2003
DOI: 10.1016/s0009-2541(03)00202-x
|View full text |Cite
|
Sign up to set email alerts
|

Phosphate Lu–Hf geochronology

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

5
38
1

Year Published

2006
2006
2016
2016

Publication Types

Select...
3
3
2

Relationship

1
7

Authors

Journals

citations
Cited by 58 publications
(44 citation statements)
references
References 47 publications
5
38
1
Order By: Relevance
“…The mean value of the 176 Lu decay constant obtained from the analysis of these terrestrial samples (1.867 · 10 À11 a À1 ) is $4% lower than the meteorite value, and, when applied to meteorites, makes their Lu-Hf ages unacceptably old ($4.75 Ga). In contrast, the 'terrestrial' decay constant, when applied to 3.7 Ga supracrustal rocks from Isua, to 2.1 Ga old rocks from West Africa (Blichert-Toft et al, 1999), and to apatites from the Eocene Gardiner intrusion (Barfod et al, 2003), yields Lu-Hf ages that agree with ages from other isotope systems, whereas, the meteorite value results in ages that are conspicuously too young. The alternatives therefore are that either all the terrestrial values are consistently wrong or the 176 Hf isochrons defined by chondrites and eucrites are biased by an early process that acted exclusively before Earth's accretion.…”
Section: Introductionmentioning
confidence: 79%
“…The mean value of the 176 Lu decay constant obtained from the analysis of these terrestrial samples (1.867 · 10 À11 a À1 ) is $4% lower than the meteorite value, and, when applied to meteorites, makes their Lu-Hf ages unacceptably old ($4.75 Ga). In contrast, the 'terrestrial' decay constant, when applied to 3.7 Ga supracrustal rocks from Isua, to 2.1 Ga old rocks from West Africa (Blichert-Toft et al, 1999), and to apatites from the Eocene Gardiner intrusion (Barfod et al, 2003), yields Lu-Hf ages that agree with ages from other isotope systems, whereas, the meteorite value results in ages that are conspicuously too young. The alternatives therefore are that either all the terrestrial values are consistently wrong or the 176 Hf isochrons defined by chondrites and eucrites are biased by an early process that acted exclusively before Earth's accretion.…”
Section: Introductionmentioning
confidence: 79%
“…1.3). The intercept of the iso- Barfod et al 2003). Abbreviations: PLAG plagioclase; WR whole rock; CPX clinopyroxene; OPX orthopyroxene; AP apatite (AP1, AP2, AP3 indicate different analyses of apatite) chron is equal to the initial ratio, which is useful for fingerprinting magma sources and contamination.…”
Section: Mineral-whole Rock Isochronsmentioning
confidence: 99%
“…Apatite preferentially incorporates rare earth elements (REE) and contains little Hf (typically ≪1 ppm) (e.g., Fujimaki 1986). Barfod et al (2003) presented a method for the separation of Lu and Hf from apatite that allows for rapid sample processing prior to analysis by multiple collectorinductively coupled plasma-mass spectrometry (MC-ICP-MS). When applied to a sample from Upper Zone b of the Skaergaard intrusion, isotopic data from three apatite fractions and the whole rock yield an isochron with a precise Lu-Hf age of 58.28 ± 0.44 Ma (Barfod et al 2003 (Fig.…”
Section: Mineral-whole Rock Isochronsmentioning
confidence: 99%
“…The long-lived 176 Hf chronometer benefits from a large range in P/D among different minerals and a high closure temperature in silicates (e.g., Scherer et al, 2000) and apatite (Barfod et al, 2003); therefore, it is potentially precise and robust against post-crystallisation heating and shock. Unsupported 176 Hf has been observed in many meteorites however, resulting in Lu-Hf dates that are up to 300 Myr older than the Pb-Pb age of the Solar System (e.g., Blichert-Toft et al, 2002;Bizzarro et al, 2012).…”
Section: © 2017 European Association Of Geochemistrymentioning
confidence: 99%