Equilibrium Configurations of Solid Cohesionless Bodies
By K. Holsapple. 2001
143 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/131a1b59e2f721e98b95653327f691ef171a4e63
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
- Kevin J. Walsh
- Daniel J. Scheeres
- M. Brown
- C. Trujillo
- Diego Paul Sánchez Lana
- Patrick Michel
- P. Pravec
- Derek C. Richardson
In Atmospheric Science
- Kevin J. Walsh
- C. Hartzell
- Patrick Michel
- Diego Paul Sánchez Lana
- Derek C. Richardson
- Daniel J. Scheeres
- P. Pravec
- M. Swift
Citations in the corpus
- PRELIMINARY RESULTS FROM NEOWISE: AN ENHANCEMENT TO THE WIDE-FIELD INFRARED SURVEY EXPLORER FOR SOLAR SYSTEM SCIENCE (2011, background): “It is possible to search for binary systems in the WISE dataset by searching for objects with lightcurve amplitude variations &1.5 magnitudes; such objects are the most likely to be binary systems (Chandrasekhar 1969; Holsapple 2001).”
- Binary asteroid population 1. Angular momentum content (2007, background): “Holsapple (2001) calculated that ωc(40 ◦) is about 10% lower than ωc(90 ◦), so real asteroids in gravity regime (i.e., with low or zero tensile strength) have an upper limit on αL from 0.9 to 1.3 for a/b from 1.0 to 3.0.”
- Photometric Observations Constraining the Size, Shape, and Albedo of 2003 EL61, a Rapidly Rotating, Pluto-sized Object in the Kuiper Belt (2005, background): “Even a solid body of moderate strength would be significantly distorted at this high rotation rate (Holsapple 2001).”
- Spin-up of rubble-pile asteroids: Disruption, satellite formation, and equilibrium shapes (2012, methodology): “( 2005 ) , where model rubble piles covering a wide parameter space of spin and shape were evolved and then compared to the analyt - ical estimates of allowable spin and shape combinations computed in the continuum limit by Holsapple ( 2001 , 2004 ) .”
- Scaling forces to asteroid surfaces: The role of cohesion (2010, background): “The connection between Holsapple’s shear model and the current model should be explored and understood in the future, but is not addressed in detail here.”