Launch of martian meteorites in oblique impacts

By N. Artemieva, B. Ivanov. 2004

187 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/8d2570ac41c4cf05fdfd2d26d90116ebf9f6f8f7

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. U. Christensen
2. B. Weiss
3. J. Gattacceca
4. S. Stanley
5. P. Rochette
6. A. S. McEwen
7. Edward B. Bierhaus
8. Julien Aubert

In Atmospheric Science

1. U. Christensen
2. J. Gattacceca
3. P. Rochette
4. A. S. McEwen
5. B. Weiss
6. Edward B. Bierhaus
7. Julien Aubert
8. P. Olson

Citations in the corpus

• THE IMPORTANCE OF SECONDARY CRATERING TO AGE CONSTRAINTS ON PLANETARY SURFACES (2006, background): “In an oblique impact, the amount of high-velocity ejecta in the downrange direction increases by an order of magnitude (Pierazzo & Melosh 2000, Artemieva & Ivanov 2004, Yamamoto et al. 2005).”
• Paleomagnetic Records of Meteorites and Early Planetesimal Differentiation (2010, background): “On the other hand, for shock pressures above ∼40 GPa, the shock-induced temperature increase (Bischoff and Stoffler 1992; Artemieva and Ivanov 2004) is usually high enough to impart a thermoremanent magnetization (TRM) to the rock during slow cooling from postshock temperatures of ∼400–1100°C.”