TY - JOUR
T1 - Variable refractory lithophile element compositions of planetary building blocks
T2 - Insights from components of enstatite chondrites
AU - Yoshizaki, Takashi
AU - Ash, Richard D.
AU - Lipella, Marc D.
AU - Yokoyama, Tetsuya
AU - McDonough, William F.
N1 - Funding Information:
We thank Roberta Rudnick and Philip Piccoli for discussions and technical assistance, Issei Narita for technical assistance, Dominik Hezel for kindly providing the ChondriteDB spreadsheet. We appreciate Conel Alexander and Kevin Righter for their helpful comments. We greatly appreciate Herbert Palme, Andreas Stracke, Dominik Hezel, and an anonymous referee for their constructive reviews, which helped improve the manuscript. We thank the associate editor Stefan Weyer for his editorial effort. We are grateful to NASA/JSC for loan of ALH 84170, ALH 84206, ALH 85119, MAC 88136 and RBT 04143, National Institute of Polar Research for ALHA77295, and the Smithsonian Institute for Allende. This work was supported by Grant-in-Aid for JSPS Research Fellow (No. JP18J20708), GP-EES Research Grant and DIARE Research Grant to TaY, JSPS KAKENHI Grant (No. 16H04081) to TeY, and NSF grant EAR1650365 to WFM.
Funding Information:
We thank Roberta Rudnick and Philip Piccoli for discussions and technical assistance, Issei Narita for technical assistance, Dominik Hezel for kindly providing the ChondriteDB spreadsheet. We appreciate Conel Alexander and Kevin Righter for their helpful comments. We greatly appreciate Herbert Palme, Andreas Stracke, Dominik Hezel, and an anonymous referee for their constructive reviews, which helped improve the manuscript. We thank the associate editor Stefan Weyer for his editorial effort. We are grateful to NASA/JSC for loan of ALH 84170, ALH 84206, ALH 85119, MAC 88136 and RBT 04143, National Institute of Polar Research for ALHA77295, and the Smithsonian Institute for Allende. This work was supported by Grant-in-Aid for JSPS Research Fellow (No. JP18J20708), GP-EES Research Grant and DIARE Research Grant to TaY, JSPS KAKENHI Grant (No. 16H04081) to TeY, and NSF grant EAR1650365 to WFM.
Publisher Copyright:
© 2021 Elsevier Ltd
PY - 2021/9/1
Y1 - 2021/9/1
N2 - Chondrites are sediments of materials left over from the earliest stage of the solar system history. Based on their undifferentiated nature and less fractionated chemical compositions, chondrites are widely considered to represent the unprocessed building blocks of the terrestrial planets and their embryos. Models of chemical composition of the terrestrial planets generally find chondritic relative abundances of refractory lithophile elements (RLE) in the bulk bodies (“constant RLE ratio rule”), based on limited variations of RLE ratios among chondritic meteorites and the solar photosphere. Here, we show that ratios of RLE, such as Nb/Ta, Zr/Hf, Sm/Nd and Al/Ti, are fractionated from the solar value in chondrules from enstatite chondrites (EC). The fractionated RLE ratios of individual EC chondrules document different chalcophile affinities of RLE under highly reducing environments and a separation of RLE-bearing sulfides from silicates before and/or during chondrule formation. In contrast, the bulk EC have solar-like RLE ratios, indicating that a physical sorting of silicates and sulfides was negligible before and during the accretion of EC parent bodies. Likewise, if the Earth's accretion was dominated by EC-like materials, as supported by multiple isotope systematics, physical sorting of silicates and sulfides in the accretionary disk did not occur. Alternatively, the Earth's precursors were high-temperature nebular condensates that formed prior to the precipitation of RLE-bearing sulfides. A lack of Ti depletion in the bulk silicate Earth, combined with similar silicate-sulfide and rutile-melt partitioning behaviors of Nb and Ti, prefers a moderately siderophile behavior of Nb as the origin of the accessible Earth's Nb depletion. Highly reduced planets that have experienced selective removal or accretion of silicates or metal/sulfide phases, such as Mercury, possibly yield fractionated, non-solar bulk RLE ratios.
AB - Chondrites are sediments of materials left over from the earliest stage of the solar system history. Based on their undifferentiated nature and less fractionated chemical compositions, chondrites are widely considered to represent the unprocessed building blocks of the terrestrial planets and their embryos. Models of chemical composition of the terrestrial planets generally find chondritic relative abundances of refractory lithophile elements (RLE) in the bulk bodies (“constant RLE ratio rule”), based on limited variations of RLE ratios among chondritic meteorites and the solar photosphere. Here, we show that ratios of RLE, such as Nb/Ta, Zr/Hf, Sm/Nd and Al/Ti, are fractionated from the solar value in chondrules from enstatite chondrites (EC). The fractionated RLE ratios of individual EC chondrules document different chalcophile affinities of RLE under highly reducing environments and a separation of RLE-bearing sulfides from silicates before and/or during chondrule formation. In contrast, the bulk EC have solar-like RLE ratios, indicating that a physical sorting of silicates and sulfides was negligible before and during the accretion of EC parent bodies. Likewise, if the Earth's accretion was dominated by EC-like materials, as supported by multiple isotope systematics, physical sorting of silicates and sulfides in the accretionary disk did not occur. Alternatively, the Earth's precursors were high-temperature nebular condensates that formed prior to the precipitation of RLE-bearing sulfides. A lack of Ti depletion in the bulk silicate Earth, combined with similar silicate-sulfide and rutile-melt partitioning behaviors of Nb and Ti, prefers a moderately siderophile behavior of Nb as the origin of the accessible Earth's Nb depletion. Highly reduced planets that have experienced selective removal or accretion of silicates or metal/sulfide phases, such as Mercury, possibly yield fractionated, non-solar bulk RLE ratios.
KW - Chemical fractionation
KW - Chondrites
KW - Earth
KW - Planets
KW - Refractory lithophile elements
UR - http://www.scopus.com/inward/record.url?scp=85108363577&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85108363577&partnerID=8YFLogxK
U2 - 10.1016/j.gca.2021.05.057
DO - 10.1016/j.gca.2021.05.057
M3 - Article
AN - SCOPUS:85108363577
SN - 0016-7037
VL - 308
SP - 173
EP - 187
JO - Geochmica et Cosmochimica Acta
JF - Geochmica et Cosmochimica Acta
ER -