Niobium-zirconium chronometry and early solar system development.

نویسندگان

  • Maria Schönbächler
  • Mark Rehkämper
  • Alex N Halliday
  • Der-Chuen Lee
  • Michèle Bourot-Denise
  • Brigitte Zanda
  • Bodo Hattendorf
  • Detlef Günther
چکیده

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 approximately 10(-5). Therefore, the solar system appears to have started with a ratio of <3 x 10(-5), which implies that Earth's initial differentiation need not have been as protracted as recently suggested.

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عنوان ژورنال:
  • Science

دوره 295 5560  شماره 

صفحات  -

تاریخ انتشار 2002