WALSH , K.j.

Last name: WALSH

First name: K.j.

2008 (v1)

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A steady-state model of NEA binaries formed by tidal disruption of gravitational aggregates

Walsh, K.J. Richardson, D.C.

Icarus, 193, pp. 553-566

Uploaded on: December 3, 2022
2011 (v1)

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The effect of an early planetesimal-driven migration of the giant planets on terrestrial planet formation

Walsh, K.J. Morbidelli, A.

International audience

Uploaded on: December 4, 2022
2008 (v1)

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Rotational breakup as the origin of small binary asteroids

Walsh, K.J. Richardson, D.C. Michel, P.

Nature, 454, pp. 188-191, http://dx.doi.org./10.1038/nature07078

Uploaded on: December 4, 2022
2009 (v1)

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Numerical simulations of asteroids modelled as gravitational aggregates with cohesion

Richardson, D.C. Michel, P. Walsh, K.J.

Planetary and Space Science, 57, pp. 183-192, http://dx.doi.org./10.1016/j.pss.2008.04.015

Uploaded on: December 3, 2022
2011 (v1)

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Numerical simulations of granular dynamics: I. Hard-sphere discrete element method and tests

Richardson, D.C. Walsh, K.J. Murdoch, N.

International audience

Uploaded on: December 4, 2022
September 2016 (v1)

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The geophysical environment of Bennu

Scheeres, D.J. Hesar, S.G. Tardivel, S.

International audience

Uploaded on: December 3, 2022
March 2016 (v1)

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Visible spectroscopy of the Polana–Eulalia family complex: Spectral homogeneity

Tanga, Paolo de León, J. Pinilla-Alonso, N.

International audience

Uploaded on: December 3, 2022
2021 (v1)

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Rotational states and shapes of Ryugu and Bennu: Implications for interior structure and strength

Roberts, J.H. Barnouin, O.S. Daly, M.G.

Images of asteroids (162173) Ryugu and (101955) Bennu acquired by the Hayabusa2 and OSIRIS-REx missions, respectively, reveal rocky worlds covered in rubble. These two asteroids do not have hydrostatic shapes, indicating that they possess some internal friction and/or cohesion even if they lack tensile strength. Understanding the deviation of...

Uploaded on: December 4, 2022
December 28, 2020 (v1)

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The Morphometry of Impact Craters on Bennu

Daly, R.T. Bierhaus, E. Barnouin, Olivier

Bennu is an~500-m-diameter rubble-pile asteroid that is the target of detailed study by the Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS-REx) mission. Here we use data from the OSIRIS-REx Laser Altimeter to assess depth-to-diameter ratios (d/D) of 108 impact craters larger than 10 m in...

Uploaded on: December 4, 2022

WALSH , K.j.

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