Very low strengths of interplanetary meteoroids and small asteroids

By O. Popova, J. Borovička, W. Hartmann, P. Spurný, E. Gnos, I. Nemtchinov, J. Trigo‐Rodríguez. 2011

190 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/1894c2186f65bfabbd047d523f1d23b59034016f

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. S. Byrne
2. A. S. McEwen
3. Ingrid Daubar
4. C. Dundas
5. M. Kennedy
6. Diego Paul Sánchez Lana
7. B. Ivanov
8. Daniel J. Scheeres

In Atmospheric Science

1. B. Ivanov
2. Diego Paul Sánchez Lana
3. S. Byrne
4. Daniel J. Scheeres
5. C. Dundas
6. A. S. McEwen
7. M. Kennedy
8. Ingrid Daubar

Citations in the corpus

• The current martian cratering rate (2010, background): “…of secondary versus primary craters at small crater sizes (e.g. Shoemaker, 1965; McEwen et al., 2005; McEwen and Bierhaus, 2006; Hartmann, 2007; Werner et al., 2009; Robbins and Hynek, 2011; Xiao and Strom, 2012), but we now have data on a set of craters known to represent only primary impactors.”
• The strength of regolith and rubble pile asteroids (2013, background): “The meteor was observed to break up high in the atmosphere, indicating a weak body and consistent with a weakly bound rubble pile [4, 33].”