Materials Map

Discover the materials research landscape. Find experts, partners, networks.

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The Materials Map is an open tool for improving networking and interdisciplinary exchange within materials research. It enables cross-database search for cooperation and network partners and discovering of the research landscape.

The dashboard provides detailed information about the selected scientist, e.g. publications. The dashboard can be filtered and shows the relationship to co-authors in different diagrams. In addition, a link is provided to find contact information.

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Materials Map under construction

The Materials Map is still under development. In its current state, it is only based on one single data source and, thus, incomplete and contains duplicates. We are working on incorporating new open data sources like ORCID to improve the quality and the timeliness of our data. We will update Materials Map as soon as possible and kindly ask for your patience.

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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (2/2 displayed)

  • 2017The I-Xe Chronometer and its Constraints on the Accretion and Evolution of Planetesimals10citations
  • 2009Collisional modification of the acapulcoite/lodranite parent body revealed by the iodine-xenon system in lodranites10citations

Places of action

Chart of shared publication
Crowther, Sarah
2 / 2 shared
Busfield, A.
1 / 1 shared
Whitby, J. A.
1 / 2 shared
Holland, Greg
1 / 1 shared
Busemann, H.
1 / 2 shared
Chart of publication period
2017
2009

Co-Authors (by relevance)

  • Crowther, Sarah
  • Busfield, A.
  • Whitby, J. A.
  • Holland, Greg
  • Busemann, H.
OrganizationsLocationPeople

article

Collisional modification of the acapulcoite/lodranite parent body revealed by the iodine-xenon system in lodranites

  • Busfield, A.
  • Gilmour, Jamie
  • Whitby, J. A.
  • Holland, Greg
  • Crowther, Sarah
  • Busemann, H.
Abstract

The I-Xe system of three lodranites has been investigated. Samples of Gibson yielded no isochrons, and late model ages are attributed to late addition of iodine. Two metal and one silicate separate from the transitional lodranite Graves Nunataks (GRA) 95209 gave ages that are consistent with each other and with the literature I-Xe age of Acapulco feldspar. These yield a mean closure age 4.19 ± 0.53 Ma after the Shallowater enstatite reference age (4562.3 ± 0.4 Ma). Such identical I-Xe ages from distinct phases imply that the parent material underwent a period of rapid cooling, the absolute age of this event being 4558.1 ± 0.7 Ma. Such rapid cooling indicates an increase in the rate at which heat could be conducted away, requiring a significant modification of the parent body. We suggest the parent body was modified by an impact at or close to the time recorded by the I-Xe system. An age of 10.4 ± 2.3 Ma after Shallowater has been determined for one whole-rock sample of Lewis Cliff (LEW) 88280. Since the release pattern is similar to that of GRA 95209 this hints that the larger grain size of this sample may reflect slower cooling due to deeper post impact burial. © The Meteoritical Society, 2009.

Topics
  • impedance spectroscopy
  • grain
  • grain size
  • phase