.106/65.18±0.136/65.82±0.146/6
Pr4.68±0.125/62.94±0.086/63.23±0.126/65.29±0.136/65.69±0.146/6
Nd3.97±0.125/62.52±0.076/62.69±0.106/64.60±0.146/64.75±0.146/6
Sm1.96±0.075/61.36±0.046/61.34±0.066/62.56±0.096/62.43±0.086/6
Eu1.35±0.045/60.95±0.036/60.93±0.046/61.83±0.056/61.66±0.056/6
Gd1.11±0.045/60.84±0.036/60.81±0.056/61.58±0.056/61.36±0.046/6
Tb0.65±0.025/60.50±0.016/60.48±0.026/61.00±0.036/60.83±0.036/6
Dy0.43±0.025/60.32±0.016/60.31±0.026/60.67±0.036/60.55±0.026/6
Ho0.28±0.015/60.21±0.016/60.20±0.016/60.45±0.026/60.38±0.016/6
Er0.18±0.015/60.15±0.016/60.13±0.016/60.30±0.016/60.25±0.016/6
Tm0.11±0.005/60.075±0.0026/60.077±0.0036/60.19±0.016/60.15±0.016/6
Yb0.069±0.0035/60.052±0.0026/60.050±0.0036/60.12±0.016/60.098±0.0046/6
Lu0.053±0.0025/60.036±0.0016/60.035±0.0026/60.088±0.0036/60.072±0.0036/6
Hf0.49±0.025/60.47±0.026/60.42±0.026/60.66±0.026/60.57±0.026/6
Ta0.35±0.015/60.35±0.016/60.33±0.016/60.74±0.026/60.70±0.026/6
W0.012±0.0045/60.007±0.0034/60.009±0.0024/60.053±0.0134/60.042±0.0086/6
Pb0/40/31/00/60/2
Th1.56±0.055/60.86±0.026/60.81±0.036/62.30±0.086/62.01±0.076/6
U0/60.021±0.0151/60/60.038±0.0103/60.047±0.0183/6

The D-values for melilite are directly influenced by the initial Ti concentration within the starting mixture. As far as two samples are appropriate enough to show, it could be that a higher Ti concentration is enhancing the incorporation possibilities for several elements.

The D-values for spinel are influenced by the very different starting compositions in respect to the aluminum and magnesium content between the starting mixtures H2, H3 and Mel3 (cf. Table 5)

Table 4

Mineral-mineral partition coefficients with corresponding 1σ error as the mean absolute standard error of the average.

Hibonite/Melilite
Hibonite/Spinel
Melilite/Spinel
D-ValueσD-ValueσD-Valueσ
Mg0.42±0.160.24±0.110.57±0.20
Si0.066±0.0183.37±1.4751.3±20.2
Ca0.21±0.0146.6±21.5217±100
Sc0.34±0.042.54±0.587.56±1.62
Ti0.39±0.1518.8±4.748.6±20.0
V0.14±0.035.91±4.9841.0±34.3
Cr
Co0.49±0.050.23±0.050.46±0.09
Ni0.53±0.280.052±0.0310.097±0.050
Cu0.20±0.040.16±0.040.80±0.20
Zn0.32±0.230.30±0.220.95±0.70
Ga0.45±0.050.82±0.161.82±0.34
Ge2.81±1.792.31±2.060.82±0.58
Rb2.31±1.480.89±0.830.39±0.36
Sr0.38±0.0340.1±21.6105±56
Y0.26±0.0329.9±26.1116±101
Zr0.17±0.029.79±1.6356.6±8.1
Nb0.25±0.09
Rh0.18±0.060.40±0.172.23±0.94
Cs
Ba0.14±0.052.60±1.8519.2±12.6
La0.50±0.046420±52212,915±706
Ce0.50±0.04
Pr0.48±0.04
Nd0.47±0.05
Sm0.43±0.05
Eu0.41±0.04
Gd0.42±0.05
Tb0.37±0.04
Dy0.34±0.05
Ho0.27±0.04997±8483651±3086
Er0.23±0.04287±2731247±1178
Tm0.18±0.02222±1351238±740
Yb0.15±0.02
Lu0.12±0.01103±37876±303
Hf0.40±0.13
Ta0.35±0.08
W0.073±0.066
Pb
Th0.45±0.05
U
Table 1

Major element concentrations of minerals and quenched silicate melts determined by EMPA. All values are given in wt%.

SampleMgO
Al2O3
SiO2
CaO
TiO2
wt%S.D.wt%S.D.wt%S.D.wt%S.D.wt%S.D.
Hibonite
H1-Ti2-R31.50±0.1486.8±0.10.86±0.148.33±0.101.77±0.21
H1-Ti5-R42.01±0.1385.1±0.70.64±0.138.36±0.083.16±0.41
H1-Ti5-R52.02±0.4784.9±1.60.70±0.178.39±0.063.19±0.97
H2-Ti2-R21.87±0.0685.7±0.31.22±0.128.27±0.091.84±0.05
H2-Ti2-R31.96±0.2885.5±2.01.12±0.258.29±0.142.23±0.62
H2-Ti5-R42.41±0.0783.8±0.30.90±0.198.30±0.093.61±0.16
H2-Ti5-R52.53±0.1883.6±0.80.91±0.158.34±0.073.86±0.57
H3-Ti5-R42.37±0.0684.8±0.40.81±0.118.27±0.093.57±0.10
H3-Ti5-R52.79±0.1182.7±0.90.96±0.398.39±0.104.37±0.41
Melilite
H1-Ti2-R30.175±0.03135.7±0.422.1±0.240.7±0.20.046±0.042
H3-R80.318±0.03035.1±1.421.6±0.340.9±0.2
Spinel
H2-R825.3±0.272.1±0.10.026±0.0120.021±0.004
H3-R819.7±1.178.3±1.30.034±0.0430.026±0.014
Mel3-R928.0±0.270.9±0.40.022±0.0360.014±0.0040.057±0.047
Mel3-R1128.0±0.270.5±0.90.037±0.0240.016±0.0070.081±0.028
Mel3-R1227.9±0.270.9±0.20.024±0.0320.011±0.0090.059±0.052
Silicate Melt
H1-Ti2-R30.79±0.1334.0±0.532.2±0.928.6±0.32.05±0.21
H1-Ti5-R40.71±0.0235.2±0.528.8±2.027.2±0.34.97±0.40
H1-Ti5-R50.66±0.0931.8±0.631.6±2.229.1±0.54.60±0.40
H2-Ti2-R21.41±0.1936.0±0.532.7±1.124.5±0.11.86±0.31
H2-Ti2-R31.38±0.2133.2±0.234.9±1.325.6±0.41.92±0.3
H2-Ti5-R41.81±0.2234.9±0.332.9±1.523.9±0.34.29±0.38
H2-Ti5-R51.59±0.1631.3±0.434.7±1.025.3±0.44.25±0.24
H2-R82.38±0.1736.2±0.731.3±0.828.1±0.3
H3-Ti5-R42.07±0.1235.8±0.828.2±1.226.8±0.64.23±0.33
H3-Ti5-R51.90±0.1831.2±0.836.2±1.828.8±0.14.42±0.24
H3-R81.69±0.1037.4±1.331.6±2.727.2±0.4
Mel3-R96.04±0.1219.1±2.136.1±4.136.3±3.01.02±0.15
Mel3-R115.33±0.5019.1±1.438.4±1.131.5±3.92.16±0.22
Mel3-R126.13±0.6718.9±4.338.5±5.732.2±7.12.18±0.91
Table 5

Compositions of the starting materials.

SiO2MgOAl2O3CaOTiO2MnCO3GeO2K2CO3
Material[wt%][wt%][wt%][wt%][wt%][wt%][wt%][wt%]
H128.20.8642.927.30.170.420.15
H1-Ti227.70.8442.026.81.990.170.410.15
H1-Ti526.80.8240.725.94.990.160.400.14
H231.91.8941.325.10.170.300.25
H2-Ti231.31.8540.524.61.950.170.290.25
H2-Ti530.41.8039.223.94.900.160.290.24
H329.52.1139.727.80.250.400.30
H3-Ti228.82.0638.827.12.230.240.390.29
H3-Ti528.02.0137.826.44.870.240.380.29
Mel129.96.3021.940.80.540.240.35
Mel239.611.37.5240.10.720.460.35
Mel332.98.8826.429.11.620.330.470.29
Table 6

Experimental run conditions. All samples were inserted into the furnace at 800 °C and heated to Tmax with the rate of 100 °C/h. For experiments with complex heating cycles the intermediate steps are given as well. The total duration of the experiments also includes the time for reaching Tmax and the time at Tquench.

SampleStarting MixRunHeating cycles
TmaxTimeCooling rateT1TimeHeating rateT2TimeCooling rateTquenchTotal TimePhases
[°C][h][°C/h][°C][h][°C/h][°C][h][°C/h][°C][h]
H2-Ti2-R2H2R215508------51450117.0hib, gl
H1-Ti2-R3H1R315508------11350333.5hib, mel, gl
H2-Ti2-R3H2R315508------11350333.5hib, gl
H1-Ti5-R4H1R415508------51450139.5hib, gl
H2-Ti5-R4H2R415508------51450139.5hib, gl
H3-Ti5-R4H3R415508------51450139.5hib, gl
H1-Ti5-R5H1R51550851350405014372421350305.7hib, gl
H2-Ti5-R5H2R51550851350405014372421350305.7hib, gl
H3-Ti5-R5H3R51550851350405014372421350305.7hib, gl
H2-R8H2R815501051350105014501021350140.0an, sp, gl
H3-R8H3R815501051350105014501021350140.0mel, sp, gl
Mel3-R9Mel3R915501051350105014501021200142.5mel, sp, gl
Mel3-R11Mel3R1115508------31200193.0sp, gl
Mel3-R12Mel3R1215508------31000211.0sp, gl

an = anorthite, gl = glass, hib = hibonite, mel = melilite, sp = spinel

Major element concentrations of minerals and quenched silicate melts determined by EMPA. All values are given in wt%. Trace element concentrations of minerals and quenched silicate melts determined with LA-ICP-MS. All values are given in µg/g. Mineral-melt partition coefficients including the available literature data. The 1σ represents the mean absolute standard error on the average and “n” stands for the number of analyzes that had been incorporated in the calculations for the D-values in the form of “n” of the mineral vs. “n” of the silicate melt. The D-values for melilite are directly influenced by the initial Ti concentration within the starting mixture. As far as two samples are appropriate enough to show, it could be that a higher Ti concentration is enhancing the incorporation possibilities for several elements. The D-values for spinel are influenced by the very different starting compositions in respect to the aluminum and magnesium content between the starting mixtures H2, H3 and Mel3 (cf. Table 5) Mineral-mineral partition coefficients with corresponding 1σ error as the mean absolute standard error of the average.

Experimental design, materials, and methods

Starting materials

The starting materials compositions are given in Table 5. Starting materials H1 and H2 are based on the starting materials Hib-1 and Hib-6 of Beckett and Stolper [1], our H3 is based on the HB-1 starting material of Kennedy et al. [2]; our starting materials Mel1, Mel2 and Mel3 are similar to the starting materials used by Kuehner et al. ([3], AK40), Beckett and Stolper ([1], AK80) and Lundstrom et al. (CAI-Glass, [4]). In total six different starting material mixtures were prepared from high purity oxides and carbonates. The resulting mixtures were homogenized in an agate mortar under acetone and were subsequently fused in a large Pt-crucible at 1500 °C for at least 3 h in a Linn VMK (Linn Gmbh, Eschenfelden, Germany) high temperature box furnace. The resulting silicate glasses were reground using the same agate mortar with acetone and the resulting powders were doped with 200 µg/g each of Sc, V, Cr, Co, Ni, Cu, Zn, Ga, Ge, Rb, Sr, Y, Zr, Nb, Rh, Cs, Ba, La, Ce, Pr, Nd, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, Lu, Hf, Ta, W, Pb, Th and U, using ICP-MS standard solutions (1000 µg/ml, Alfa Aesar, Germany). However, Ti was added to the hibonite starting mixtures (H1-Ti2, H1-Ti5, H2-Ti2, H2-Ti5 and H3-Ti2, H3-Ti5) using high purity TiO2 (Alfa Aesar, Germany). Compositions of the starting materials.

Experimental techniques

Experiments were conducted in a vertical tube furnaces (Gero GmbH, Neuhausen, Germany) at atmospheric pressure. We used the so-called “wire-loop technique” [5], [6], [7] where small amounts of starting material powder are mixed with an organic glue (UHU Gmbh, Flinke Flasche, Germal">any) and suspended on a 0.1 mm thick an class="Chemical">Pt wire. The loops are about 3 mm in diameter each. Using a home-made platinum wire “chandelier”, several samples could be run simultaneously. The samples were placed in the hot zone of the furnace at 800 °C. The temperature paths were designed so that the samples were first heated to temperatures well above the liquidus (i.e. 1550 °C, Tmax in Table 6), the run was left at 1550 °C (Tmax in Table 6) for at least 8–10 h, and then slowly cooled down to the final run temperature (Tquench) to equilibrate crystals with melts. Most experimental runs were performed with a single cooling ramp, whereas some experiments (H1-Ti5-R5, H2-Ti5-R5, H3-Ti5-R5, H2-R8, H3-R8, Mel3-R9; Table 6) were run with a more complex multi step cooling and heating cycle close to the liquidus temperature. In these runs the experiment was first heated to 1550 °C, then cooled to 1350 °C, left for 10–40 h, then heated with 50 °C/h to 1437 or 1450 °C (c.f. Table 6), left for a few hours, and then cooled to the final run temperature (Tquench). This technique was employed by Kennedy et al. [2] to facilitate crystal growth. However, we found no significant difference between runs with a single cooling ramp compared to the complex heating/cooling experiments. Table 6 shows that the total run time of the experiments was between 100 and 300 h. The experiments were quenched in air by rapidly removing them from the furnace. Details of all experimental parameters are given in Table 6. Experimental run conditions. All samples were inserted into the furnace at 800 °C and heated to Tmax with the rate of 100 °C/h. For experiments with complex heating cycles the intermediate steps are given as well. The total duration of the experiments also includes the time for reaching Tmax and the time at Tquench. an = anorthite, gl = glass, hib = hibonite, mel = melilite, sp = spinel The samples were mounted in epoxy resin, polished, and pre-examined using optical microscopy and a JEOL JSM-6610 LV SEM scanning electron microscope equipped with EDX system at the University of Münster. Samples that contained hibonite, melilite or spinel large enough for further chemical characterization were subsequently analyzed for major and trace elements.

Analytical techniques

Major elements analyses were performed with a JXA-8530F Hyperprobe field emission electron beam microprobe analyzer (EMPA) at the University of Münster. Operating at 15 kV acceleration voltage, a beam diameter of 3 μm and 5 nA beam current for the silicate melts and 15 nA for the minerals. We used a five WDX detector setup with two TAP crystals (Mg, Al), two PET (Ca, Si) and one LiF crystal (Ti). Natural and synthetic materials that were used for standardization are: jadeite (Na2O), kyanite (Al2O3), sanidine (K2O), Cr-diopside (Cr2O3), diopside (CaO), San Carlos olivine (MgO), fayalite (FeO), hypersthene (SiO2), rhodonite (MnO) and rutile (TiO2). A number of secondary standards (chromite, olivine, cr-diopside) were measured as unknowns to monitor external precision and accuracy. Trace elements were measured by with a ThermoFisher Element II sector field ICP-MS coupled to a Photon Machines AnalyteG2 ArF Excimer laser at the University of Münster, operating with a 4 J/cm2 laser fluency and a repetition rate of 5 Hz. A HelEx 2-volume sample cell was used which holds up to 8 one-inch diameter mounts, 6 thin sections and additional reference materials. Prior to sample analyses, the system was tuned with the NIST SRM 612 for high sensitivity, stability, and low oxide rates (232Th16O/232Th < 0.2%). Spot sizes for analysis were between 35 and 50 μm in diameter, while the 50 µm where mainly used for the silicate glasses. Total measurement time was 75 s with 40 s ablation time on the sample and 20 s on the background, the wash out delay was 15 s. The NIST 612 standard glass [8] was used as an external standard and the BIR-1G [8] and BCR-2G [8] were analyzed as unknowns over the course of this study to monitor precision and accuracy. Twelve sample measurements were bracketed by three measurements of the NIST 612 glasses. For the hibonite and melilite crystals, 43Ca was used as an internal standard, for spinel 26Mg and for the silicate melts 29Si was used internal standard element.
Subject areaEarth Sciences
More specific subject areaExperimental petrology, Geochemistry, Planetology, Planetary sciences
Type of dataTable, figure
How data was acquiredHigh-temperature furnace: Gero GmbH, Germany (University of Münster)
Scanning electron microscope (SEM) JEOL JSM-6610 LV in high vacuum mode equipped with EDX system (University of Münster)
Electron microprobe analysis (EMPA): JEOL JXA-8530F Hyperprobe equipped with a field emission gun (University of Münster)
Laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS): Thermo element sector field – ICP-MS with Photon Machines Analyte G2 laser ablation system (University of Münster)
Data formatMajor element data of minerals and quenched melts: data in .xlsx format
Trace element data of minerals and quenched melts: data in .xlsx format
Mineral/melt trace element partition coefficients: data in .xlsx format
Mineral/mineral trace element partition coefficients: data in .xlsx format
Experimental featuresHigh temperature experiments were run at high temperatures to equilibrate hibonite, melilite, and spinel, with silicate melts. The experimental run products were mounted in epoxy resins and polished using a variety of diamond pastes. The mounts were carbon coated, and major elements were analyzed using EMPA techniques. Subsequently, trace element concentrations of minerals and glasses within the samples were determined using LA-ICP-MS techniques.
Data accessibilitySupplementary materials
Table 2

Trace element concentrations of minerals and quenched silicate melts determined with LA-ICP-MS. All values are given in µg/g.

Hibonite

H1-Ti2-R3
H1-Ti5-R4
H1-Ti5-R5
H2-Ti2-R2
H2-Ti2-R3
H2-Ti5-R4
H2-Ti5-R5
µg/gS.D.µg/gS.D.µg/gS.D.µg/gS.D.µg/gS.D.µg/gS.D.µg/gS.D.
Mg13367± 251815263± 219514105± 323514245± 282217157± 325918699± 279920315± 5382
Si7058± 10083778± 6684712± 7805629± 8639282± 12725229± 8414912± 758
Ca59563± 210459749± 216559978± 217259077± 216659234± 209559349± 216759577± 2119
Sc30.6± 2.028.2± 2.128.3± 2.228.7± 2.028.3± 1.924.6± 1.925.5± 1.9
Ti11302± 141221355± 179719485± 254612899± 173614804± 112424027± 209928123± 3082
V6.26± 0.573.46± 0.473.44± 0.535.70± 0.625.98± 0.564.87± 0.593.82± 0.49
Cr29.1± 8.332.1± 9.825.0± 9.123.9± 9.027.9± 7.620.7± 9.723.8± 7.6
Co185± 9280± 16270± 21123± 6132± 7199± 12226± 13
Ni327± 85353± 51320± 76137± 44201± 55249± 41369± 126
Cu11.0± 1.111.8± 1.28.67± 1.0912.2± 1.211.5± 1.09.48± 1.167.98± 0.91
Zn13.7± 3.414.7± 4.814.7± 4.112.4± 3.512.9± 3.314.2± 4.612.1± 3.3
Ga247± 13180± 9175± 11200± 11258± 14233± 11229± 15
Ge7.31± 2.428.23± 2.847.00± 2.659.32± 2.688.04± 2.2510.7± 2.99.32± 2.32
Rbb.d.lb.d.lb.d.lb.d.lb.d.l0.93± 0.310.57± 0.18
Sr92.5± 4.094.4± 4.494.7± 5.591.8± 4.293.0± 4.194.8± 4.598.8± 4.9
Y36.7± 2.123.4± 1.425.5± 1.953.8± 3.249.0± 2.832.2± 1.930.1± 2.2
Zr27.6± 1.721.8± 1.421.1± 1.530.1± 2.028.9± 1.818.5± 1.221.0± 1.7
Nb9.63± 0.598.17± 0.558.10± 0.5820.3± 1.220.3± 1.110.2± 0.610.8± 0.7
Rh7.14± 0.744.52± 0.554.91± 0.944.25± 0.546.29± 0.697.30± 0.888.87± 1.40
Csb.d.l0.43± 0.180.41± 0.15b.d.l0.33± 0.12b.d.lb.d.l
Ba3.57± 0.752.76± 0.783.33± 0.842.84± 0.883.09± 0.752.94± 0.773.40± 0.86
La378± 16291± 11286± 14589± 26484± 20446± 18426± 23
Ce454± 19354± 15346± 19608± 27496± 21447± 19450± 23
Pr372± 15281± 13277± 18421± 18354± 15306± 15303± 15
Nd319± 16235± 12232± 16428± 23366± 19305± 15297± 20
Sm247± 14180± 10178± 13316± 20280± 16223± 12218± 18
Eu143± 7102± 5102± 7183± 9160± 8127± 6121± 8
Gd142± 8104± 7106± 11217± 13186± 11142± 10140± 11
Tb95.1± 5.167.4± 3.470.3± 5.1139± 8120± 687.9± 4.683.6± 6.1
Dy46.6± 3.331.5± 2.133.7± 3.164.8± 4.955.8± 4.039.6± 2.736.4± 3.7
Ho42.4± 2.628.7± 1.630.8± 2.458.9± 3.952.2± 3.335.9± 2.032.4± 2.9
Er15.9± 1.311.6± 0.911.6± 1.126.0± 2.122.4± 1.714.3± 1.013.8± 1.5
Tm9.56± 0.655.88± 0.386.79± 0.5515.6± 1.113.7± 0.98.38± 0.527.56± 0.72
Yb11.3± 1.07.44± 0.758.00± 0.9415.3± 1.413.9± 1.28.49± 0.847.70± 0.89
Lu7.52± 0.494.43± 0.314.91± 0.4211.8± 0.810.5± 0.76.05± 0.405.62± 0.50
Hf39.6± 2.534.2± 2.233.7± 3.162.1± 4.155.8± 3.540.4± 2.643.8± 3.7
Ta40.1± 2.235.7± 1.936.8± 2.884.6± 4.981.9± 4.445.9± 2.552.0± 3.9
W0.09± 0.060.10± 0.070.20± 0.100.28± 0.130.19± 0.090.13± 0.100.29± 0.11
Pbb.d.lb.d.l0.27± 0.11b.d.lb.d.lb.d.lb.d.l
Th131± 771.5± 3.572.3± 5.0191± 11162± 9110± 5106± 8
Ub.d.l0.01± 0.01b.d.l0.02± 0.010.01± 0.010.01± 0.010.01± 0.01

  1 in total

1.  High Temperature Evaporation and Isotopic Fractionation of K and Cu.

Authors:  Mason Neuman; Astrid Holzheid; Katharina Lodders; Bruce Fegley; Bradley L Jolliff; Piers Koefoed; Heng Chen; Kun Wang 王昆
Journal:  Geochim Cosmochim Acta       Date:  2021-10-13       Impact factor: 5.010

  1 in total

北京卡尤迪生物科技股份有限公司 © 2022-2023.