Late Accretion on the Earliest Planetesimals Revealed by the Highly Siderophile Elements

Author:

Dale Christopher W.1,Burton Kevin W.1,Greenwood Richard C.2,Gannoun Abdelmouhcine3,Wade Jonathan4,Wood Bernard J.4,Pearson D. Graham15

Affiliation:

1. Department of Earth Sciences, Durham University, Durham DH1 3LE, UK.

2. Planetary and Space Science Research Institute, Open University, Walton Hall, Milton Keynes MK7 6AA, UK.

3. Laboratoire Magmas et Volcans, OPGC, UBP, UMR 6524, 5 Rue Kessler, 63038 Clermont Ferrand Cedex, France.

4. Department of Earth Sciences, University of Oxford, Parks Road, Oxford OX1 3PR, UK.

5. Department for Earth and Atmospheric Sciences, University of Alberta, Edmonton T6G 2E3, Canada.

Abstract

Coming Late to the Planetesimal Highly siderophile (iron-loving) elements (Re, Os, Ir, Ru, Rh, Pt, Pd, and Au) must have been added to the mantles of Earth, the Moon, and Mars after their iron cores formed; otherwise the mantles would be devoid of these elements, which tend to be segregated to the core. Dale et al. (p. 72 ) report data on highly siderophile elements in rocks from different planetary bodies, including asteroid 4 Vesta and other differentiated asteroids, which are representative of the planetesimals from which the solar system planets formed. Like the larger planetary bodies, differentiated asteroids, which formed over the first few million years of the solar system, bear the evidence of the late addition of highly siderophile elements to their mantles. Thus, this process was not unique to Earth, the Moon, and Mars and happened over an extended period of time in the inner solar system.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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