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Asteroid Physical Properties ProbePhysical properties of asteroidal and cometary nuclei are important to measure because they are critical to understanding the origin and evolution of these objects. Since direct measurement of the physical properties of asteroid surfaces is impractical to conduct, a set of experiments to measure in-situ physical properties, including density, strength, and seismic compressional velocity, of the ground of asteroidal and cometary nuclei were conducted. Such a package of instruments may be included on an asteroid or cometary lander/sampler to measure in-situ physical properties of asteroids in the solar system. Three unconsolidated materials: Portland cement, All purpose sand, and Bedford chips, with the average grain size increasing in order (Fig. 1), are chosen to simulate the asteroid ground surfaces.
Document ID
20040062109
Acquisition Source
Johnson Space Center
Document Type
Extended Abstract
Authors
H Anita Ai
(California Institute of Technology Pasadena, United States)
Thomas J Ahrens
(California Institute of Technology Pasadena, United States)
Date Acquired
August 21, 2013
Publication Date
March 15, 2004
Publication Information
Publication: Lunar and Planetary Science XXXV: Asteroids, Meteors, Comets
Publisher: Lunar and Planetary Institute
Subject Category
Lunar and Planetary Science and Exploration
Report/Patent Number
LPSC-2004-1962
LPI-Contrib-1197
Meeting Information
Meeting: 35th Lunar and Planetary Science Conference (LPSC)
Location: Houston, TX
Country: US
Start Date: March 15, 2004
End Date: March 19, 2004
Sponsors: Lunar and Planetary Institute, National Aeronautics and Space Administration
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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