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Constraints on the Distances and Timescales of Solid Migration in the Early Solar System from Meteorite Magnetism

  • Authors: James F.J. Bryson, Benjamin P. Weiss, John B. Biersteker, Ashley J. King, and Sara S. Russell

2020 The Astrophysical Journal 896 103.

  • Provider: AAS Journals

Caption: Figure 5.

Equal area stereographic projections of the directions of (a) the LC component, (b) the MC and LT components, and (c) the HC and HT components of our subsamples. The components recovered from individual interior subsamples are shown by the gray points. The single components recovered from the fusion-crusted subsamples are shown by the light blue points. The average MC and HC directions are depicted by the black stars in (b) and (c), respectively, and the average fusion crust direction is depicted by the dark blue star in (a)–(c). The ellipses around the directions recovered from the individual subsamples are MAD values of each subsample, and the ellipses around the average values are α95 values.

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