Earth's Uranium and Thorium content and geoneutrinos fluxes based on enstatite chondrites

2014 ◽  
Vol 407 ◽  
pp. 1-8 ◽  
Author(s):  
Marc Javoy ◽  
Edouard Kaminski
Science ◽  
1958 ◽  
Vol 128 (3317) ◽  
pp. 204-205 ◽  
Author(s):  
W. M. SACKETT ◽  
H. A. POTRATZ ◽  
E. D. GOLDBERG
Keyword(s):  

1996 ◽  
Vol 31 (5) ◽  
pp. 647-655 ◽  
Author(s):  
Yanhong ZHANG ◽  
Derek W. G. SEARS
Keyword(s):  

2014 ◽  
Vol 130 ◽  
pp. 167-187 ◽  
Author(s):  
Camille Cartier ◽  
Tahar Hammouda ◽  
Régis Doucelance ◽  
Maud Boyet ◽  
Jean-Luc Devidal ◽  
...  

1968 ◽  
Vol 76 ◽  
pp. 1-51
Author(s):  
J Hansen

Radioactive veins containing the rare-earth minerals monazite and bastnaesite are found in tension joints in Precambrian sandstone, granite, lavas and dykes on the eastern side of the alkaline Ilímaussaq intrusion in South Greenland. The veins were formed in several phases. First, small cracks were mineralized with hematite, fluorite, quartz and radioactive material. This was followed by emplacement of brown albititic veins in which albite and opaque material predominate, green veins with a high content of ægirine, white albititic veins, carbonate veins and finally quartz veins. All the vein minerals may be coated by a late iron-manganese oxide. Most often the veins are separate, but they may also occur composite. The veins are from a few millimetres to about three metres wide; most commonly they are one to ten centimetres wide. The radioactivity is mostly due to thorium, but a few veins have a uranium content higher than that of thorium. The thorium content ranges from 60 to 4500 ppm, the uranium from 17 to 1500 ppm. The ratio thorium/uranium ranges from 0.1 to 57.2. The radioactivity is predominantly connected with pigmentary material, thorite, thorianite, monazite and bastnäsite. Other minerals identified in the vein are ægirine, acmite, albite, arfvedsonite, apatite, biotite, calcite, chlorite, eudialyte, fluorite, hematite, lithium mica, mesodialyte, microcline, neptunite, pyrite, quartz and sphalerite. The following constants were calculated from X-ray powder diagrams made with a Guinier-Hagg camera.Bastnäsite: a0 = 7.120 ± 7 x 10-3 Å; C0 = 9.77 ± 2 x 10-2 Å; c0/a0 = 1.372; V0 = 428.96 Å3. Monazite: a0 = 6.780 ± 5 x 10-3 Å; b0 = 7.025 ± 4 x 10-3 Å; C


Science ◽  
1957 ◽  
Vol 126 (3274) ◽  
pp. 612-614
Author(s):  
George L. Bate ◽  
J. R. Huizenga ◽  
Herbert A. Potratz
Keyword(s):  

2020 ◽  
Vol 6 (7) ◽  
pp. eaay7604 ◽  
Author(s):  
Martin Schiller ◽  
Martin Bizzarro ◽  
Julien Siebert

Nucleosynthetic isotope variability among solar system objects provides insights into the accretion history of terrestrial planets. We report on the nucleosynthetic Fe isotope composition (μ54Fe) of various meteorites and show that the only material matching the terrestrial composition is CI (Ivuna-type) carbonaceous chondrites, which represent the bulk solar system composition. All other meteorites, including carbonaceous, ordinary, and enstatite chondrites, record excesses in μ54Fe. This observation is inconsistent with protracted growth of Earth by stochastic collisional accretion, which predicts a μ54Fe value reflecting a mixture of the various meteorite parent bodies. Instead, our results suggest a rapid accretion and differentiation of Earth during the ~5–million year disk lifetime, when the volatile-rich CI-like material is accreted to the proto-Sun via the inner disk.


2005 ◽  
Vol 40 (6) ◽  
pp. 855-868 ◽  
Author(s):  
M. KIMURA ◽  
M. K. WEISBERG ◽  
Y. LIN ◽  
A. SUZUKI ◽  
E. OHTANI ◽  
...  

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