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This article explores the existence of plate tectonics during the Hadean Eon, a time period before the formation of rocks. It examines various sources of evidence, such as planetary analogues, ancient zircons, and isotopic composition, to determine if plate tectonics occurred during this early phase of Earth's history.
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Hadean plate tectonics – fact or fiction? Martin J.Whitehouse Swedish Museum of Natural History, Stockholm, Sweden Penrose, June 2006
In the absence of Hadean rocks, what can we look at ? • Planetary analogues, e.g. Mars, differentiated meteorites • Post-Hadean rock record • Super-ancient zircon, e.g. Jack Hills (the only direct sample) Sampling the Hadean Earth Penrose, June 2006
Mars – evidence for ancient (<3.9 Ga) long-lived crust Moon & differentiated meteorites (eucrites) – evidence for elevated U-Pb ratios of their surfaces (“high µ”) Planetary analogues Frey et al. 2002 Zuber et al. 2000 Penrose, June 2006
Long-term isolation of isotopic reservoirs: Pb isotopes from SW Greenland Elevated Pb isotope composition of BIF, metasediments and >3.8 Ga TTG’s at Isua require early separation of a high µ reservoir and isolation for > 500 Ma. 3.7 Ga TTG’s reflect typical depleted mantle and subduction geochemistry. Post-Hadean rock record Kramers, in press, after Kamber et al. 2003 Penrose, June 2006
Long-term isolation of isotopic reservoirs 142Nd anomaly at Isua Isua metasediments preserve a 142Nd/144Nd ratio significantly higher than bulk Earth. 146Sm has a half life of only 103 Ma, hence such anomalies require silicate Earth differentiation in the first few 100 Myr of Earth history. Preservation of the positive 142Nd anomaly in 3.7 Ga sediments requires isolation of a depleted (high Sm/Nd) reservoir from a mixing mantle Post-Hadean rock record Caro et al., 2003 Penrose, June 2006
Paucity of ancient zircon in early Archaean sediments The oldest metasediments do not contain substantially older detrital zircon (Nutman, 2001). Consistent with a predominantly basaltic and/or juvenile ancient crust with no significant old zircon source. Post-Hadean rock record Nutman, 2001 Penrose, June 2006
Solar rare gases in plume magmas 4He/3He & 21Ne/22Ne ratios in plume magmas are lower than MORB and suggest a pure solar component in the lower mantle (Earth is chondritic not solar). Solution of this paradox lies in accumulation of solar wind exposed regolith on a long-lived basaltic crust eventually tranferred to an isolated (?) deep mantle reservoir . Post-Hadean rock record Tolstikhin & Hofmann, 2005 Penrose, June 2006
Hadean zircon: U-Pb & O isotopes Oldest Jack Hills zircon indicates SiO2 rich melts existed at 4.4 Ga. Elevated δ18O of some of these grains has been used to suggest interaction with liquid water but evidence remains equivocal. Hadean detrital zircon Nemchin et al., 2005 Penrose, June 2006
Hadean zircon: Hf isotopes Jack Hills zircon indicates development of an enriched reservoir >4.4 Ga (also seen for Acasta gneisses). Enriched reservoir is no longer evident in early-mid Archean rocks. Spread may reflect differentiation of long-lived crust which disappeared at the end of the Hadean. Hadean detrital zircon Kramers, in press; data from Amelin (1999, 2000), Harrison et al. (2005) Penrose, June 2006
Transition from single to multiple plate tectonics Kamber et al., 2005 Hadean tectonic model Long-term (500 Ma) isolation of isotopic reservoirs Burial by basaltic outpouring puts hydrated crust at depth – crustal melt products yield zircon (e.g. Jack Hills) Instability ultimately dooms crust to destruction by recycling into mantle at onset of multiple plate tectonics Penrose, June 2006