Niobium-zirconium chronometry and early solar system development

Maria Schonbachler; Maria Schönbächler; Mark Rehkämper; Alex N. Halliday; Der Chuen Lee; Michèle Bourot-Denise; Brigitte Zanda; Bodo Hattendorf; Detler Günther

doi:10.1126/science.1067400

Niobium-zirconium chronometry and early solar system development

Maria Schonbachler, Maria Schönbächler, Mark Rehkämper, Alex N. Halliday, Der Chuen Lee, Michèle Bourot-Denise, Brigitte Zanda, Bodo Hattendorf, Detler Günther

Research output: Contribution to journal › Article › peer-review

Abstract

Niobium-92 (92Nb) decays to zirconium-92 (92Zr) with a half-life of 36 million years and can be used to place constraints on the site of p-process nucleosynthesis and the timing of early solar system processes. Recent results have suggested that the initial 92Nb/93Nb of the solar system was high (> 10-3). We report Nb-Zr internal isochrons for the ordinary chondrite Estacado (H6) and a clast of the mesosiderite Vaca Muerta, both of which define an initial 92Nb/93Nb ratio of ∼10-5. Therefore, the solar system appears to have started with a ratio of

Original language	English
Pages (from-to)	1705-1708
Number of pages	3
Journal	Science
Volume	295
Issue number	5560
DOIs	https://doi.org/10.1126/science.1067400
Publication status	Published - 1 Mar 2002

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title = "Niobium-zirconium chronometry and early solar system development",

abstract = "Niobium-92 (92Nb) decays to zirconium-92 (92Zr) with a half-life of 36 million years and can be used to place constraints on the site of p-process nucleosynthesis and the timing of early solar system processes. Recent results have suggested that the initial 92Nb/93Nb of the solar system was high (> 10-3). We report Nb-Zr internal isochrons for the ordinary chondrite Estacado (H6) and a clast of the mesosiderite Vaca Muerta, both of which define an initial 92Nb/93Nb ratio of ∼10-5. Therefore, the solar system appears to have started with a ratio of",

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T1 - Niobium-zirconium chronometry and early solar system development

AU - Schonbachler, Maria

AU - Schönbächler, Maria

AU - Rehkämper, Mark

AU - Halliday, Alex N.

AU - Lee, Der Chuen

AU - Bourot-Denise, Michèle

AU - Zanda, Brigitte

AU - Hattendorf, Bodo

AU - Günther, Detler

PY - 2002/3/1

Y1 - 2002/3/1

N2 - Niobium-92 (92Nb) decays to zirconium-92 (92Zr) with a half-life of 36 million years and can be used to place constraints on the site of p-process nucleosynthesis and the timing of early solar system processes. Recent results have suggested that the initial 92Nb/93Nb of the solar system was high (> 10-3). We report Nb-Zr internal isochrons for the ordinary chondrite Estacado (H6) and a clast of the mesosiderite Vaca Muerta, both of which define an initial 92Nb/93Nb ratio of ∼10-5. Therefore, the solar system appears to have started with a ratio of

AB - Niobium-92 (92Nb) decays to zirconium-92 (92Zr) with a half-life of 36 million years and can be used to place constraints on the site of p-process nucleosynthesis and the timing of early solar system processes. Recent results have suggested that the initial 92Nb/93Nb of the solar system was high (> 10-3). We report Nb-Zr internal isochrons for the ordinary chondrite Estacado (H6) and a clast of the mesosiderite Vaca Muerta, both of which define an initial 92Nb/93Nb ratio of ∼10-5. Therefore, the solar system appears to have started with a ratio of

UR - https://www.scopus.com/pages/publications/0036500597

U2 - 10.1126/science.1067400

DO - 10.1126/science.1067400

M3 - Article

SN - 0036-8075

VL - 295

SP - 1705

EP - 1708

JO - Science

JF - Science

IS - 5560

ER -

Niobium-zirconium chronometry and early solar system development

Abstract

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