Differentiated Planetesimals and the Parent Bodies of Chondrites

By B. Weiss, L. Elkins‐Tanton. 2013

159 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/0d317edde4dcd524f426c042476ba47932816826

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. F. DeMeo
2. Kevin J. Walsh
3. Clark R. Chapman
4. T. Burbine
5. C. Alexander
6. R. Binzel
7. R. Greenwood
8. I. Franchi

In Geophysics

1. Clark R. Chapman
2. T. Burbine
3. F. DeMeo
4. Kevin J. Walsh
5. C. Alexander
6. R. Greenwood
7. I. Franchi
8. R. Binzel

Citations in the corpus

• The Compositional Structure of the Asteroid Belt (2015, background): “Also, there is the suggestion that the CV chondrites, at least, formed in the presence of magnetic fields generated by dynamos in their planetesimal cores (Weiss and Elkins-Tanton, 2013), i.”
• Melting and differentiation of early-formed asteroids: The perspective from high precision oxygen isotope studies (2017, background): “Early, rapid planetesimal accretion may also be a problem for models invoking differentiated bodies with thick outer chondritic crusts (Elkins-Tanton et al., 2011; Weiss and Elkins-Tanton, 2013).”