Thermal alteration of asteroids: evidence from meteorites

By K. Keil. 2000

152 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/54bfb31a326c23f4b377d4d250fdd53943f7d02e

How researchers see this paper

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In Astronomy and Astrophysics

1. D. Jewitt
2. C. Agnor
3. N. Movshovitz
4. J. Castillo‐Rogez
5. E. Scott
6. E. Asphaug
7. M. Jutzi
8. M. Gaffey

In Geophysics

1. N. Movshovitz
2. J. Castillo‐Rogez
3. E. Scott
4. E. Asphaug
5. D. Jewitt
6. M. Jutzi
7. M. Gaffey
8. C. Agnor

Citations in the corpus

• Mineralogy of Asteroids (2011, background): “However, this result was consistent with the evidence that a large majority of the meteorite parent bodies experienced high temperatures and underwent at least partial differentiation (e.g., Keil, 2000).”
• THE ACTIVE ASTEROIDS (2011, background): “, 2008), which themselves reflect metamorphism to temperatures ∼800◦C to 960◦C (Keil 2000).”
• Ceres’ evolution and present state constrained by shape data (2010, background): “…hydrothermal activity in the early objects, which could have entailed hydration of the silicate phase or even driving off part the water (see also Grimm and McSween, 1989; Wilson et al., 1999; Keil, 2000; Young et al., 2003; Travis and Schubert, 2005; McCord and Sotin, 2005; Palguta et al., 2007).”
• Space weathering and the interpretation of asteroid reflectance spectra (2010, background): “, Keil, 2000), 80% of which have undergone strong heating and at least partial differentiation. The iron meteorites alone derive from at least 55 – and perhaps as many as 80 – separate parent bodies. By contrast, as noted by Rubin et al. (2008): ‘‘It is likely that the majority of the different”
• Chondrules and the Protoplanetary Disk (2011, background): “Peak temperatures: LL (Huss et al. 2006), CO ( Jones & Rubie 1991), CR (Keil 2000), CV [Allende 650◦C (Huss et al. 2006), metamorphosed CVs (Schoenbeck et al. 2006, Krot and Hutcheon 1997)], CB (this work).”
• Accretion Efficiency during Planetary Collisions (2004, background): “Finally, collisions are counted on to explain diverse aspects of the meteoritic rock record (e.g., Keil 2000).”
• Chondrule formation during planetesimal accretion (2011, background): “This agrees with radioisotopic (Bizzarro et al., 2005; Kleine et al., 2005; Lee and Halliday, 1996) and petrological (Keil, 2000) records.”