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The Population of Small Near-Earth Objects: Composition, Source Regions, and Rotational Properties

  • Authors: Juan A. Sanchez, Vishnu Reddy, Audrey Thirouin, William F. Bottke, Theodore Kareta, Mario De Florio, Benjamin N. L. Sharkey, Adam Battle, David C. Cantillo, Neil Pearson

Juan A. Sanchez et al 2024 The Planetary Science Journal 5 .

  • Provider: AAS Journals

Caption: Figure 10.

Molar contents of wollastonite (Wo) vs. ferrosilite (Fs) for NEOs 85990, 2015 BC, 2015 WF13, 2015 XC, 2016 EF28, 2017 RR15, and 2020 RO6. The error bars correspond to the values determined by Burbine et al. (2009), 3 mol% for Fs and 1 mol% for Wo. The approximate range of pyroxene chemistries for howardites, noncumulate eucrites, cumulate eucrites, and diogenites from Sanchez et al. (2013) are indicated as dashed boxes.

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