187Re- 187Os Nuclear Geochronometry of Diamond Sulphide Inclusions: Constraining the Chemical Evolution of the SCLM
187Re- 187Os Nuclear Geochronometry of Diamond Sulphide Inclusions: Constraining the Chemical Evolution of the SCLM
Abstract ID#: 33194
English Abstract:
Nuclear geochronometry [1-2] is a new research field constrained by other scientific fields like cosmology, cosmochemistry and nuclear theory. It connects geochronology with nuclear astrophysics. Based upon terrestrial signatures from at least two rapid (r) neutron-capture processes [3], so-called nucleogeochronometric TPI ages are calculated by means of two-point-isochrones (TPI). Because of identified Re/Os nuclear production ratios ≈ 1 and ultra-subchondritic initial 187Os/188Os ratios, it is argued that Earth’s inner core (IC) contains isotopic signatures of a 13.78 Ga old component, as it can be found within the komatiitic basalt [5085 BasKom] (Onverwacht Group, South Africa) [4]. The other signatures are assigned to the Earth’s outer core (OC), due to at least one gravitational collapse of the old component ≈ 3.48 Ga [2]. 187Os/188Osi ratios of sulphide inclusions from eclogitic diamonds usually plot above an r-process chronometer evolution line in an 187Os/188Os evolution diagram, the eclogite field [5] showing a pronounced bulge contemporaneous with the Great Oxidation Event ≈ 2.22 Ga – 2.46 Ga. This coincides with an 187Re/188Os fractionation event ≈ 2.3 ± 0.3 Ga, constrained by TPI ages for the Ellendale (Australia) peridotitic diamond sulphide inclusions EL50 and EL23 reported in the literature [6]. Contrary to eclogitic sulphide inclusions, 187Os/188Os ratios of most peridotitic sulphide inclusions [6] plot below the r-process chronometer evolution line, pointing to significant Re losses of the r-process reservoir. From the emerging pattern it may be concluded that 187Os/188Osi ratios of eclogitic diamond sulphide inclusions between 3 Ga and 1 Ga are due to episodic mixing, mingling and fractionation of IC/OC isotopic signatures and redistribution of Re during the evolution of the SCLM. This could explain the difficulty to obtain reliable conventional model or isochrone ages for these inclusions, a problem which may be solved by means of nuclear geochronometry.
[1] Roller (2014), GSA Abstr. with Programs, 46, 323. [2] Roller (2014), Abstract S51B-4444, Fall Meeting, AGU 2014. [3] Burbidge et al. (1957) Revs. Mod. Phys. 29, 547 – 650. [4] Birck et al. (1994), EPSL 124, 139 – 148. [5] Shirey et al. (2011), Science 333, 434 – 436. [6] Smit et al. (2010) GCA 74, 3292 - 3306.
