nucleation of the widmanstatten pattern in iron meteoritesThe Widmanstatten pattern develops at low temperatures during the evolution of the asteroids. We have studied the origin of the Widmanstatten pattern in order to obtain metallographic cooling rates in the temperature range (approx. 700 to 300 deg C). This paper summarizes our recent evaluation of the various mechanisms for the formation of the Widmanstatten pattern. All chemical groups of the iron meteorites are considered. We also propose a new mechanism for the formation of the Widmanstatten pattern in the low P metal phase of iron, stony-iron and stony meteorites. The results of this evaluation enables us to more accurately determine metallographic cooling rates particularly when incorporated with other recent advances in Fe-Ni and Fe-Ni (P saturated) phase diagrams and interdiffusion coefficients.
Yang, J. (Massachusetts Univ. Amherst, MA, United States)
Goldstein, J. I. (Massachusetts Univ. Amherst, MA, United States)
August 21, 2013
January 1, 2004
Publication: Lunar and Planetary Science XXXV: Achondrites: An Awesome Assortment
Lunar and Planetary Science and Exploration
Public Use Permitted.
IDRelationTitle20040062060Analytic PrimaryLunar and Planetary Science XXXV: Achondrites: An Awesome AssortmentDocument Inquiryvisibility_off